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  <front>
    <journal-meta><journal-id journal-id-type="publisher">WES</journal-id><journal-title-group>
    <journal-title>Wind Energy Science</journal-title>
    <abbrev-journal-title abbrev-type="publisher">WES</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Wind Energ. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2366-7451</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/wes-9-203-2024</article-id><title-group><article-title>Influence of rotor blade flexibility on the near-wake behavior of the NREL 5 <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> wind turbine</article-title><alt-title>Influence of rotor blade flexibility on the near-wake behavior of the NREL 5 <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> wind turbine</alt-title>
      </title-group><?xmltex \runningtitle{Influence of rotor blade flexibility on the near-wake behavior of the NREL 5\,{$\unit{{MW}}$} wind turbine}?><?xmltex \runningauthor{L.~H\"{o}ning~et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff3">
          <name><surname>Höning</surname><given-names>Leo</given-names></name>
          <email>leo.hoening@iwes.fraunhofer.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Lukassen</surname><given-names>Laura J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Stoevesandt</surname><given-names>Bernhard</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6626-1084</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Herráez</surname><given-names>Iván</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Physics, Carl von Ossietzky University Oldenburg, Küpkersweg 70, 26129 Oldenburg, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>ForWind, Institute of Physics, Carl von Ossietzky University Oldenburg, Küpkersweg 70, <?xmltex \hack{\break}?>26129 Oldenburg, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Aerodynamics and Numerical Wind Energy Meteorology, Fraunhofer Institute for Wind Energy Systems – Fraunhofer IWES, Küpkersweg 70, 26129 Oldenburg, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Laboratory for Wind and Solar Energy, University of Applied Sciences Emden/Leer, <?xmltex \hack{\break}?>Constantiapl. 4, 26723 Emden, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Leo Höning (leo.hoening@iwes.fraunhofer.de)</corresp></author-notes><pub-date><day>22</day><month>January</month><year>2024</year></pub-date>
      
      <volume>9</volume>
      <issue>1</issue>
      <fpage>203</fpage><lpage>218</lpage>
      <history>
        <date date-type="received"><day>11</day><month>July</month><year>2023</year></date>
           <date date-type="accepted"><day>28</day><month>November</month><year>2023</year></date>
           <date date-type="rev-recd"><day>25</day><month>November</month><year>2023</year></date>
           <date date-type="rev-request"><day>18</day><month>August</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2024 </copyright-statement>
        <copyright-year>2024</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://wes.copernicus.org/articles/.html">This article is available from https://wes.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://wes.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://wes.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e148">High-fidelity computational fluid dynamics (CFD) simulations of the National Renewable Energy Laboratory (NREL) 5 <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> wind turbine rotor are performed, comparing the aerodynamic behavior of flexible and rigid blades with respect to local blade quantities as well as the wake properties. The main focus has been set on rotational periodic quantities of blade loading and fluid velocity magnitudes in relation with the blade tip vortex trajectories describing the development of those quantities in the near wake. The results show that the turbine loading in a quasi-steady flow field is mainly influenced by blade deflections due to gravitation. Deforming blades change the aerodynamic behavior, which in turn influences the surrounding flow field, leading to non-uniform wake characteristics with respect to speed and shape.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e168">Since renewable energies have gained increasing attention in the context of global warming, the wind energy industry has grown considerably over the last decades, even though the growth should be even larger to reach the climate goals <xref ref-type="bibr" rid="bib1.bibx39" id="paren.1"/>.  In this context, the ever-increasing demand of energy, the urgency of replacing fossil resources and the economic demand for low prices in a highly competitive energy market lead to growing rotor sizes <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx5" id="paren.2"/>. Larger rotors allow for higher energy output and a reduction of the levelized cost of energy.  On the other hand, increasing rotor diameters along with mass restrictions forces the blade structures to become slender, which is accompanied by more flexibility and, thus, larger deformations of the blade due to wind loads. While blade flexibility has little effect on the overall rotor performance for smaller wind turbine rotors, aeroelasticity has significant effects on multi-megawatt turbines with long and slender blades <xref ref-type="bibr" rid="bib1.bibx26" id="paren.3"/>. Instabilities like vortex-induced vibrations or flutter occur with an increased probability and therefore gained increasing research interest over the last years <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx10 bib1.bibx13 bib1.bibx20" id="paren.4"/>. These highly unsteady phenomena need to be investigated further to ensure a prevention of unwanted blade vibrations. In this context, this work is intended to contribute to the basic understanding of deforming wind turbine blades.</p>
      <p id="d1e183">Most wind turbine design tools are based on computationally efficient engineering tools using low-fidelity blade element momentum (BEM) theory models. Low-fidelity models are often based on smaller, more rigid turbines and need to be corrected towards dynamic flow phenomena like dynamic stall for a rapidly changing angle of attack, 3D effects near the blade root, and tip or skewed wakes for more flexible cases <xref ref-type="bibr" rid="bib1.bibx28" id="paren.5"/>. In order to gain more reliable results, high-fidelity fluid-structure interaction (FSI) tools that<?pagebreak page204?> couple computational fluid dynamics (CFD) with computational structural dynamics (CSD) models have been recently receiving increasing attention.</p>
      <p id="d1e189">Several studies have investigated the difference between rigid and flexible rotors with respect to aerodynamic loads. <xref ref-type="bibr" rid="bib1.bibx40" id="text.6"/> showed that the aeroelastic deformation of the National Renewable Energy Laboratory (NREL) 5 <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> wind turbine, which has a rotor diameter of 126 <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>, results in a reduction of aerodynamic loads mainly due to torsional deformation. The non-linear Euler–Bernoulli beam, which was used in that study, was coupled to their in-house incompressible fluid solver once per revolution.  Similar findings were made by <xref ref-type="bibr" rid="bib1.bibx4" id="text.7"/>, where the same rotor was simulated with OpenFOAM using a finite element method (FEM) based on a non-linear geometrically exact beam theory (GEBT) implementation including a loose coupling once per time step between the structure and the flow field that is calculated solving the unsteady Reynolds-averaged Navier–Stokes (URANS) equations, neglecting the influence of gravity. This study showed that the averaged aerodynamic power output is reduced due to two reasons. On the one hand, the blades are bending towards a smaller rotor diameter, which results in less area to extract energy from, and on the other hand, due to the twisting of the blades towards lower angles of attack (AoAs), which leads to a lower lift-to-drag ratio.  This reduction of AoA due to the torsional deformation was also shown by <xref ref-type="bibr" rid="bib1.bibx19" id="text.8"/> for a floating setup under surge motion making use of OpenFOAM coupled to the multi-body dynamic solver MBDyn. <xref ref-type="bibr" rid="bib1.bibx7" id="text.9"/> simulated a pre-bent 80 <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> diameter turbine in turbulent inflow using the CFD code FLOWer, showing an increase in rotor torque for the flexible blades due to the bending resulting in an increasing AoA and a deformation towards a larger rotor disk area. The opposing behavior in these studies can be explained by the different structural models of the underlying turbines. However, these findings have not been related to effects in the respective wind turbine rotor wakes yet.</p>
      <p id="d1e229">Besides the aerodynamic loading, wind turbine blades are influenced by gravity and centrifugal forces, which bend the blades independently of the aerodynamic forces. The influence of these forces is expected to be growing with increasing rotor sizes and the naturally accompanying flexibility of the structures. While the centrifugal force is expected to be constant in time for a constant rotational speed of the rotor and tends to straighten the blade in radial direction, the gravity force has a 1P blade passing frequency, with its direction depending on the azimuthal position. This leads to a dynamic blade deformation behavior as a result of the gravitational loading in contrast to the almost constant influence of the centrifugal force.  Despite its influence on deformation and loading, <xref ref-type="bibr" rid="bib1.bibx31" id="text.10"/> concluded that the gravitational impact on the total power output of a generic 10 <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> wind turbine is negligible. The influence of gravitation on the turbine wake has not been investigated in detail yet, but it is important to understand the influence of blade flexibility in the context of wind farm layouts, where the wake of a turbine in the first row affects the inflow of turbines in the second row.</p>
      <p id="d1e244">Comparisons between wakes of rigidly and flexibly modeled rotors have been studied for differently sized rotor blades. Under complex flow situations, i.e., sheared and yawed inflow, <xref ref-type="bibr" rid="bib1.bibx6" id="text.11"/> showed that little differences are visible in the wake of a 2.3 <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> rotor using URANS in the incompressible Navier–Stokes solver EllipSys3D. <xref ref-type="bibr" rid="bib1.bibx18" id="text.12"/> simulated the NREL 5 <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> rotor coupled to a multi-body dynamics solver and investigated local aerodynamic behavior under turbulent inflow. Under these complex conditions they concluded that on the scale of the turbine diameter, turbulence has a larger influence on the wake of a rotor than the flexibility of blades. However, smaller scales in wake regions closer to the rotor have not been investigated yet. Those are important, since the way the fluid is interacting with a wind turbine determines its characteristics further downstream.</p>
      <p id="d1e269">On the other hand, small-scale numerical investigations of the rotor near-wake expansions have been performed making use of Navier–Stokes actuator disk (AD), actuator line (AL) approaches, and 3D vortex panel methods <xref ref-type="bibr" rid="bib1.bibx22" id="paren.13"/> or body fitted rigid Reynolds-averaged Navier–Stokes simulations (RANS) <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx11" id="paren.14"/>. <xref ref-type="bibr" rid="bib1.bibx12" id="text.15"/> investigated the stability of a wind turbine tip vortex making use of large eddy simulations (LES) and an AL approach.  Whilst AD/AL methods are limited to engineering corrections and small turbine RANS simulations assume the blades to be rigid, a coupled FSI investigation regarding the near-wake expansion has not been performed according to the authors' knowledge.</p>
      <p id="d1e281">Based on these findings, the objective of this study is to investigate the effects of blade flexibility and gravitational loading on the blade aerodynamic forces of an averaged-sized MW turbine as well as their impact on the near-wake behavior, i.e., wake velocity deficits and blade tip vortex trajectories. The rotor is investigated under rated operating conditions in uniform inflow perpendicular to the rotor plane. Although this setup is supposed to reflect optimal rotor blade behavior, we will show that in this baseline case already differences can be seen in the flow of rigid and flexible blades resulting in non-uniform wake behavior for flexible blades. It is assumed that these results are superimposed by even more influences under off-rated conditions. The aerodynamic findings in the rotor plane are linked towards near-wake effects, highlighting the differences of the tip vortex trajectories and wake velocity deficits of rigid and flexible blades. In this paper we investigate the characteristic aerodynamic parameters that are necessary for analyzing the near-wake development. This can be of interest for wind farm studies.</p>
      <p id="d1e284">In Sect. <xref ref-type="sec" rid="Ch1.S2"/> the numerical setup including the solvers and post-processing methodologies is described. The results of the simulated cases focusing on aerodynamic<?pagebreak page205?> characterization of rigid and flexible blades and turbine wake behavior are discussed in Sect. <xref ref-type="sec" rid="Ch1.S3"/>. Finally, a conclusion is given in Sect. <xref ref-type="sec" rid="Ch1.S4"/>, recapitulating the results and giving an outlook for future investigations.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Numerical methods and setup</title>
      <p id="d1e301">In order to study the impact of structural flexibility on the aerodynamic behavior, simulations of the NREL 5 <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> generic reference wind turbine <xref ref-type="bibr" rid="bib1.bibx17" id="paren.16"/> are performed. With a rotor diameter of 126 <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>, it can be considered an averaged-sized wind turbine in comparison to currently installed wind turbines <xref ref-type="bibr" rid="bib1.bibx37" id="paren.17"/>. Additionally, several studies of coupled CFD–CSD simulations on that specific turbine were performed <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx18 bib1.bibx19" id="paren.18"/> that can be taken into account for comparison purposes. This is important, since for a generic wind turbine no measurement campaigns have been conducted that simulations could be compared to.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Numerical discretization schemes and solver setup</title>
      <p id="d1e336">Simulations are performed using open-source software <xref ref-type="bibr" rid="bib1.bibx24" id="text.19"/>, where the incompressible, transient flow solver <italic>pimpleDyMFoam</italic> is coupled to the in-house non-linear structural finite element beam solver BeamFOAM <xref ref-type="bibr" rid="bib1.bibx3" id="paren.20"/>.  The structural beam implementation makes use of the finite element GEBT formulation that was originally proposed by <xref ref-type="bibr" rid="bib1.bibx30" id="text.21"/> and <xref ref-type="bibr" rid="bib1.bibx35" id="text.22"/> and is capable of resolving large deformations of wind turbine blades. Within this study, 49 iso-parametric beam elements per blade are used corresponding to the generic NREL design, each consisting of two nodes with 6 degrees of freedom. Each beam accounts for gyroscopic effects and stiffening due to centrifugal forces. The temporal integration made use of the second-order generalized-<inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> scheme <xref ref-type="bibr" rid="bib1.bibx2" id="paren.23"/>. The coupling of fluid and structure is embedded inside the OpenFOAM framework without the necessity of external code communication and operates in a so-called loose coupling manner, which means that information is exchanged once per time step.</p>
      <p id="d1e365">The incompressible, transient flow is simulated using the hybrid Spalart–Allmaras delayed detached eddy simulation method <xref ref-type="bibr" rid="bib1.bibx36" id="paren.24"/>. To advance the solution in time, a second-order implicit backward method was used. The spatial discretization makes use of a second-order accurate Gauss linear scheme for the gradient terms and a first-order Gauss upwind scheme for the divergence terms. The rotation of the blades is accounted for by using sliding mesh interfaces between the three blade grids, the rotor disk and the farfield grid.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Case setup</title>
      <p id="d1e380">This work focuses on the blade flexibility; therefore the complexity of the setup is reduced. The inflow is uniform and perpendicular to the rotor plane. The rotor is neither coned nor tilted, which leads to symmetric inflow conditions. The tower and nacelle are not modeled either, and the blades are extruded at the blade roots towards the center of rotation to compose a closed hub region of the three cylindrical structures. Rotor operation is set towards rated conditions. All settings are listed in Table <xref ref-type="table" rid="Ch1.T1"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e388">Overview of the main rotor characteristics of the NREL 5 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> reference turbine and the investigated conditions.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">Value</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Rated aerodynamic power</oasis:entry>
         <oasis:entry colname="col2">5.3 <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Number of rotor blades</oasis:entry>
         <oasis:entry colname="col2">3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Blade length/rotor diameter</oasis:entry>
         <oasis:entry colname="col2">61.5/126 <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Rated wind speed (<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">11.4 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Rated rotational speed</oasis:entry>
         <oasis:entry colname="col2">12.1 <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">RPM</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Blade pre-cone angle</oasis:entry>
         <oasis:entry colname="col2">0<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Rotor tilt angle</oasis:entry>
         <oasis:entry colname="col2">0<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Blade mass</oasis:entry>
         <oasis:entry colname="col2">17 740 <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">kg</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e570">Overview of the initial and boundary conditions for the inlet, outlet and internal field of all simulated cases.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">Inlet</oasis:entry>
         <oasis:entry colname="col3">Outlet</oasis:entry>
         <oasis:entry colname="col4">Free-stream initial</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">conditions</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Velocity [<inline-formula><mml:math id="M22" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>]</oasis:entry>
         <oasis:entry colname="col2">11.4 (Dirichlet)</oasis:entry>
         <oasis:entry colname="col3">Neumann</oasis:entry>
         <oasis:entry colname="col4">11.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Pressure [<inline-formula><mml:math id="M23" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pa</mml:mi></mml:mrow></mml:math></inline-formula>]</oasis:entry>
         <oasis:entry colname="col2">Neumann</oasis:entry>
         <oasis:entry colname="col3">0.0 (Dirichlet)</oasis:entry>
         <oasis:entry colname="col4">0.0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Modified turbulent viscosity <inline-formula><mml:math id="M24" display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">ν</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:math></inline-formula> [<inline-formula><mml:math id="M25" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>]</oasis:entry>
         <oasis:entry colname="col2">4.5 <inline-formula><mml:math id="M26" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Dirichlet)</oasis:entry>
         <oasis:entry colname="col3">Neumann</oasis:entry>
         <oasis:entry colname="col4">4.5 <inline-formula><mml:math id="M28" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Turbulent eddy viscosity <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ν</mml:mi><mml:mi mathvariant="normal">t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> [<inline-formula><mml:math id="M31" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>]</oasis:entry>
         <oasis:entry colname="col2">3 <inline-formula><mml:math id="M32" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Dirichlet)</oasis:entry>
         <oasis:entry colname="col3">Neumann</oasis:entry>
         <oasis:entry colname="col4">3 <inline-formula><mml:math id="M34" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{2}?></table-wrap>

      <p id="d1e841">The boundary conditions of the rectangular domain are shown in Table <xref ref-type="table" rid="Ch1.T2"/>. All sides are modeled as slip walls. The values of the turbulent quantities are set for laminar flow at the inlet. Fully turbulent conditions are assumed in the boundary layer on the blade surface.</p>
      <p id="d1e846">In order to investigate the influence of flexibility of the blades on the aerodynamic behavior and near-wake effects, three simulations are performed: one with rigid blades (called rigid case in the following), one with flexible blades (called flexible case), and one with flexible blades excluding gravity effects (flexible-noG case).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Numerical grid</title>
      <p id="d1e857">The numerical grid for all simulations is based on the numerical grid used by <xref ref-type="bibr" rid="bib1.bibx3" id="text.25"/>. They showed that a reasonable convergence for investigating aerodynamic effects taking into account fluid-structure interactions was reached for a mesh consisting of 36.38 million cells. This mesh was called the medium-sized mesh and is composed of five mesh parts, namely three blade meshes, a farfield and a rotor mesh.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e865">Mesh specifications: <bold>(a)</bold> the overall domain size and shape, <bold>(b)</bold> blade tip ring refinement zone and size, and <bold>(c)</bold> mesh resolution in the boundary layer at <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f01.png"/>

        </fig>

      <p id="d1e899">The blade meshes were created using the BladeBlockMesher utility <xref ref-type="bibr" rid="bib1.bibx25" id="paren.26"/>, which composes 2D sectional meshes into a 3D structured blade volume mesh, consisting only of hexahedral cells. The blade meshes are generated with a resolution of 260 cells in spanwise direction. The chordwise component contains 300 cells, and 40 cells are distributed in blade normal direction. The cells normal to the surface follows a ratio of 1.2, and in order to limit the computational costs and to circumvent high aspect ratio<?pagebreak page206?> cells inside the boundary layer, an adaptive wall function is applied (Fig. <xref ref-type="fig" rid="Ch1.F1"/>c). This wall function is capable of blending automatically between a high-Re and a low-Re approach, depending on the local <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msup><mml:mi>y</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> value. For the majority of the cells inside the first layer, a <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi>y</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> value between 30 and 70 is applied. Here, the wall function ensures a consistent turbulent viscosity profile for all simulated walls. In situations with low velocities close to the blades and smaller <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msup><mml:mi>y</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> values, the wall function is switched off automatically to increase accuracy for, for example, flow separation.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e944">Number of cells in different mesh regions, comparing the baseline medium mesh of the former study described in <xref ref-type="bibr" rid="bib1.bibx4" id="text.27"/> with the tip-refined mesh used within this work.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Mesh</oasis:entry>
         <oasis:entry colname="col2">Blade mesh</oasis:entry>
         <oasis:entry colname="col3">Rotor mesh</oasis:entry>
         <oasis:entry colname="col4">Farfield mesh</oasis:entry>
         <oasis:entry colname="col5">Total</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">cells</oasis:entry>
         <oasis:entry colname="col3">cells</oasis:entry>
         <oasis:entry colname="col4">cells</oasis:entry>
         <oasis:entry colname="col5">cells</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M40" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M42" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M44" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M46" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Medium <xref ref-type="bibr" rid="bib1.bibx4" id="paren.28"/></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">3.56</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">7.23</oasis:entry>
         <oasis:entry colname="col4">18.47</oasis:entry>
         <oasis:entry colname="col5">36.38</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Tip-refined mesh used in this study</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">3.56</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">13.11</oasis:entry>
         <oasis:entry colname="col4">59.93</oasis:entry>
         <oasis:entry colname="col5">73.05</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{3}?></table-wrap>

      <p id="d1e1138">The domain measures 5 rotor diameters (<inline-formula><mml:math id="M50" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>) upstream and <inline-formula><mml:math id="M51" display="inline"><mml:mn mathvariant="normal">15</mml:mn></mml:math></inline-formula> D downstream of the rotor plane. All sides are located <inline-formula><mml:math id="M52" display="inline"><mml:mn mathvariant="normal">3.5</mml:mn></mml:math></inline-formula> D from the rotational center (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a). The overall domain setup was kept, but as this study highlights the behavior of the tip vortex trajectory, additional mesh refinement was introduced in the wake of the blade tips to ensure a proper resolution of the flow in that region. This refinement is accounted for using a ring-shaped zone downstream of the blade tips, as shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b. As shown in the literature <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx21 bib1.bibx11 bib1.bibx22" id="paren.29"/>, the trajectory of the tip vortex is expected to have a characteristic inboard motion on the order of 1 %–2 % of blade length. This movement needs to be captured properly. With the level of refinement used in this study, we ensure a minimum of seven cells within this scale. The highest resolution is located around the blade tip, where the vortex and blade surface are closest. Since the trajectory of the tip vortex is part of both the rotor mesh and the farfield mesh, both grid regions are equipped with an increased number of cells, leading to a total grid size of 73.05 million cells. This already doubles the numerical costs of the medium case mesh. The total number of cells and their distribution after the refinements is shown in Table <xref ref-type="table" rid="Ch1.T3"/>. In contrast to <xref ref-type="bibr" rid="bib1.bibx4" id="text.30"/>, the setup used here allows very detailed vortex core tracking in the vicinity of the blade tip. An even higher cell refinement would exceed 100 million cells and would not be manageable by the used infrastructure.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Mesh deformation algorithm</title>
      <p id="d1e1184">To account for blade deformations inside the CFD domain, a mesh update algorithm developed by <xref ref-type="bibr" rid="bib1.bibx3" id="text.31"/> was used. This method aims at providing a cost-efficient and robust algorithm specifically developed for wind turbine simulations in OpenFOAM. Here, new mesh point coordinates are calculated in each time step without the need to solve a set of equations, where the deformation calculation costs are similar to those of a rigid mesh rotation. Within this method, all mesh volume cells surrounding the blade, as well as the blade surface cells, are projected onto the moving blade beam<?pagebreak page207?> using a Newton algorithm. Each cell is assigned to a specific beam element to account for the respective blade deformation magnitude. All mesh cells are assigned into one of three mesh regions that are differently affected by the blade deformation. The closest region surrounding the blade surface moves rigidly with the blade, making sure no boundary layer cells are deformed during the process. Between the rigidly moved mesh region and the outer fixed zone, a polynomial of selectable order smooths out the blade mesh motion. Within this study, a first-order polynomial is used. All cells outside of this transition region are not affected by any deformation.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Aerodynamic data extraction</title>
      <p id="d1e1198">The wake induction is extracted from the CFD simulation using the in-house “3-point” method first introduced by <xref ref-type="bibr" rid="bib1.bibx27" id="text.32"/>. This method gives the opportunity to account for unsteady blade deformations and non-symmetric inflows for all azimuthal positions. Other aerodynamic quantities, i.e., angle of attack (AoA), lift and drag coefficients, on the rotor blades are derived from the obtained induction factors and the calculated pressure distribution, as well as the viscous forces. This method uses six points, three points on the pressure and three points on the suction side, which are distributed parallel to the chord of each analyzed blade section. The distance of the points towards the local chord is kept constant, to account for blade deformation during the simulation. These points are used to interpolate a representative AoA and local induced velocity while excluding effects of bound circulation as well as reducing the up- and downwash of the blade. This method gives the possibility to account for dynamic effects like yaw misalignment, different azimuth positions and deforming blades also close to the blade root and tip, which is considered important for the investigation of blade tip vortex trajectories. Since the aerodynamic quantities are based on probing locations inside the fluid domain, the results are influenced by vortices trailing from the blade surface. Therefore, the resulting quantities at the tip are to be considered a qualitative estimate to assess the aerodynamic behavior for a relative comparison between different blade setups.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Simulations framework</title>
      <p id="d1e1213">Simulations are performed on the EDDY high-performance computing cluster of the University of Oldenburg <xref ref-type="bibr" rid="bib1.bibx14" id="paren.33"/>. A total of 480 computing cores are used in each simulation run, computing a total of 220 <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">s</mml:mi></mml:mrow></mml:math></inline-formula>, i.e., 44 full rotor rotations. One simulation run took about 25 <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula>, with less than 1 % more computational effort for the flexible case setup in comparison to the rigid calculation. Simulation results were extracted from the last full rotor rotation if not stated differently.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
      <p id="d1e1244">In the following, the three simulation cases, i.e., rigid, flexible and flexible-noG, are investigated in more detail, highlighting their respective impact on the aerodynamic rotor blade behavior, and they connect these findings with the characteristics of the flow in the wake of the rotor.  The effect of flexibility and gravitation on the aerodynamic performance at the rotor blades is studied in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>. The resulting effects on the near wake, i.e., velocity induction and tip vortex trajectory, are shown in Sects. <xref ref-type="sec" rid="Ch1.S3.SS2"/> and <xref ref-type="sec" rid="Ch1.S3.SS3"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T4" specific-use="star"><?xmltex \currentcnt{4}?><label>Table 4</label><caption><p id="d1e1256">Rotationally averaged thrust and power results for rigid and flexible setups (<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula> simulation contains precone, tilt and tower; <inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> simulations contain pre-cone).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Simulation</oasis:entry>
         <oasis:entry colname="col2">Model</oasis:entry>
         <oasis:entry colname="col3">Thrust</oasis:entry>
         <oasis:entry colname="col4">Power</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">[<inline-formula><mml:math id="M57" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">kN</mml:mi></mml:mrow></mml:math></inline-formula>]</oasis:entry>
         <oasis:entry colname="col4">[<inline-formula><mml:math id="M58" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula>]</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Current work (rigid)</oasis:entry>
         <oasis:entry colname="col2">Spalart–Allmaras DDES</oasis:entry>
         <oasis:entry colname="col3">757.8</oasis:entry>
         <oasis:entry colname="col4">5.45</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="bibr" rid="bib1.bibx4" id="text.34"/> (rigid)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M59" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M60" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>-SST URANS</oasis:entry>
         <oasis:entry colname="col3">761.7</oasis:entry>
         <oasis:entry colname="col4">5.51</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="bibr" rid="bib1.bibx18" id="text.35"/> (rigid)<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M62" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M63" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>-SST DDES</oasis:entry>
         <oasis:entry colname="col3">758.7</oasis:entry>
         <oasis:entry colname="col4">5.41</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="bibr" rid="bib1.bibx15" id="text.36"/>  (rigid)<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M65" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M66" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>-SST RANS</oasis:entry>
         <oasis:entry colname="col3">780</oasis:entry>
         <oasis:entry colname="col4">5.54</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Current work (flexible)</oasis:entry>
         <oasis:entry colname="col2">Spalart–Allmaras DDES</oasis:entry>
         <oasis:entry colname="col3">759.2</oasis:entry>
         <oasis:entry colname="col4">5.43</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Current work (flexible-noG)</oasis:entry>
         <oasis:entry colname="col2">Spalart–Allmaras DDES</oasis:entry>
         <oasis:entry colname="col3">760.0</oasis:entry>
         <oasis:entry colname="col4">5.44</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="bibr" rid="bib1.bibx4" id="text.37"/> (flexible-noG)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M67" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M68" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>-SST URANS</oasis:entry>
         <oasis:entry colname="col3">771.3</oasis:entry>
         <oasis:entry colname="col4">5.49</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><xref ref-type="bibr" rid="bib1.bibx15" id="text.38"/>  (flexible)<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M70" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M71" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula>-SST RANS</oasis:entry>
         <oasis:entry colname="col3">808</oasis:entry>
         <oasis:entry colname="col4">5.66</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{4}?></table-wrap>

<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Aerodynamic behavior</title>
      <p id="d1e1577">Firstly, the overall global thrust <inline-formula><mml:math id="M72" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and power <inline-formula><mml:math id="M73" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> quantities are computed by <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M76" display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> describes the azimuth angle and <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> denotes the average over the last rotor revolution <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≤</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">360</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, which corresponds to a time span of <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4.959</mml:mn></mml:mrow></mml:math></inline-formula> s; <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mn mathvariant="normal">360</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> define a blade pointing in upwards direction.  The averaged quantities for the three simulation cases are in good agreement with the literature. Table <xref ref-type="table" rid="Ch1.T4"/> shows a comparison to various sources for rigid and flexible simulations of the NREL5 <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> rotor, taking into account slightly different configurations with respect to rotor tilt, pre-cone or tower inclusion. In the current investigation, the total thrust shows slightly higher loads when including blade flexibility compared to the rigid case, while the total aerodynamic power slightly decreases. This is also confirmed in the study by <xref ref-type="bibr" rid="bib1.bibx4" id="text.39"/>, which uses a similar setup.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1735">Rotationally averaged tangential and axial force distributions <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mtext>tan</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mtext>ax</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> for rigid and flexible blades over the outer half of blade span related to normalized radial locations. <inline-formula><mml:math id="M85" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> is the rotor radius, and <inline-formula><mml:math id="M86" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> defines the radial position on the blade.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f02.png"/>

        </fig>

      <p id="d1e1814">In the next step, the rotationally averaged force distributions of axial and tangential forces are investigated, i.e., <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mtext>ax</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mtext>tan</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rtn</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>.  Under flexible conditions and a uniform wind coming from the front, the blades tend to bend towards lower aerodynamic forces in the outboard region of the rotor, where the largest deformations are apparent. This holds for spanwise positions outboard of <inline-formula><mml:math id="M89" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 47 <inline-formula><mml:math id="M90" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M91" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 75 % relative span) as shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>, where the rotationally averaged tangential force in the upper graph and the rotationally averaged axial force in the lower graph are smaller for flexible blades, respectively. This is important, since most of the torque, and therefore power of wind turbines, is extracted from the wind in the outer third of the rotor blades due to the corresponding lever arms and the larger swept area. It is also shown that neglecting the gravitational loads barely influences the mean aerodynamic loads, as the corresponding tangential and axial forces are only slightly lower than the loads of the flexible blades including gravity. For spanwise positions between 50 % and 75 % radius, the blade forces including flexibility are slightly larger than for the rigid case, which aligns with the study by <xref ref-type="bibr" rid="bib1.bibx4" id="text.40"/>. This is due to the fact that the deformation of the blade leads to slightly higher AoAs for the flexible cases throughout the whole span. In the blade region outboard of 75 % <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> the forces are lower for the flexible cases. This can be explained by two counter acting phenomena. On the one hand the higher angle of attack leads to higher loads on the blade. On the other hand, the large flapwise deformation leads to a reduction of the rotor radius and thus in lower a circumferential speed and a change in inflow angle closer to the tip. The contribution of the angle of attack on the loads can be considered approximately linear, whereas the influence of the speed on the blade forces is quadratic and therefore prevails. The resulting forces outboard of 75 % span are therefore smaller for the flexible blades, although a larger AoA is present. Nevertheless, the radial part between 50 % and 75 % of the blade contributes less to the overall power output than the outer part, due to the smaller lever arm. Also a smaller total force difference between the rigid and flexible case than in the most outboard 25 % of blade span makes this region less attractive for this study, which aims at highlighting the differences between these setups. The blade region inboard of 50 % blade span is not shown since the total deformation<?pagebreak page209?> in all investigated regions is much smaller and the resulting differences in the force distributions are negligible.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1916"><bold>(a)</bold> Time series of tangential force (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mtext>tan</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) and axial force (<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mtext>ax</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) for the three cases of rigid and flexible blades over one rotation at 95 % span (i.e., at <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.95</mml:mn></mml:mrow></mml:math></inline-formula>), where the flexible blade forces are shown including gravity (solid red line) and without gravity (dotted red line). The rigid blade forces are shown as a dashed blue line. <bold>(b)</bold> Frequencies of the flexible and flexible-noG forces at 95 % span. Eigenfrequencies are marked as dashed black vertical lines. The 1P frequency is shown as vertical dotted magenta lines.</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f03.png"/>

        </fig>

      <p id="d1e1980">It is important to note that even though the curves of flexible and flexible-noG in Fig. <xref ref-type="fig" rid="Ch1.F2"/> lie almost on top of each other, a detailed look into the distribution resolved over one rotation shows clear differences. For that purpose, the force development of the 0.95 <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> location from Fig. <xref ref-type="fig" rid="Ch1.F2"/> is plotted against the respective azimuth angle in Fig. <xref ref-type="fig" rid="Ch1.F3"/>.  As visible in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a, the time series of the sectional forces at a spanwise position of 95 % span shows almost constant forces for the rigid blade and the flexible-noG case. While both flexible setups, consistent with the averaged forces of Fig. <xref ref-type="fig" rid="Ch1.F2"/>, show lower force values than the rigid case, a sinusoidal behavior within one rotation is clearly dominating the force development of the flexible blade including gravity. The reduction of forces due to blade deformation aligns with the findings of <xref ref-type="bibr" rid="bib1.bibx40" id="text.41"/>. The lowest loads are given at an azimuth angle of around 90<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, while the maximal loads occur around 270<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth. A frequency analysis of the forces acting on the flexible blades (with gravity, i.e., flexible case, and without gravity, i.e., flexible-noG case) is shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>b. The dominant frequency in the flexible case corresponds to the rotationally periodic 1P frequency (vertical dotted magenta line), which does not exist in the flexible-noG case. However, both cases show a clear impact of the second lowest eigenfrequency, which corresponds to the first edgewise mode (second vertical dashed black line). The larger impact of the edgewise component of blade vibrations, in contrast to the flapwise mode, is based on the fact that for attached flows, the aerodynamic damping in flapwise direction is significantly larger than in edgewise direction <xref ref-type="bibr" rid="bib1.bibx8" id="paren.42"/> and is therefore also more pronounced in the force frequencies. In Fig. <xref ref-type="fig" rid="Ch1.F3"/>b the 1P frequency and the other eigenfrequencies (Eigenf.) are clearly distinguishable.</p>
      <p id="d1e2035">While this frequency only has the second highest power spectral density in the flexible blade case, it dominates the force time series in the flexible-noG simulation. This clearly shows that the external 1P excitation only arises from the gravitation and therefore is not present in the flexible-noG results.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2040"><bold>(a)</bold> Edgewise (<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi>x</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>), <bold>(b)</bold> flapwise (<inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi>y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>) and <bold>(c)</bold> torsional (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>) blade tip deformation over one rotation for the flexible and flexible-noG case at <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f04.png"/>

        </fig>

      <p id="d1e2113">In Fig. <xref ref-type="fig" rid="Ch1.F4"/>, the blade tip deformation is shown, which also corresponds to the maximal deformation in edgewise, flapwise and torsional direction of the whole blade. Although being slightly further outboard than the section at 95 % span from Fig. <xref ref-type="fig" rid="Ch1.F3"/>, it describes an equivalent blade deformation behavior.</p>
      <p id="d1e2121">The dominating dynamic sinusoidal edgewise deflection component in Fig. <xref ref-type="fig" rid="Ch1.F4"/>a can be directly linked to the 1P gravitational load in Fig. <xref ref-type="fig" rid="Ch1.F3"/>, since the lever arm of gravitation for a blade in horizontal positions at 90 and 270<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth is the largest. The main cause of the reduction of power of the flexible blades in comparison to the rigid can on the one hand be traced back to the flapwise deflection (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b), which results in a smaller area swept by the turbine blades and therefore less energy that is extracted from the wind. On the other hand, the torsional degree of freedom impacts the loading, since a lower angle of attack is directly linked to a reduction of the local lift and drag components in the “linear region” and therefore impacts the lift-to-drag ratio <xref ref-type="bibr" rid="bib1.bibx29" id="paren.43"/>. As shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/>c, the torsional component is in phase with the edgewise deformation and has its largest influence at 90 and 270<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2156">Simplified representation of the gravity force acting on a turbine blade section at radial position <inline-formula><mml:math id="M105" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>.  Solid black airfoil: undeformed blade twist condition of rigid blade, dashed–dotted blue  airfoil: nose down deformation for azimuth angles of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≤</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">180</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, dashed green airfoil: nose up deformation for azimuth angles of <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mn mathvariant="normal">180</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≤</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">360</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">Fg</mml:mi><mml:mn mathvariant="normal">90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (in blue) and <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">Fg</mml:mi><mml:mn mathvariant="normal">270</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (in green) show the direction of gravitation for the respective azimuth angles. The local twist angle and AoA are given by <inline-formula><mml:math id="M110" display="inline"><mml:mi mathvariant="italic">φ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M111" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, respectively. The relative velocity <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>rel</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> results from the velocity components in the axial direction (<inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) and rotational velocity <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>r</mml:mi><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msup><mml:mi>a</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M115" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msup><mml:mi>a</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> define the induction factors in axial and tangential directions. <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> defines the undisturbed freestream velocity and <inline-formula><mml:math id="M118" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula> the angular velocity. Center of mass (CM), elastic axis (EA) and aerodynamic center (AC) are all located on the chord line.</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f05.png"/>

        </fig>

      <p id="d1e2353">This shows that a wind turbine rotor operating at rated conditions in a uniform inflow faces its largest influence of a dynamic excitation of structural deformation due to gravitational loads. Here, between 0 and 180<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth, the blade bends forward towards the leading edge, and during the upward rotation between 180<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 360<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth, it bends backwards in the direction of the trailing edge. Due to the structural nature of this blade, the center of mass (CM) is located downstream of the elastic axis (EA) on the chord line. This holds true for all sections along the blade, exemplarily shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/>. In combination with the local twist angles, the gravity force leads to a torsion of the blade. Thus, for a downward-moving blade, the angle of attack is reduced with increasing twist angle, while the AoA is increased for an upward-moving blade, where the twist angle is reduced. This can be explained using the simplified velocity triangle, where the inflow speed <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>inf</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the circumferential speed <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>rot</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>r</mml:mi><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msup><mml:mi>a</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> form the relative velocity <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>rel</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. Here, <inline-formula><mml:math id="M125" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> reflects the local axial induction and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msup><mml:mi>a</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> the local tangential induction factors. The constant <inline-formula><mml:math id="M127" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula> gives the rotational speed.</p>
      <p id="d1e2484">The dynamic torsion of the blade (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c) clearly shows the deformation due to the gravitation, forming a sinusoidal shape with a maximal deformation amplitude of <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>|</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover><mml:mo>|</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. Additionally, higher-frequency components can be found in the time series and superimpose the sinusoidal torsion behavior with oscillations due to the eigenfrequencies of the blade with a much smaller magnitude. Although barely visible in the three investigated deformation components (Fig. <xref ref-type="fig" rid="Ch1.F4"/>), it can be observed in the resulting forces acting on the blade especially in the frequency domain (Fig. <xref ref-type="fig" rid="Ch1.F3"/>b). In contrast, the flexible-noG case displays nearly constant aerodynamic forces and deformation due to the fact that the gravitational induced loads are completely missing (Fig. <xref ref-type="fig" rid="Ch1.F4"/>).</p>
      <p id="d1e2520">In the subsequent analysis of blade flexibility on different aerodynamic quantities, the focus lies therefore on the comparison of the rigid blades with the flexible blades including gravitational loads.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2526">Angle of attack distribution for <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> during one rotation for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2563">Axial induction factor distribution for <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> during one rotation for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f07.png"/>

        </fig>

<sec id="Ch1.S3.SS1.SSS1">
  <label>3.1.1</label><title>Angle of attack</title>
      <p id="d1e2605">As stated above, the inflow is constant and homogeneous for all cases, so the effect of the blade flexibility can be best assessed by focusing on the comparison between the rigid blades and the blades subjected to the periodic gravity-induced blade deformation. The flexible-noG simulations, in which no significant deformations occur (Fig. <xref ref-type="fig" rid="Ch1.F4"/>), are therefore omitted from the analysis. Therefore, in the following all investigations refer to the rigid and flexible cases. A<?pagebreak page210?> comparison of the local AoA for the most outboard 10 % of the blade simulations (corresponding to <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>) is shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>, where the respective azimuthal position is plotted against the radial location on the blade, showing rigid results in Fig. <xref ref-type="fig" rid="Ch1.F6"/>a and flexible results in Fig. <xref ref-type="fig" rid="Ch1.F6"/>b. The investigated AoA magnitude is accounted for with color bins of <inline-formula><mml:math id="M132" display="inline"><mml:mn mathvariant="normal">0.4</mml:mn></mml:math></inline-formula><inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p id="d1e2652">For the rigid blade case, the AoA becomes larger with increasing radius but stays constant for each section independently of the azimuth angle. The radial increasing effect is also visible for the flexible blade, but in contrast to the rigid case, it deviates over the azimuth angle, showing the expected sinusoidal shape.  The smallest AoA for the flexible blades is observed at 90<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth, whilst for 270<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth its maximum is present. This phenomenon can directly be linked to the torsional deformation, as shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/>c, where the gravitation twists the blade towards lower AoA during a downwards movement of the blade and towards higher AoAs when moving upwards again.</p>
</sec>
<?pagebreak page211?><sec id="Ch1.S3.SS1.SSS2">
  <label>3.1.2</label><title>Axial induction</title>
      <p id="d1e2683">Similar trends are visible in the representation of the axial induction (Fig. <xref ref-type="fig" rid="Ch1.F7"/>), where each color bin represents an axial induction portion of 0.03. A general reduction of the axial induction towards the tip is visible for rigid and flexible blades. At the most outboard position it vanishes due to the ever shrinking surface and the blade boundary layers merging between pressure and suction side of the blade.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2690">Lift coefficient (<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">l</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) distribution for <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> during one rotation for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f08.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e2738">Drag coefficient (<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) distribution for <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> during one rotation for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f09.png"/>

          </fig>

      <p id="d1e2785">Since the axial induction factor describes the amount of velocity reduction of the freestream normal to the rotor plane, it gives an estimate of the amount of energy taken from the fluid. From Fig. <xref ref-type="fig" rid="Ch1.F7"/>, it is therefore expected that more energy is extracted with the flexible blade pointing towards 270<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> than at 90<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth. This matches the findings in Fig. <xref ref-type="fig" rid="Ch1.F3"/>, where the maximal axial and tangential force is occurring at <inline-formula><mml:math id="M142" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 270<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and the minimal force is to be found at <inline-formula><mml:math id="M144" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 90<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth, respectively.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS1.SSS3">
  <label>3.1.3</label><title>Lift, drag and lift-to-drag ratio</title>
      <p id="d1e2852">Next to the forces described in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>, the lift, drag and lift-to-drag ratio coefficients play an important role, since they represent the loading on the blades and allow for an estimate of whether the blade operates under optimal conditions. Since modern wind turbines are lift driven, a maximal energy extraction from the wind is present, when the lift-to-drag ratio reaches its maximum, which corresponds to the maximal ratio of lift over drag. Lift and drag are also direct inputs to engineering models like the blade element momentum theory, so that a deep understanding of those quantities is vital for the improvement of such design tools <xref ref-type="bibr" rid="bib1.bibx32" id="paren.44"/>.</p>
      <?pagebreak page212?><p id="d1e2860">The coefficients for lift and drag are calculated from the simulation results using the local pressure distribution at various sections along the blade, leading to a force vector that is split into lift and drag directions using the angle of attack calculated from the “3-point” method in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1.SSS1"/>. Figure <xref ref-type="fig" rid="Ch1.F8"/> shows the lift coefficient distribution of the rigid and flexible blade cases in bins of <inline-formula><mml:math id="M146" display="inline"><mml:mn mathvariant="normal">0.015</mml:mn></mml:math></inline-formula>, with consistent reduction of lift towards the tip. The minimal lift at 90<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and maximal lift at 270<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth for the flexible blades is as expected since the same behavior is shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/> for the absolute force values in tangential and normal direction.</p>
      <p id="d1e2895">The drag coefficient in Fig. <xref ref-type="fig" rid="Ch1.F9"/>, contrary to the corresponding lift values, increases with radial distance. Since under these operating conditions, the drag values in general are very small, drag bins of <inline-formula><mml:math id="M149" display="inline"><mml:mn mathvariant="normal">0.0075</mml:mn></mml:math></inline-formula> are shown. The distribution of minimal and maximal drag coefficient values coincides with the findings of lift and AoA. This is an expected behavior, since most airfoils operate in the so-called ”linear region” when exposed to incoming angles of attack between 4.8 and 8.0<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (cf. Fig. <xref ref-type="fig" rid="Ch1.F6"/>), where the boundary layer is fully attached to the blade surface and the drag force is directly proportional to the angle of attack.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e2921">Lift-to-drag ratio distribution for <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> during one rotation for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f10.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e2958">Mean velocity magnitude slice in the <inline-formula><mml:math id="M152" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M153" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> plane at <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> D downstream of the turbine with incoming flow direction in <inline-formula><mml:math id="M155" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> direction for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades. Color coding bounded such that all values of <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>mean</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.596</mml:mn></mml:mrow></mml:math></inline-formula> are shown in white, while all values of <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>mean</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.526</mml:mn></mml:mrow></mml:math></inline-formula> are marked in dark blue.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f11.png"/>

          </fig>

      <p id="d1e3051">Since in the investigated region the drag grows faster with increasing AoA compared to the lift, the lift-to-drag ratio of <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">l</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is not constant but shows sinusoidal behavior for the flexible blade over one rotation with a maximal lift-to-drag ratio for minimal drag at an azimuth of 90<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F10"/>). From an aerodynamic standpoint, the blade airfoils in the investigated region therefore show better performance when the blade is moving downwards, than for an upward-moving blade.</p>
      <p id="d1e3083">Summarized, the aerodynamic investigation of the most outboard 10 % of the blade (i.e., <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>≤</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula>) reveals a major difference between rigid and flexible structures.  The investigation of AoA, induction, and force coefficients shows a clear dependency of the flexible blades on the azimuth angle. Since the aerodynamic behavior in the rotor plane characterizes the interaction of blades with the surrounding air, differences in the induction due to flexibility are expected to be visible in the wake of the turbine, too. This is studied in the next section.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e3108">Mean velocity magnitude slice in the <inline-formula><mml:math id="M161" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M162" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> plane at <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D downstream of the turbine with incoming flow direction in <inline-formula><mml:math id="M164" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> direction for <bold>(a)</bold> rigid and <bold>(b)</bold> flexible blades. Color coding bounded such that all values of <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>mean</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.596</mml:mn></mml:mrow></mml:math></inline-formula> are shown in white, while all values of <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mtext>mean</mml:mtext></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.456</mml:mn></mml:mrow></mml:math></inline-formula> are marked in dark blue.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f12.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Effects in the wake</title>
      <?pagebreak page213?><p id="d1e3211">To investigate the effect of a sinusoidal aerodynamic behavior within one rotation of the blade, a characterization of the whole wake cross section at different downstream locations is made. Here, slices at <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> D and <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D in the wake of the turbine normal to the flow direction are investigated with respect to the mean speed magnitude for speed in <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> direction, i.e., <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:msqrt><mml:mrow><mml:msubsup><mml:mi>u</mml:mi><mml:mi>x</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>u</mml:mi><mml:mi>y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>u</mml:mi><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:msqrt><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rot</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. Here, <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mo>〉</mml:mo><mml:mtext>rot</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> denotes the average over the last whole rotation. In Fig. <xref ref-type="fig" rid="Ch1.F11"/>, the mean velocity distribution of the wakes of both simulations are compared, with the rigid blade case in Fig. <xref ref-type="fig" rid="Ch1.F11"/>a and the results for the flexible blades in Fig. <xref ref-type="fig" rid="Ch1.F11"/>b. The velocity magnitude ranges are chosen such that the region of maximal blade deformation becomes apparent. The resulting shape of the visualized speed reduction is forming a uniform ring. The rigid blade case shows a uniform wake velocity deficit over the whole azimuth with minimal wake speed at <inline-formula><mml:math id="M172" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 80 % span. This radial location of minimum speed can also be observed in the case of the flexible blades but with a clear shift between left and right, corresponding to 270 and 90<inline-formula><mml:math id="M173" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth. Here, a velocity difference of <inline-formula><mml:math id="M174" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 5 % is visible between the two sides. Also the expansion of the visualized wake speed is larger at 270 than at 90<inline-formula><mml:math id="M175" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth.  This results in a non-uniform thickness of the ring shape, indicating that the wake stream tube expansion itself is deformed in a way that the wake radius is larger at azimuthal positions of lower wake speed and smaller at azimuthal positions with higher wake speed.</p>
      <p id="d1e3348">Although less significant, similar results are shown for a <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D downstream location as shown in Fig. <xref ref-type="fig" rid="Ch1.F12"/>. The total influenced area seems to expand and smear out.  Since mixture of fluid between the outer free stream and the inner wake is not expected within 1 to 2 diameters downstream of the turbine <xref ref-type="bibr" rid="bib1.bibx1" id="paren.45"/>, this can be explained by increasing turbulent mixture inside the stream tube, that is created by the rotor itself. This effect is more dominant at the <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D downstream location compared to the <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> D downstream location. The minimal wake speed in the flexible case is shifted slightly towards the ground (dark blue region), which is attributed to the counterclockwise rotation of the wake. Similar rotation is also present in the rigid blade case, but it is not visible here due to the uniform character of the rigid rotor wake. This rotation opposing the clockwise rotation of the turbine is based on the conservation of momentum and has been reported in many studies before <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx41 bib1.bibx23" id="paren.46"/>.  Contrary to the uniform ring shape of the rigid wake, again the shape of the wake of the flexible simulation is deformed, trending towards an oval contour.</p>
      <p id="d1e3396">This is consistent with the results from the aerodynamic investigation in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>, where lower speeds in the wake<?pagebreak page214?> of azimuthal positions of larger induction or higher angles of attack were observed. Thus, the impact of flexible rotor blades on the aerodynamic behavior of the wind turbine is as well transported into the wake and still visible at least <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D downstream of the turbine.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Tip vortex trajectory in the near wake</title>
      <p id="d1e3421">From the findings of the aerodynamic behavior in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/> and the mean wind speeds analyzed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>, a clear difference between azimuth positions of 90 and 270<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> is evident for flexible blades in contrast to the rigid blade representation. Apart from the difference in mean wind speeds, also the shape of the wake stream tube deviates. To quantify these variations, a deeper investigation of the blade tip vortex trajectories is made in the following.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e3439">Stream tube extraction from the <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> field: <bold>(a)</bold> general representation of a stream tube through a rotor plane. <bold>(b)</bold> Tip vortex cores at different instants in time. Color coding bounded such that all values of <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> are shown in white, while all values of <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">6000</mml:mn></mml:mrow></mml:math></inline-formula> are marked in yellow.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f13.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e3497">Tip vortex trajectory for rigid blades (blue) and flexible blades (red) at <bold>(a)</bold> 90<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth and <bold>(b)</bold> 270<inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth (averaged over five blade vortex trajectories), including asymmetric error bars for the maximal and minimal values of all trajectories.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://wes.copernicus.org/articles/9/203/2024/wes-9-203-2024-f14.png"/>

        </fig>

      <?pagebreak page215?><p id="d1e3531"><?xmltex \hack{\newpage}?>In general, the stream tube, being formed by all particles of the fluid moving through the rotor plane, has a smaller diameter upstream of the turbine, where the speed is higher, than downstream of the rotor disk where the speed is smaller (Fig. <xref ref-type="fig" rid="Ch1.F13"/>a). The larger the reduction of wind velocity, the wider the stream tube is to be expected further downstream as a consequence of the mass conservation. A representative structure, that describes the behavior of the stream tube at the blade tip, is the trajectory of the tip vortex of the blades, since it reflects the most outboard part of the fluid moving through the rotor plane. Based on the comparison of the rigid and flexible blades in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>, different behavior for the wake expansion has to be visible at different azimuth positions. For that purpose, the tip vortex trajectories are extracted from the flow field in horizontal planes parallel to the inflow direction making use of the <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> criterion described in <xref ref-type="bibr" rid="bib1.bibx16" id="text.47"/>. Figure <xref ref-type="fig" rid="Ch1.F13"/>b shows a representative <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> field extracted from the rigid blade CFD simulation at different time instants orthogonal to the rotor plane. Here, <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> defines the radial and <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula> the axial position normalized by the blade length. The wake age is defined such that at 0<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> the blade tip is located at <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>/</mml:mo><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.0</mml:mn></mml:mrow></mml:math></inline-formula>. During rotation, the blade passes through the slice, forming a tip vortex that is transported downstream in time, following a characteristic path. For the uniform conditions of the rigid setup, this path is independent of the blade position and can be extracted in any plane perpendicular to the rotor plane.  The largest deviations of the aerodynamic quantities (Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>) and the wake velocity reductions (Sect.<xref ref-type="sec" rid="Ch1.S3.SS2"/>) are present for the azimuth angles, where the blade is positioned horizontally, i.e., 90 and 270<inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Therefore, it is also expected that the largest differences in the tip vortex trajectories are visible under these conditions. To quantify these differences and the influence of blade flexibility on the path, the vortex trajectory is analyzed for tip vortices trailed at 90 and 270<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for the rigid and flexible simulation. This radial location of the vortex trajectory is defined by the position of maximal values of <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> inside the vortex core.</p>
      <p id="d1e3666">Figure <xref ref-type="fig" rid="Ch1.F14"/> shows the non-dimensionalized radial location of the tip vortex trajectory averaged over the latest five times<?pagebreak page216?> the blade is passing through the plane of interest. The wake age is limited to 120<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, since this corresponds to the instant the next blade is slicing through the plane, forming a new vortex trajectory heading downstream normal to the rotor plane. The radial position <inline-formula><mml:math id="M197" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> of the vortex core is normalized by the blade radius <inline-formula><mml:math id="M198" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>. Vortex core locations are tracked at each 2<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of the wake age, making sure that the near-wake expansion is properly resolved. A characteristic inboard tip vortex motion is visible for all cases for the first 20<inline-formula><mml:math id="M200" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> wake age before expanding the stream tube and exceeding the actual radius of the rotor blades between 35 and 50<inline-formula><mml:math id="M201" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> wake age. This characteristic trajectory aligns with the findings of <xref ref-type="bibr" rid="bib1.bibx38" id="text.48"/> and <xref ref-type="bibr" rid="bib1.bibx11" id="text.49"/> for their investigation for rigid blades, but a comparison between rigid and flexible blades is displayed for the first time in this work.</p>
      <p id="d1e3728">It is visible that the radial location of the tip vortex of the rigid blade case exceeds the trajectory of the flexible blades at 90<inline-formula><mml:math id="M202" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth in the whole investigated region (Fig. <xref ref-type="fig" rid="Ch1.F14"/>a), whereas opposing behavior is shown at 270<inline-formula><mml:math id="M203" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth (Fig. <xref ref-type="fig" rid="Ch1.F14"/>b). A larger stream tube expansion corresponds to a higher velocity reduction and vice versa. This is supported by the findings made in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>, where the investigation of axial induction factors in Fig. <xref ref-type="fig" rid="Ch1.F7"/> showed that the flexible blades induce a higher velocity reduction at 270<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and induce a lower velocity reduction in the axial component at 90<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth compared to the rigid blade case.  Apart from the impact on the wake flow, this affects the loading of the rotor as well. Non-uniform blade root bending moments are the consequence of each of the three blades, leading to an additional 3P main shaft and tower top excitation in the case of a full wind turbine setup. Consequently, this needs to be considered in the design process of large flexible rotors.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusion</title>
      <p id="d1e3785">In the current study, three different simulations of the NREL5 <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">MW</mml:mi></mml:mrow></mml:math></inline-formula> turbine were performed using a uniform inflow velocity at rated conditions. A rigid blade setup is compared to a setup with flexible blades with gravity and flexible blades without gravity.  Aerodynamic quantities have been extracted from the flow field using the “3-point” method. As with any other method, uncertainties in the obtained results are unavoidable. However, the uncertainties apply in the same manner to the rigid and flexible blade cases. Since the focus of this investigation lies in a relative comparison between the rigid and flexible cases, and not on the absolute value of the aerodynamic quantities, the possible influence of the uncertainties is considered not to be critical for our analysis.</p>
      <p id="d1e3796">It was shown that the aerodynamic forces of flexible rotor blades vary with the azimuth angle of each blade. This effect becomes stronger in outer parts of the blades, which contribute most to the global power output due to larger lever arms, as a consequence of the deformations induced by the gravitational loads. In uniform inflow, this effect is dominated by gravitational loading, which especially increases torsional deformations and, therefore, leads to a dynamic change in induction and AoA.  Since the direction of gravitation strictly follows a 1P frequency, the resulting excitation of the blades shows a rotationally periodic sinusoidal behavior in all investigated aerodynamic quantities. With this turbine setup, the investigation reveals a much larger lift-to-drag ratio for a blade moving downwards than for an upward-moving blade, which leads to the conclusion that the investigated blade region performs better when the blade is descending.</p>
      <p id="d1e3799">Furthermore, it was shown that in contrast to the uniform wake of a rigid rotor, this varying aerodynamic behavior of the flexible setup is also transported into the wake, visible in rotationally periodic wake speed deficits. This deficit rotates opposing the turbine in the counterclockwise direction, leading to an asymmetry in the speed distribution varying with downstream distance. A 5 % speed difference was observed for the flexible simulation case within one rotation at <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> D and <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> D downstream locations. This asymmetry, visible in the deformation of the wake shape, can be quantified by the tip vortex trajectory at 90 and 270<inline-formula><mml:math id="M209" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> azimuth within the first 120<inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> of wake age. This led to the conclusion that the radial near-wake expansion downstream of the downward-moving blades is smaller for the flexible blades than for the rigid blade setup. Opposing behavior was observed in the near wake of the blades moving upward. To the authors' knowledge this effect has not been addressed before, and it can serve as a basis for the analysis of more complex operating conditions.</p>
      <p id="d1e3844">With wind turbines becoming larger and larger, the described influences are expected to be more pronounced, since larger diameters are directly accompanied with more flexible structures. It is therefore worth studying these effects in more detail. Thus, these effects should be taken into account for future investigations and designs of large, flexible rotor blades, since the sinusoidal varying aerodynamic forces increase the impact of alternating blade loads on various turbine components. Also during conditions, where blades operate close to stall, the deformation due to gravitational loading could potentially cause unwanted flow separation and lead to highly dynamic phenomena, e.g., dynamic stall. Additionally, the decay of the wake further downstream and the impact of blade-flexibility-driven skewed wakes on a following turbine, for example in a wind farm, should be investigated.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3852">The raw data of the simulation results can be provided by contacting the corresponding author.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3858">LH performed the simulations, post-processing and analysis. LJL and IH provided assistance and guidance of the underlying methods. LH wrote the paper with corrections from LJL, BS and IH.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3864">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3870">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3876">The computations were performed on the high-performance computing system EDDY of the University of Oldenburg.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3881">This research has been supported by the project WIMS-Cluster by the Federal Ministry of Economic Affairs and Climate Action (grant no. 0324005).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3887">This paper was edited by Alessandro Bianchini and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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