<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0"><?xmltex \bartext{15th~EMS Annual Meeting\,\&\, 12th~European Conference on Applications of Meteorology~(ECAM)}?>
  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ASR</journal-id>
<journal-title-group>
<journal-title>Advances in Science and Research</journal-title>
<abbrev-journal-title abbrev-type="publisher">ASR</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Adv. Sci. Res.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1992-0636</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/asr-13-63-2016</article-id><title-group><article-title>Representation of the grey zone of turbulence in the atmospheric boundary layer</article-title>
      </title-group><?xmltex \runningtitle{Representation of the grey zone of turbulence in the atmospheric boundary layer}?><?xmltex \runningauthor{R.~Honnert}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Honnert</surname><given-names>Rachel</given-names></name>
          <email>rachel.honnert@meteo.fr</email>
        </contrib>
        <aff id="aff1"><institution>CNRM-Météo-France, CNRM/GMAP, Toulouse, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Rachel Honnert (rachel.honnert@meteo.fr)</corresp></author-notes><pub-date><day>19</day><month>April</month><year>2016</year></pub-date>
      
      <volume>13</volume>
      <fpage>63</fpage><lpage>67</lpage>
      <history>
        <date date-type="received"><day>12</day><month>January</month><year>2016</year></date>
           <date date-type="rev-recd"><day>29</day><month>March</month><year>2016</year></date>
           <date date-type="accepted"><day>30</day><month>March</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016.html">This article is available from https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016.html</self-uri>
<self-uri xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016.pdf">The full text article is available as a PDF file from https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016.pdf</self-uri>


      <abstract>
    <p>Numerical weather prediction model forecasts at horizontal grid lengths in
the range of 100 to 1 km are now possible. This range of scales is the
“grey zone of turbulence”. Previous studies, based on large-eddy simulation
(LES) analysis from the MésoNH model, showed that some assumptions of some turbulence schemes on
boundary-layer structures are not valid. Indeed, boundary-layer thermals are
now partly resolved, and the subgrid remaining part of the thermals is
possibly largely or completely absent from the model columns. First, some
modifications of the equations of the shallow convection scheme have been
tested in the MésoNH model and in an idealized version of the operational
AROME model at resolutions coarser than 500 m. Secondly, although the
turbulence is mainly vertical at mesoscale (<inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2 km resolution), it is
isotropic in LES (<inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 100 m resolution). It has been proved by LES analysis
that, in convective boundary layers, the horizontal production of turbulence
cannot be neglected at resolutions finer than half of the boundary-layer height. Thus, in
the grey zone, fully unidirectional turbulence scheme should become
tridirectional around 500 m resolution. At Météo-France, the
dynamical turbulence is modelled by a K-gradient in LES as well as at
mesoscale in both MésoNH and AROME, which needs mixing lengths in the
formulation. Vertical and horizontal mixing lengths have been calculated from
LES of neutral and convective cases at resolutions in the grey zone.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The grey zone of turbulence is defined by <xref ref-type="bibr" rid="bib1.bibx18" id="text.1"/> as the scales
on the order of the energy-containing turbulence scale. At these resolutions,
the turbulence structures are neither entirely subgrid scale (as in global
and mesoscale models) nor largely resolved (as in large-eddy simulations – LESs).
<xref ref-type="bibr" rid="bib1.bibx7" id="text.2"/> used LES coarse-graining to produce similarity
functions linking the subgrid or resolved part of the turbulent fluxes and
the horizontal resolution of the model out of the height of the thermals.
They indicated that the grey zone exists from resolutions smaller than 2
times the boundary-layer height in convective boundary layers (CBLs). Regional
models are now approaching the sub-kilometre scales, and <xref ref-type="bibr" rid="bib1.bibx7" id="text.3"/>
showed that neither unidirectional (1-D) non-local mesoscale boundary-layer (BL)
turbulence scheme nor isotropic (3-D) LES schemes are appropriate at
these scales. That is why the turbulence schemes have to be adapted to the
grey zone of turbulence.</p>
      <p><?xmltex \hack{\newpage}?><xref ref-type="bibr" rid="bib1.bibx2" id="text.4"/> blended a 3-D-Smagorinsky with a 1-D non-local BL scheme with
the help of the similarity functions proposed by <xref ref-type="bibr" rid="bib1.bibx7" id="text.5"/>.
<xref ref-type="bibr" rid="bib1.bibx10" id="text.6"/> extended the Mellor and Yamada scheme by modifying the length
scales using statistics obtained from LES coarse-graining. <xref ref-type="bibr" rid="bib1.bibx15" id="text.7"/>
quantified the local and non-local turbulence at scales in the grey zone to
adjust the vertical profiles resulting from their non-local K-gradient scheme.</p>
      <p>These adaptations strongly depend on the schemes which are currently used at
mesoscale or LES. At Météo-France, the turbulence in the atmospheric BL
is represented by an eddy-diffusivity/mass-flux parameterization (EDMF;
<xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx16" id="altparen.8"/>). The updraughts are represented by
the mass-flux scheme which starts at the ground (hereafter PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula>;
<xref ref-type="bibr" rid="bib1.bibx12" id="altparen.9"/>) and represents the shallow convection, while the rest of
the turbulence is represented by a K-gradient scheme (hereafter CBR;
<xref ref-type="bibr" rid="bib1.bibx4" id="altparen.10"/>). Both parts of this scheme are being modified to adapt
Météo-France models to the grey zone of turbulence. In this article,
modifications of PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula> are presented in the second section as well as
preliminary results in the third section. As perspective, the “true” CBR
mixing lengths in the grey zone are presented.</p>
</sec>
<sec id="Ch1.S2">
  <title>A new mass-flux scheme</title>
      <p>As many mass-flux schemes, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula> is based on several assumptions which are
valid at large scales. It assumes in particular that the thermal surface is
small, the resolved vertical velocity is zero, and the thermal field is quasi-stationary.</p>
      <p><xref ref-type="bibr" rid="bib1.bibx8" id="text.11"/> determined the characteristics of the non-local
turbulence (BL thermals) in the grey zone by means of a conditional sampling.
Figure <xref ref-type="fig" rid="Ch1.F1"/> shows a 16 km long horizontal cross section of an LES. The
thermals (in white) and the part of the thermals which impact the subgrid
mass-flux scheme at 1 km resolution (in black) have been determined by the
conditional sampling of <xref ref-type="bibr" rid="bib1.bibx8" id="text.12"/>. The environment of the
structures is in red. Figure <xref ref-type="fig" rid="Ch1.F1"/> shows that at 16 km resolution,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula>'s assumptions are valid: the thermal surface is small, the resolved
vertical velocity is zero, as the grid cell contains both the updraughts and
the compensatory subsidence, and the thermal field is quasi-stationary.
However, in the grey zone, they are not verified. Indeed, as seen on the
1 km zoom of Fig. <xref ref-type="fig" rid="Ch1.F1"/>, the thermal surface (in black) may be large,
the resolved vertical velocity is not zero, as one thermal can fill the
grid cell, and the thermal field is probably not quasi-stationary.</p>
      <p>However, mass-flux schemes can be developed without the three assumptions
presented before. The initial schemes (PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula>; <xref ref-type="bibr" rid="bib1.bibx13" id="altparen.13"/>) describe the
behaviour of parameters of one unique thermal in the mesh (the vertical
velocity <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the mass-flux <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the total potential temperature <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mrow><mml:msub><mml:mi>l</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>,
the thermal surface area <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, the buoyancy inside the
thermal <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>B</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the pressure and the entrainment (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>)/detrainment (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>)
lateral closure). <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are constant. Equations (1)–(4) show the
modifications (in red) of PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula>. The non-negligible resolved vertical velocity
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) is added in Eqs. (1), (3), and (4). The thermal surface is
not negligible and appears at the denominator in Eqs. (3)–(4). The surface
triggering of the mass flux (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, Eq. 5) depends on the resolution.

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="italic">α</mml:mi><mml:mfenced close=")" open="("><mml:msub><mml:mi>w</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msup></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mrow><mml:msub><mml:mi>l</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mrow><mml:msub><mml:mi>l</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>l</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msup></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:msub><mml:mi>w</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msup></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>B</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mfenced close=")" open="("><mml:msub><mml:mi>w</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msup></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn>0.075</mml:mn><mml:mo>×</mml:mo><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mtext>tanh</mml:mtext><mml:mfenced open="(" close=")"><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>x</mml:mi></mml:mrow><mml:mrow><mml:mi>h</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>h</mml:mi><mml:mi>c</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>+</mml:mo><mml:mn>0.8</mml:mn></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p><?xmltex \hack{\newpage}?>Then, the finer the resolution or the smaller the BL height, the smaller the
subgrid turbulent flux. The scheme produces less subgrid turbulence.
Consequently, resolved BL thermals are created.</p>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
      <p>The results presented in this section compare model simulations and
coarse-grained LES of a dry CBL (hereafter IHOP). This case has been
performed using radio soundings collected during the International H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
Project (IHOP<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2002</mml:mn></mml:msub></mml:math></inline-formula>) campaign <xref ref-type="bibr" rid="bib1.bibx17" id="paren.14"/>. This field experiment
took place in the US Southern Great Plains from 13 May to 25 June 2002.
Here, we used the 14 June 2002 case corresponding to a growing CBL near
Homestead, Oklahoma (cf. <xref ref-type="bibr" rid="bib1.bibx3" id="altparen.15"/>). This day was characterized by high
pressure (1016 hPa or more) and light wind (less than 5 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).
The vertical shear was weak. The well-mixed boundary layer reached
1.5 km in the beginning of the afternoon. The radio soundings were made in
the morning from 14:00 to 18:00 UTC (09:00 to 13:00 LT – local time). This case was
chosen as it presented a relatively uniform site topography and a typical
development of continental convective boundary layer. The simulations lasted for 7 h.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>16 km long horizontal cross section of an LES (IHOP
case, 14:00 LT, 500 m altitude) and 1 km long zoom. The thermal fraction
is in white, the core of the thermals (strong vertical velocity) is in black,
and the environment is in red (see <xref ref-type="bibr" rid="bib1.bibx8" id="altparen.16"/>).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016-f01.pdf"/>

      </fig>

      <p>Méso-NH <xref ref-type="bibr" rid="bib1.bibx11" id="paren.17"/> is the research model at Météo France. It
can be used in various configurations of the turbulence scheme (from LES to
synoptic), in idealized cases, as well as in real cases. In
Fig. <xref ref-type="fig" rid="Ch1.F2"/>a and b, the resolved turbulent kinetic energy (TKE) of the new
parameterization (in green) is compared at 500 m and 1 km resolution with
the results of the LES coarse-graining (in black), those of simulations with
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula> (in blue), and without mass flux at all (in red). The new parameterization
is scale-adaptive and produces the resolved TKE calculated from the LES,
even if it produces a bit too much TKE at 500 m and not enough at 1 km resolution.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Resolved TKE in Méso-NH at <bold>(a)</bold> 500 m and <bold>(b)</bold> 1 km
resolution in IHOP. The reference (coarse-grained LES) is in black, and the
parameterization in green. The blue lines are results of simulations with
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>09</mml:mn></mml:msub></mml:math></inline-formula>, and the red ones result from simulations without shallow convection.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016-f02.png"/>

      </fig>

      <p><?xmltex \hack{\newpage}?>AROME <xref ref-type="bibr" rid="bib1.bibx14" id="paren.18"/> is the operational regional model at Météo
France. Its turbulence scheme is the same as Méso-NH, but the configuration
is fixed (for mesoscale simulations) and it simulates real cases only. It is
challenging to test a new turbulence parameterization in the operational AROME
as there is no reference. That is why, in these tests, we used
idealized-AROME. This model has no land surface or lateral coupling and no
surface scheme. The imposed boundary conditions allow us to reproduce in AROME
the idealized cases previously studied in LES.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F3"/> shows subgrid TKE produced by the new parameterization at
resolutions from 500 m to 2 km (dotted lines) and the subgrid TKE at
resolutions from 62.5 m to 8 km calculated from LES. In the middle of the
BL, the parameterization follows the LES reference. However, in the surface
layer, the turbulence is underestimated. This default is not due to the
mass-flux parameterization, but it results from limits of the K-gradient scheme.
Indeed, it is purely 1-D in AROME, while in the surface layer, a 3-D dynamical
turbulence is required.</p>
</sec>
<sec id="Ch1.S4">
  <title>Limits of the mass-flux modifications: from 1-D to 3-D turbulence scheme</title>
      <p>A second problem appears in the grey zone of turbulence: the dimensionality
of the scheme. At mesoscale, the horizontal homogeneity assumption allows the
computation of the vertical (1-D) turbulent flux only. On the contrary, in LES, the
turbulence is assumed isotropic, thus 3-D. The limit resolution at which the
horizontal turbulent movements are not negligible is in the grey zone.
<xref ref-type="bibr" rid="bib1.bibx6" id="text.19"/> quantified the production terms of the TKE at grey-zone
resolutions from LES coarse-graining. At mesoscale, the turbulence is mainly
produced by thermals; thus the (vertical) mass-flux scheme has the most
impact. However thermal production of TKE is reduced in the grey zone, as the
thermals are partly resolved, and the vertical and horizontal components of
the dynamical production of TKE become larger; thus the 3-D K-gradient scheme
becomes critical.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Subgrid TKE in AROME at 500 m and 1 km resolution in
the IHOP. “MNH” means the reference LES (in full lines) and AROME means the
new parameterization (in dotted lines).</p></caption>
        <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016-f03.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p><bold>(a)</bold> Vertical and <bold>(b)</bold> horizontal mixing lengths computed at
resolutions from 12.5 to 800 m. CASES-99 (neutral BL).</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://asr.copernicus.org/articles/13/63/2016/asr-13-63-2016-f04.png"/>

      </fig>

      <p><xref ref-type="bibr" rid="bib1.bibx6" id="text.20"/> have proved that the limit resolution at which the
horizontal turbulent movements are not negligible is about 0.5 times the
size of the energy-containing structures in free CBL (about 500 m
resolution). So, the modifications made in the mass-flux part impact the
scheme until about 500 m resolution. The K-gradient scheme has to be
modified for finer resolutions. Firstly, a 3-D K gradient is necessary. AROME,
for instance, has no 3-D turbulence scheme. This limits the modelling of the
smallest scales of the grey zone of the turbulence with AROME. Secondly, the
subgrid turbulence is not isotropic in the grey zone (as proved in
<xref ref-type="bibr" rid="bib1.bibx6" id="altparen.21"/>). Méso-NH, for instance, possesses a 3-D turbulence
scheme. However, the turbulence is always assumed isotropic. In particular,
the LES scheme uses a unique mixing length on the horizontal and on the
vertical. Finally, the mixing length is on the order of the boundary-layer
height at mesoscale <xref ref-type="bibr" rid="bib1.bibx1" id="paren.22"/> and on the order of the mesh size in LES.</p>
      <p>The size of the vertical and horizontal mixing lengths is studied in the grey
zone. The eddy diffusivity (<inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula>) is calculated from the fluxes
(<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> in Eqs. 6–8) and
gradients (e.g. <inline-formula><mml:math display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> in Eqs. 6–8)
computed by LES coarse-graining of IHOP and an additional neutral case at
several resolution in the grey zone (Eqs. 6–8). The mixing lengths (<inline-formula><mml:math display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>)
are computed from the eddy diffusivity and the TKE (<inline-formula><mml:math display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>) (Eqs. 9–11) in the
CBR equations (<inline-formula><mml:math display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is a constant).

              <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E6"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E9"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>C</mml:mi><mml:msub><mml:mi>L</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:msub><mml:msqrt><mml:mi>e</mml:mi></mml:msqrt></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E10"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>C</mml:mi><mml:msub><mml:mi>L</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:msqrt><mml:mi>e</mml:mi></mml:msqrt></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E11"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>C</mml:mi><mml:msub><mml:mi>L</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:msqrt><mml:mi>e</mml:mi></mml:msqrt></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the mixing lengths in the neutral BL (CASES-99)
based on the CASES-99 experiment which took place from 1 to 31 October 1999
near Leon, Kansas. It was first designed to study stable BL, morning and
evening transitions periods. Measurements were taken during neutral
conditions. <xref ref-type="bibr" rid="bib1.bibx5" id="text.23"/> first described this LES. The rugosity
length of the site is 0.1 m, and the friction velocity is 0.42 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. A
constant (293.15 K) potential temperature is imposed until
750 m altitude <xref ref-type="bibr" rid="bib1.bibx5" id="paren.24"/> and then a constant adiabatic gradient
until 1500 m altitude. The stable boundary layer kills the turbulence above
750 m altitude and limits the size of the eddies. Thus, the eddies remain
small enough to be contained in the LES domain. The heat flux at the surface
is zero along the simulations, as well as the humidity flux at the surface.
The simulations are dry. Thus, the buoyancy flux is zero during the
simulations and the production of turbulence is purely dynamical. The
geostrophic wind is zonal and prescribed at 10 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F4"/> shows vertical and horizontal mixing lengths computed by
Eqs. (6)–(11). Both vertical and horizontal mixing lengths are larger at
mesoscale. Under 1000 m altitude, the vertical mixing lengths are
consistent with the literature: at mesoscale, they behave as in <xref ref-type="bibr" rid="bib1.bibx1" id="text.25"/>
with a maximum of a few hundred metres in the BL, while at small scale, they
behave as the Deardorff mixing length (the size of the grid cell) with a
relatively constant value in the BL of a few tens of metres. Above the BL, the
method reaches its limits as the fluxes and gradients are very small. The
horizontal mixing lengths are larger at the surface, where there is a maximum
of horizontal movements. At mesoscale, the very large horizontal mixing
lengths may result from small horizontal gradients at these scales. The fine
resolutions present horizontal mixing lengths on the order of the vertical
lengths as turbulence is isotropic at those scales.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Numerical weather prediction model forecasts at horizontal grid lengths in
the range of 100 m to 1 km are now possible. This range of scales is in
the “grey zone of turbulence”. Previous studies, based on LES analysis from
the MésoNH model, showed that some assumptions of turbulence schemes on BL
structures are not valid. Indeed, BL thermals are now partly resolved and the
subgrid remaining part of the thermals is possibly largely or completely absent
from the model columns. Moreover, although the turbulence is mainly vertical
at mesoscale, it is isotropic in LES. It has been proved by LES analysis
that, in CBL, the turbulence is neither 1-D nor isotropic in the grey zone.</p>
      <p>At Météo-France, the turbulence scheme is an EDMF. In this study, in
order to model the turbulence at all scales, both the mass flux and the
K-gradient part of the scheme are examined. Firstly, the equations of the
shallow convection (mass flux) scheme have been modified in order to remove
the mesoscale assumptions, which are not valid in the grey zone. These
modifications have been tested in the MésoNH model and in an idealized
version of the operational AROME model. Secondly, horizontal and vertical
mixing lengths have been calculated from LES of neutral and CBL cases at
resolutions in the grey zone. These mixing lengths will be introduced in 3-D
CBR, which will amend the K-gradient scheme in the grey zone. <?xmltex \hack{\newline}?><?xmltex \hack{\newline}?><?xmltex \hack{\noindent\small Edited by: G.-J.~Steeneveld \hack{\newline}
Reviewed by: two anonymous referees}?></p>
</sec>

      
      </body>
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    </app></app-group></back>
    <!--<article-title-html>Representation of the grey zone of turbulence in the atmospheric boundary layer</article-title-html>
<abstract-html><p class="p">Numerical weather prediction model forecasts at horizontal grid lengths in
the range of 100 to 1 km are now possible. This range of scales is the
“grey zone of turbulence”. Previous studies, based on large-eddy simulation
(LES) analysis from the MésoNH model, showed that some assumptions of some turbulence schemes on
boundary-layer structures are not valid. Indeed, boundary-layer thermals are
now partly resolved, and the subgrid remaining part of the thermals is
possibly largely or completely absent from the model columns. First, some
modifications of the equations of the shallow convection scheme have been
tested in the MésoNH model and in an idealized version of the operational
AROME model at resolutions coarser than 500 m. Secondly, although the
turbulence is mainly vertical at mesoscale ( &gt;  2 km resolution), it is
isotropic in LES ( &lt;  100 m resolution). It has been proved by LES analysis
that, in convective boundary layers, the horizontal production of turbulence
cannot be neglected at resolutions finer than half of the boundary-layer height. Thus, in
the grey zone, fully unidirectional turbulence scheme should become
tridirectional around 500 m resolution. At Météo-France, the
dynamical turbulence is modelled by a K-gradient in LES as well as at
mesoscale in both MésoNH and AROME, which needs mixing lengths in the
formulation. Vertical and horizontal mixing lengths have been calculated from
LES of neutral and convective cases at resolutions in the grey zone.</p></abstract-html>
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