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Data & statistics on mean total kinetic energy spectra as func – 5455 results

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I. Parameters for the simulations. SP50 denotes the self-propelled wake with 50% mean kinetic energy and energy spectrum A, TP1 denotes the turbulent patch with spectrum B, and TP2 denotes the turbulent patch with spectrum C. Case SP10 is a self-propelled wake with 10% mean kinetic energy and case TP10 corresponds to a turbulent patch with a similar energy spectrum (spectra E and F, respectively). ...
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I. Parameters for the simulations. SP50 denotes the self-propelled wake with 50% mean kinetic energy and energy spectrum A, TP1 denotes the turbulent patch with spectrum B, and TP2 denotes the ...

www.mech.kth.se/~matds/docs/Pal_SS_PF_2013.pdf

is 0.3 whereas for case SP10, U0 = 0.11, implying that SP50 has ∼50% mean kinetic energy of the total in comparison to ∼10% in SP10. As in our previous work ...
in time. The initial mean velocity profile used for the self-propelled wake cases SP50

Sep 2013 | www.mech.kth.se – 8 more results from this site
Original Url: http://www.mech.kth.se/~matds/docs/Pal_SS_PF_2013.pdf
Time- and depth-averaged horizontal kinetic energy spectra (Re eff = 6600): BOUS (Ro r = 0.5, black) and QG (blue). Spectra are normalized by the mean of kinetic energy Ek . A red line ∝ k −5/3 is plotted for comparison.

Time- and depth-averaged horizontal kinetic energy spectra (Re eff = 6600): BOUS (Ro r = 0.5, black) and QG (blue). Spectra are normalized by the mean of kinetic energy Ek . A red line ∝ k −5/3 is ...

www.locean-ipsl.upmc.fr/~Xavier.Capet/publications/papers/JFM_10_Molemaker.pdf

of the kinetic energy spectrum ∼Kh (figure 13). By wavenumber extrapolation, this implies ...
, z), the fluctuation kinetic energy as a function of horizontal wavenumber (kx , ky ) and z using ...
which is computed by means of the (root mean square) r.m.s. value of the non-dimensional

Jun 2010 | www.locean-ipsl.upmc.fr
Original Url: http://www.locean-ipsl.upmc.fr/~Xavier.Capet/publications/papers/JFM_10_Molemaker.pdf
Convergence rates of the gPC representation for the 643 case. (a) L2 norms of the error in the mean kinetic energy and enstrophy spectra versus number of quadrature points; Cs follows U (0.35, 0.35). (b) L2 norms of the error in kinetic energy and enstrophy spectra versus polynomial order P . Two different Smagorinsky constant ranges are presented: large range: Cs follows U (0.35, 0.35) and small range: ...
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Convergence rates of the gPC representation for the 643 case. (a) L2 norms of the error in the mean kinetic energy and enstrophy spectra versus number of quadrature points; Cs follows U (0.35, 0.35 ...

people.mech.kuleuven.be/~jmeyers/resources/downloads/Lucor_Meyers_Sagaut_JFM585.pdf

on the energy spectra E(k, t), representative of the convergence of large-scale flow features ...
Kinetic energy Enstrophy 10–1 [%] 10–2 µ 10–3 10–4 10–5 (a) 10–6 ...
to the parameter Cs by means of generalized polynomial chaos. This provides an elegant

Jul 2007 | people.mech.kuleuven.be – 9 more results from this site
Original Url: http://people.mech.kuleuven.be/~jmeyers/resources/downloads/Lucor_Meyers_Sagaut_JFM585.pdf
Final-time energy properties of singular vectors, with initial amplitudes multiplied by α = 5 and propagated by the tangent-linear model: (a) the dry energy partitioned in kinetic, potential and surface-pressure terms, (b) the potential, kinetic and total energy spectra and (c) the mean energy distribution. (d)–(f) are as (a)–(c), but from the nonlinear model.
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Final-time energy properties of singular vectors, with initial amplitudes multiplied by α = 5 and propagated by the tangent-linear model: (a) the dry energy partitioned in kinetic, potential and ...

collaboration.cmc.ec.gc.ca/science/rpn/publications/pdf/QJ_Zadra_2004_22_11_04_official.pdf

energy partitioned in kinetic, potential and surface-pressure terms, (b) the potential, kinetic and total energy spectra and (c) the mean energy distribution ...
For α = 1 (Figs. 10(a), (b), (c)) the nonlinear propagation gives a larger energy ...
◦ N, the energy distribution, after the appropriate rescaling, is similar to the one produced

Nov 2004 | collaboration.cmc.ec.gc.ca – 7 more results from this site
Original Url: http://collaboration.cmc.ec.gc.ca/science/rpn/publications/pdf/QJ_Zadra_2004_22_11_04_official.pdf
Of spherical shell averaged potential and kinetic energy spectra for data #2 at time t = 6. The high wave number scaling is k−1 indicating that in this representation the energy is dominated by waves. Inset: same spectra averaged over time 3 t 6 shows that the spectra have converged over the time period that the mean potential enstrophy becomes constant (see fig. 1).

Of spherical shell averaged potential and kinetic energy spectra for data #2 at time t = 6. The high wave number scaling is k−1 indicating that in this representation the energy is dominated by waves ...

math.lanl.gov/~skurien/papers/KurienWinTay_epl08.pdf

and potential energy spectra for our simulation, computed as follows: ...
of the Laplacian leads to an enhanced bottleneck in the energy spectrum, to be interpreted ...
the coefficient of the viscous term in order that the energy in the largest shell is resolved

Oct 2008 | Mathematical Modeling and Analysis
Original Url: http://math.lanl.gov/~skurien/papers/KurienWinTay_epl08.pdf
Monthly variations of the characteristic wave numbers (upper panel), spectral amplitudes (middle panel) and slopes (bottom panel) of the mean vertical wave number spectra for GWs in the troposphere over Wuhan station. The solid, dotted and dashed curves denote the spectral parameters for the zonal kinetic energy, meridional kinetic energy and potential energy densities, respectively.

Monthly variations of the characteristic wave numbers (upper panel), spectral amplitudes (middle panel) and slopes (bottom panel) of the mean vertical wave number spectra for GWs in the troposphere ...

www.ann-geophys.net/24/3257/2006/angeo-24-3257-2006.pdf

5, but for the monthly variations of the spectral parameters of the mean vertical wave number spectra ...
Figures 5 and 6 demonstrate the monthly variations of the spectral parameters for the averaged vertical wave number spectra in the troposphere and stratosphere over Wuhan

Dec 2006 | www.ann-geophys.net
Original Url: http://www.ann-geophys.net/24/3257/2006/angeo-24-3257-2006.pdf
The kinetic energy spectra for glevel-11 in the zonal wavenumber domain for the different latitudinal circle. The red, green, blue lines are the tropics, mid-latitudes, and polar region, respectively. The solid black line represents the global mean of kinetic energy.

The kinetic energy spectra for glevel-11 in the zonal wavenumber domain for the different latitudinal circle. The red, green, blue lines are the tropics, mid-latitudes, and polar region, respectively ...

www.tulips.tsukuba.ac.jp/dspace/bitstream/2241/104814/1/sola_5(180).pdf

Terasaki et al., Characteristics of the Kinetic Energy Spectrum of NICAM Model Atmosphere

Dec 2009 | redirect
Original Url: http://www.tulips.tsukuba.ac.jp/dspace/bitstream/2241/104814/1/sola_5(180).pdf
Sampled THz vector potential. Series of kinetic energy spectra of 5p electrons detached from xenon atoms by a 13.5 nm XUV pulse in the presence of an intense pulsed THz field. The energy shift of the electrons versus the XUV/THz delay directly represents the vector potential ATHz . The less intense electron signal at lower energies stems from stronger bound xenon 5s electrons. The spectra shown in (a) ...

Sampled THz vector potential. Series of kinetic energy spectra of 5p electrons detached from xenon atoms by a 13.5 nm XUV pulse in the presence of an intense pulsed THz field. The energy shift of the ...

peer.mpdl.mpg.de/pubman/item/peer:48027:1/component/peer:48025/PEER_stage2_10.1088_slsh_0953-4075_slsh_43_slsh_19_slsh_194010.pdf

a series of kinetic energy spectra of Xe 5p photoelectrons detached by 13.5 nm FLASH ...
By analyzing the fluctuation of the mean energy of single-shot photoelectron spectra ...
Time-diagnostics for improved dynamics experiments at XUV FELs (a) (b) Electron kinetic energy (eV) Electron kinetic energy (eV) Time delay (ps) Time delay (ps)

May 2010 | Publication Manager
Original Url: http://peer.mpdl.mpg.de/pubman/item/peer:48027:1/component/peer:48025/PEER_stage2_10.1088_slsh_0953-4075_slsh_43_slsh_19_slsh_194010.pdf
The spectra of the velocity correlations along the line-of-sight of the lidar following the procedure outlined in Gal-Chen et al (1992). Fitting a -5/3 slope to the power spectra shown in figure 4 we can estimate the kinetic energy dissipation rate for the three data sets. The kinetic energy dissipation rates for the three sets of data are shown in table 1.

The spectra of the velocity correlations along the line-of-sight of the lidar following the procedure outlined in Gal-Chen et al (1992). Fitting a -5/3 slope to the power spectra shown in figure 4 we ...

www.geo.uni.lodz.pl/~icuc5/text/P_6_1.pdf

corrected values of kinetic energy dissipation rate, integral length scale and velocity ...
was pointed perpendicular to the mean wind direction. The wind profiles calculated from the lidar data are shown in figure 2. During the experiment the mean wind direction ...
May02-1 May02-2 May03-3 hei ght (m ) 2 -2 Radial Velocity Variance (m s ) Figure 3: Radial velocity wind variance profiles taken Figure 4: spectra of the velocity correlations along the

Jan 1992 | Wydział Nauk Geograficznych UŁ - Strona główna
Original Url: http://www.geo.uni.lodz.pl/~icuc5/text/P_6_1.pdf
Near rotor wake; (a) distributions of turbulent kinetic energy and relative streamlines; and (b) 1-D spatial energy-density spectra along the sample lines indicated in (a). The rotor trailing edge is located at (0,0). Solid line: E11(k1); dotted line: 3/4 E22(k1); dashed line: a -5/3 slope line fits E11(k1). Estimated turbulent kinetic energy dissipation rate, ε (calculated using Equation 6), and Kolmogorov ...
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Near rotor wake; (a) distributions of turbulent kinetic energy and relative streamlines; and (b) 1-D spatial energy-density spectra along the sample lines indicated in (a). The rotor trailing edge is ...

www.me.jhu.edu/~lefd/turbo/papers/chow_etal_igti2003.pdf

is characterized by elevated turbulent kinetic energy, concentrated vorticity (as seen in Figure 2c) as well as quadruple distributions of Reynolds shear stress and mean shear

Feb 2003 | Johns Hopkins University Whiting School of Engineering – 9 more results from this site
Original Url: http://www.me.jhu.edu/~lefd/turbo/papers/chow_etal_igti2003.pdf
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