On the vertical velocity component in the mesoscale Lofoten vortex of the Norwegian Sea

2017 ◽  
Vol 53 (6) ◽  
pp. 641-649 ◽  
Author(s):  
T. V. Belonenko ◽  
I. L. Bashmachnikov ◽  
A. V. Koldunov ◽  
P. A. Kuibin
2021 ◽  
Author(s):  
Ebba Dellwik ◽  
Poul Hummelshøj ◽  
Gerhard Peters

<p>Sonic anemometers provide point observations of the three-dimensional velocity field at high sampling rates and are crucial instruments for understanding and quantifying the fluxes of momentum, energy and scalars between the atmosphere and Earth’s surface. Since the beginning of sonic anemometry 50 years ago, the characterization of flow distortion, i.e. how the instrument structure alters the flow, has been an ongoing research topic. Multi-path sonic anemometry provides a new opportunity to research and understand flow distortion on the vertical velocity component, since several positions in the small measurement volume can be measured simultaneously. In this work, we use data from a flat terrain measurement campaign in 2020, in which several sonic anemometers were mounted on 4m towers placed 4m apart. The analysis is focused on the Multipath Class-A sonic anemometer (Metek GmbH, Germany), which provides vertical velocity observations from three vertical paths 120 degrees and 0.1m apart. Vertical velocities are also calculated from several combinations of the tilted paths. We investigate how the vertical velocity component is altered depending on wind direction relative to different parts of the instrument structure. We demonstrate that by an optimal combination of the different paths, the vertical velocity variance and fluxes can be significantly enhanced. We also show spectra, and especially look at the high frequency end of the spectrum, where the relative behaviour of the velocity components is known from fundamental turbulence theory. Further, the relative importance of transducer shadowing and pressure-induced blockage effects is discussed.</p>


2000 ◽  
pp. 45
Author(s):  
Rodrigo Da Silva ◽  
Osvaldo Luis Leal de Moraes

In this work it is investigated the turbulence characteristics of the surface boundary layer in conditions of not space homogeneity.The main of the work is to analyze the turbulence intensity and the spectra of the vertical velocity component in terms of the Monin-Obukhov similarity theory. The results are also compared with those obtained in conditions of space homogeneity.The turbulence data were obtained in two fields campaigns accomplished in a region of complex topography. A 12 m micrometeorological tower equipped with fast and slow response sensors was used in both experiments.The nondimensional functions, φw = σw / u* , φθ = σθ / |T* | and φε = kzε / u3* , did not present a consistent dependence with z/L. Suggesting that local scales should be used for their normalization.The normalized spectrum of the vertical velocity component, fSw( f ) /u²*φ2/3ε, was analyzed, for several z/L values in function of the frequency adimensional n = fz /ū . In the high frequency side the spectra converge to a single universal curve that obey the n-2/3 law. However, in the low frequencies side it is not observed a clear separation of the spectra with z/L values.


2005 ◽  
Vol 42 ◽  
pp. 255-261 ◽  
Author(s):  
Jon Ove Hagen ◽  
Trond Eiken ◽  
Jack Kohler ◽  
Kjetil Melvold

AbstractThe geometry of glaciers is affected by both the mass balance and the dynamics. We present repeated GPS measurements of longitudinal altitude profiles on three glaciers in Svalbard and show that surface altitude changes alone cannot be used to assess the mass balance. The three measured glaciers are in different dynamic modes, and the observed changes in geometry are strongly affected by the dynamics. Nordenskiöldbreen shows no significant change in the geometry, indicating that the mass balance is in steady state with the dynamics. On Amundsenisen the surface has lowered by 1.5–2.0 ma–1 in the lower part of the accumulation area at 520–550m a.s.l., indicating that the ice flux is higher than the mass-balance input, probably due to a surge advance of the glacier further downstream affecting the higher part of the drainage area. On Kongsvegen the opposite situation was found. Here the geometry of the profile showed a clear build-up of 0.5 ma–1 in the accumulation area and a lowering of 1 ma–1 in the lower part of the ablation area. The ice velocity is very low, giving a negligible vertical velocity component and an ice flux that is far smaller than the mass-balance flux, indicating that the glacier is building up towards a surge advance. Our results show that if mapping of height changes is to be used to monitor the response of the glaciers to climate change, both surface net mass-balance data and dynamic data are needed.


2009 ◽  
Vol 5 (S266) ◽  
pp. 380-383
Author(s):  
E. A. De Souza–Rossetto ◽  
H. J. Rocha–Pinto

AbstractThe globular cluster luminosity function distribution shows a peak at MV ≈ −7.5 mag. There are some indications that the kinematic parameters are correlated with luminosity. In particular, Alfaro et al. (2001) have studied the properties of the Galactic globular cluster system and they found a correlation between spatial-velocity component and globular cluster absolute magnitude. The authors assumed that the globular clusters can be separated into two groups. The first is composed of globular clusters with MV < −7.5 mag and moving preferentially towards the north Galactic pole, while the faintest globular clusters, composing the second group, move towards the Galactic disk. We have selected a sample of globular clusters using the same criteria as Alfaro et al. (2001) and have checked that this apparent relation indeed exists. Nevertheless, we decided to investigate whether it could be a fortuitous relation or an intrinsic property by checking its validity for eight different epochs at past and future times. The orbital parameters for the globular clusters at these eight epochs were found by orbital integration using a typical Galactic potential. We show that this relation between the vertical velocity component and the absolute magnitude among globular clusters is not coherent with time and the velocity distribution does not support the hypothesis of Alfaro et al. for the existence of two dynamical groups of globular clusters.


1975 ◽  
Vol 70 (2) ◽  
pp. 251-255 ◽  
Author(s):  
C. C. Tung

The probability density function and the first three statistical moments of the velocity, acceleration and dynamic pressure are obtained for a Gaussian, stationary, homogeneous, random gravity-wave field in deep water, using infinitesimal wave solutions. It is shown that the velocity, acceleration and pressure are non-Gaussian. While the horizontal accelerations and vertical velocity component are of zero mean and unskewed, the dynamic pressure, vertical acceleration and horizontal velocity components are skewed and have non-zero mean.


2018 ◽  
Vol 68 (12) ◽  
pp. 1711-1725 ◽  
Author(s):  
Igor Bashmachnikov ◽  
Tatyana Belonenko ◽  
Pavel Kuibin ◽  
Denis Volkov ◽  
Victor Foux

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