scholarly journals Stellar scintillations in a spaceborne occultation experiment for atmospheric irregularities with the variable anisotropy

2015 ◽  
Vol 28 (11) ◽  
Keyword(s):  
2021 ◽  
Vol 9 (1) ◽  
pp. 65-89
Author(s):  
Zhenzhen Yang ◽  
Yajuan Yang ◽  
Jiawei Sun ◽  
Baode Li

Abstract Let p(·) : ℝ n → (0, ∞] be a variable exponent function satisfying the globally log-Hölder continuous and let Θ be a continuous multi-level ellipsoid cover of ℝ n introduced by Dekel et al. [12]. In this article, we introduce highly geometric Hardy spaces Hp (·)(Θ) via the radial grand maximal function and then obtain its atomic decomposition, which generalizes that of Hardy spaces Hp (Θ) on ℝ n with pointwise variable anisotropy of Dekel et al. [16] and variable anisotropic Hardy spaces of Liu et al. [24]. As an application, we establish the boundedness of variable anisotropic singular integral operators from Hp (·)(Θ) to Lp (·)(ℝ n ) in general and from Hp (·)(Θ) to itself under the moment condition, which generalizes the previous work of Bownik et al. [6] on Hp (Θ).


Ground Water ◽  
2015 ◽  
Vol 53 (6) ◽  
pp. 955-958 ◽  
Author(s):  
Andrea Borghi ◽  
Philippe Renard ◽  
Gabriel Courrioux

2014 ◽  
Vol 7 (6) ◽  
pp. 1861-1872 ◽  
Author(s):  
V. Kan ◽  
V. F. Sofieva ◽  
F. Dalaudier

Abstract. In this paper, we consider possibilities for studying the anisotropy of small-scale air density irregularities using satellite observations of bi-chromatic stellar scintillations during tangential occultations. Estimation of the anisotropy coefficient (the ratio of the characteristic horizontal to vertical scales) and other atmospheric parameters is based on the comparison of simulated/theoretical and experimental auto-spectra and coherency spectra of scintillation. Our analyses exploit a 3-D model of the spectrum of atmospheric inhomogeneities, which consists of anisotropic and isotropic components. For the anisotropic component, a spectral model with variable anisotropy is used. Using stellar scintillation measurements by GOMOS (Global Ozone Monitoring by Occultation of Stars) fast photometers, estimates of the anisotropy coefficient are obtained for atmospheric irregularities with vertical scales of 8–55 m at altitudes of 43–30 km. It is shown that the anisotropy increases from about 10 to 50 with increasing vertical scales.


2009 ◽  
Vol 80 (2) ◽  
Author(s):  
Ippei Kishida ◽  
Fumiyasu Oba ◽  
Yukinori Koyama ◽  
Akihide Kuwabara ◽  
Isao Tanaka

1997 ◽  
Vol 102 (D16) ◽  
pp. 19449-19459 ◽  
Author(s):  
Francis Dalaudier ◽  
Alexandre S. Gurvich

2007 ◽  
Vol 90 (16) ◽  
pp. 162501 ◽  
Author(s):  
Miguel González-Guerrero ◽  
José Luis Prieto ◽  
David Ciudad ◽  
Pedro Sánchez ◽  
Claudio Aroca

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
E. Saavedra ◽  
A. Riveros ◽  
J. L. Palma

AbstractThe high frequency dynamic behaviors of magnetic nanorings with variable anisotropy along their radius have been studied using micromagnetic simulations. The dynamic susceptibility spectrum and spatial localization of the ferromagnetic resonance modes are investigated by varying anisotropy gradients in nanorings of 200 nm of external radius, with different internal radii. Both the resonant frequencies and the number of peaks depend on the lower energy magnetization configuration which in turn is a function of anisotropy gradients. Besides, it is shown that the effects of the anisotropy gradient are relevant even for the narrowest ring of 10 nm wide. The idea of controlling frequencies by modifying the anisotropy gradients of the system suggests the possibility of using these nanostructures in potential magnetic controllable frequency devices.


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