Using stellar scintillation for studies of turbulence in the Earth's atmosphere

被引：9

作者：

Sofieva, V. F. ^{[1
]}

Dalaudier, F. ^{[2
]}

Vernin, J. ^{[3
]}

机构：

[1] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland

[2] Univ Paris 06, Univ Versailles St Quentin, CNRS INSU, LATMOS IPSL, F-78280 Guyancourt, France

[3] Univ Nice Sophia Antipolis, Observ Cote Azur, Lab Lagrange, CNRS UMR7293, F-06108 Nice 2, France

来源：

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2013年 / 371卷 / 1982期

基金：

美国国家科学基金会; 芬兰科学院;

关键词：

stellar scintillation; atmosphere; turbulence; gravity waves; remote sensing; AIR DENSITY IRREGULARITIES; SCALE ELIMINATION MODEL; GRAVITY-WAVE CAMPAIGN; SPACECRAFT OBSERVATIONS; INTERNAL WAVES; INTENSITY SCINTILLATION; REFRACTIVE-INDEX; 3-DIMENSIONAL SPECTRUM; PLANETARY ATMOSPHERES; CHROMATIC REFRACTION;

D O I：

10.1098/rsta.2012.0174

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Stellar scintillation observed through the Earth's atmosphere is the result of interaction of light waves and the turbulent atmosphere. This review is dedicated to using stellar scintillation measurements for studies of turbulence in the Earth's atmosphere. We present an overview of ground-based, airborne and satellite stellar scintillation measurements, discuss the approaches to data analyses and give an overview of the main geophysical results. We also discuss the benefits of the scintillation method in studies of the structure of air density irregularities and its limitations.

引用

页数：23

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