Description, accessibility and usage of SOIR/Venus Express atmospheric profiles of Venus distributed in VESPA (Virtual European Solar and Planetary Access)

被引:8
作者
Trompet, L. [1 ]
Geunes, Y. [1 ]
Ooms, T. [1 ]
Mahieux, A. [1 ,2 ]
Wilquet, V. [1 ]
Chamberlain, S. [1 ]
Robert, S. [1 ]
Thomas, I. R. [1 ]
Erard, S. [3 ]
Cecconi, B. [3 ]
Le Sidaner, P. [4 ]
Vandaele, A. C. [1 ]
机构
[1] Royal Belgian Inst Space Aeron, 3 Av Circulaire, B-1180 Brussels, Belgium
[2] Fonds Natl Rech Sci, Brussels, Belgium
[3] Univ Paris Diderot, PSL Res Univ, CNRS, LESIA,Observ Paris,UPMC,UMR8109, 5 Pl J Janssen, F-92195 Meudon, France
[4] PSL Res Univ, CNRS, Observ Paris, DIO,UMS2201, 61 Av Observ, F-75014 Paris, France
关键词
Data service; Planetary atmosphere; Vertical profiles; Venus; CALIBRATION; SPECTRA;
D O I
10.1016/j.pss.2017.04.022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Venus Express SOIR profiles of pressure, temperature and number densities of different constituents of the mesosphere and lower thermosphere of Venus are the only experimental data covering the 60 km to 220 km range of altitudes at the terminator of Venus. This unique dataset is now available in the open access VESPA infrastructure. This paper describes the content of these data products and provides some use cases.
引用
收藏
页码:60 / 64
页数:5
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