The atmospheres of Venus and Mars : proceedings of the C3.1 Meeting of COSPAR Scientific Commission C which was held during the Thirtieth COSPAR Scientific Assembly, Hamburg, Germany, 11-21 July, 1994
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書誌事項
The atmospheres of Venus and Mars : proceedings of the C3.1 Meeting of COSPAR Scientific Commission C which was held during the Thirtieth COSPAR Scientific Assembly, Hamburg, Germany, 11-21 July, 1994
（Advances in space research, vol. 16,
published for the Committee on Space Research [by] Pergamon, 1995
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注記
Includes bibliographical references and index
内容説明・目次
内容説明
The atmospheres of the other terrestrial planets remain a focus of considerable interest. A highlight of current studies is numerical modelling, particularly general circulation models of the Martian atmosphere. The continued interest in Martian dynamics is complemented by recent developments in understanding photochemistry and the origins of the Martian atmosphere. Some of the results from the recent Russian Phobos missions relate to this, particularly with reference to aerosol properties and anomolous water vapour abundances on Mars. Fresh information has been acquired regarding the deep atmosphere of Venus from the newly discovered near infrared atmospheric "windows" from both ground-based and Galileo - NIMS spectral observations in this spectral region. It has become clear that the Venusian tropopause has a complicated dynamical structure, as well as a complex chemical and radiative environment. Some species, such as carbon monoxide, are globally variable and probably act as tracers for the global circulation.
Water vapour, on the other hand, seems to be well mixed both horizontally and vertically, but with a much smaller abundance than had been inferred from earlier measurements. New intelligence concerning upper atmosphere temperature structure is still being gathered from Pioneer, Vega and Venera observations and radio occultation experiments. This volume contains a selection of papers presented at the C3.1. Meeting of COSPAR Scientific Commission C.
目次
- Regular and irregular baroclinic waves in a Martian general circulation model - a role for diurnal forcing?, M. Collins et al
- an operational data assimilation scheme for the Martian atmosphere, S.R. Lewis and P.L. Read
- aspects of atmospheric science and instrumentation for Martian missions, A.-M. Harri et al
- evidences of the regolith-atmosphere water exchange on Mars from the ISM (phobos-2) infrared spectrometer observations, D.V. Titov et al
- experimental data on aerosols on Mars - viking, phobos and future missions, V.I. Moroz
- numerical simulations of the nearsurface phenomena on Mars, K.V. Karelsky and A.S. Petrosyan
- O+ escape in the polar ion exosphere of Mars, S.A. Haider
- photochemistry and stability of the atmosphere of Mars, S.K. Atreya and Z.G. Gu
- a simple test of the induced nature of the Martian tail, C.T. Russell et al
- removal of Mars atmospheric gas absorption from phobos-2/ISM spectra, M.M. Castronuovo and C. Ulivieri
- carbon monoxide in the deep atmosphere of Venus, F.W. Taylor
- the structure of the Venusian atmosphere at high latitudes, L.V. Zasova
- the nightward ion flow scenario at Venus revisited, L.H. Brace et al
- PASDA - a tool to design atmospheric descent bodies with parachutes, D. Adler et al.
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