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恶劣可怕的火星环境 被引量:2

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作者 吴国兴
出处 《太空探索》 2005年第5期18-20,共3页 Space Exploration
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  • 1Acuna M H, Connerney J E P, Wasilewski P, et al. The magnetic field of Mars-Summary of results from the aerobraking and mapping orbits I J ]. J. Geophys. Res. ,2001,106:23403 - 23418.
  • 2Lei F, Hands A, Clucas S, et al. Improvement to and validations of the QinetiQ atmospheric radiation model (QARM) [ J ]. IEEE Trans. Nucl. Sci. , 2006,53 ( 4 ) : 1851 - 1858.
  • 3Margarita M Marinova, Oded Aharonson, Erk As- phaug. Mega-impact formation of the Mars hemispher- ic dichotomy[ J]. Nature,2008 (453) : 1216 - 1219.
  • 4G. De Angelis. Modeling of the Martian environment for radiation analysis [ J ]. Nuclear Physics, 2007, B166 : 184 - 202.
  • 5Zurek R W, Martin L J. Interannual variability of plan- etencircling dust storms on Mars [ J ]. J. Geophys. Res. ,1993(98) :3247 -3259.
  • 6Hourdin F, P Le Van, F Forget, et al. Meteorological variability and the annual surface pressure cycle on Mars[ J]. J. Atmos. Sci. , 1993 (50) :3625 - 3640.
  • 7Barnes J R. Time spectral analysis of mid - latitude disturbances in the Martian atmosphere [ J ]. J. Atmos. Sci. , 1980 ( 37 ) :2002 - 2015.
  • 8Barnes J R. Midlatitude disturbances in the Martian at- mosphere: a second Mars year [ J ]. J. Atmos. Sci., 1981(38) :225 - 234.
  • 9Collins M, S R Lewis, P L Read, et al. Baroclinic wave transitions in the Martian atmosphere [ J ]. Ica- rus, 1996(120) :344 - 357.
  • 10Seiff A, D B Kirk. Structure of the atmosphere of Mars in summer at mid - latitudes [ J ]. J. Geophys. Res. , 1977 (82) : 4364 - 4378.

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