火星大气环流模型研究进展Evolvement of Mars Atmospheric Circulation Model
杨瑞琰;闫霏霏;黄定华;肖龙;张振飞;
摘要(Abstract)：
火星尘暴是火星上特有的大气运动,也是人类登陆火星的主要障碍。考虑到火星的具体情况,早期针对火星大气的研究主要集中在实验室的物理模拟实验,建立火星大气实验室,研究在火星大气条件下火星尘埃扬起的机制等方面。同时根据地球大气物理的运动方程、能量方程和质量守恒方程,并与早期的火星观测数据进行比较,从而建立起火星大气环流的一般模型(GC-Ms)。GCMs模型对大中尺度的模拟计算能够取得好的效果,但对小尺度的计算很困难,为研究火星大量中等尺度和小尺度的大气环流现象(如尘暴的发生机制等),近来已经建立起了适合火星区域大气环流系统的模型(MRAMS)。MRAMS同时也是Mars Global Surveyor(MGS)用来处理高分辨率资料的理想工具。
关键词(KeyWords)： 火星;大气;环流;模型
基金项目(Foundation):
作者(Author): 杨瑞琰;闫霏霏;黄定华;肖龙;张振飞;
Email:
DOI:
参考文献(References)：
- [1]Greeley R,White B R,Leach R N,et al.Mars:Windfriction speeds for particle movement[J].Geophys.Res.Lett.,1976,(3):417-420.
- [2]Greeley R,Leach R,White B R,et al.Threshold windspeeds for sand on Mars:Windtunnel si mulations[J].Geophys.Res.Lett.,1980,(7):121-124.
- [3]White B R,Lacchia B M,Greeley R,et al.Aeolian behaviour of dust in a si mulated Martian environment[J].J.Geophys.Res.,1997,102(E11):25629-25640.
- [4]Greeley R,Iversen J D.Wind as a geological process on earth,mars,venus,and Titan[M].Cambridge:Cambridge Univer-sity Press,1985:1-333.
- [5]Greeley R,Whelley P L,Neakrase L D V.Martian dust dev-ils:Directions of movement inferredfromtheir tracks[J].Geo-phys.Res.Lett.,2004,31(24):L24702.
- [6]Mintz Y.The general circulation of planetary at mospheres[C]∥Kellog W W,Sagan C.The At mospheres of Mars and Ve-nus.[S.l.]:[s.n.],1961,NAS NRC944,107146.
- [7]Gierasch PJ,Goody R M.An approxi mate calculation of radi-ative heating and radiative equilibriumin the Martian at mos-phere[J].Plan.Space Sci.,1967,15:1465-1477.
- [8]Leovy C,Mintz Y.Numerical si mulation of the at mospheric circulation and cli mate of Mars[J].J.At mos.Sci.,1969,26(6):1167-1190.
- [9]Goody R M,Belton M J S.Radiative relaxation ti mes for Mars:A discussion of Martian at mospheric dynamics[J].Plan.Space Sci.,1967,15:247-256.
- [10]Mass C,Sagan C.Anumerical circulation model withtopogra-phy for the Martian southern hemisphere[J].J.At mos.Sci.,1976,33:1418-1430.
- [11]Rafkin S C R,Haberle R M,Michaels TI.The mars regional at mospheric modeling system-model description[J].Icarus,2001,151:228-256.
- [12]Pielke R A,Cotton W R,Walko R L,et al.Acomprehensive meteorological modeling system-RAMS[J].Meteorol.At mos.Phys.,1992,49:69-91.
- [13]Haberle R M,Joshi M M,Murphy J R,et al.General circula-tion model si mulations of the Mars Pathfinder at mospheric structure investigation/meteorology data[J].J.Geophys.Res.,1999,104:8957-8974.
- [14]Haberle R M,Houben H C,Hertenstein R,et al.A bound-arylayer model for Mars:Comparison with vikinglander entry data[J].J.At mos.Sci.,1993,50:1545-1559.
- [15]Haberle R M,Pollack J B,Barnes J R,et al.Mars at mos-pheric dynamics as si mulated by the NASA-Ames general cir-culation model(I):The zonal mean circulation[J].J.Geo-phys.Res.,1993,98:3093-3123.
- [16]Seiff A.Mars at mospheric winds indicated by motion of the Viking landers during parachute descent[J].J.Geophys.Res.,1993,98:7461.
- [17]Seiff A,Kirk D B.Structure of the at mosphere of Mars in summer at mid-latitudes[J].J.Geophys.Res.,1977,82:4364-4378.
- [18]达道安,杨亚天,涂建辉.太阳系行星及行星际大气环境特性研究[J].宇航学报,2006,27(6):1306-1313.