Curvilinear features in the southern hemisphere observed by Mars Global Surveyor Mars Orbiter Camera

详细信息    查看全文

• 作者：Huiqun  ; Wang^a ;   ; ^{hwang@cfa.harvard.edu} ; Anthony D.  ; Toigo^b ;   ; ¹ ; Mark I.  ; Richardson^c
• 关键词：Atmospheres ; Dynamics ; Atmospheres ; Structure ; Mars ; Atmosphere
• 刊名：Icarus
• 出版年：2011
• 出版时间：September 2011
• 年：2011
• 卷：215
• 期：1
• 页码：242-252
• 全文大小：2591 K

文摘

We have used the complete set of Mars Global Surveyor (MGS) Mars Daily Global Maps (MDGMs) to study martian weather in the southern hemisphere, focusing on curvilinear features, including frontal events and streaks. ¡°Frontal events?refer to visible events that are morphologically analogous to terrestrial baroclinic storms. MDGMs show that visible frontal events were mainly concentrated in the 210?00¡ãE (60?50¡ãW) sector and the 0?0¡ãE sector around the southern polar cap during L_s = 140?50¡ã and L_s = 340?0¡ã. The non-uniform spatial and temporal distributions of activity were also shown by MGS Thermal Emission Spectrometer transient temperature variations near the surface. ¡°Streaks?refer to long curvilinear features in the polar hood or over the polar cap. They are an indicator of the shape of the polar vortex. Streaks in late winter usually show wavy segments between the 180¡ã meridian and Argyre. Model results suggest that the zonal wave number m = 3 eastward traveling waves are important for their formation.