The Mars Pathfinder atmospheric structure investigation meteorology (ASI/MET) experiment

被引:358
作者
Schofield, JT
Barnes, JR
Crisp, D
Haberle, RM
Larsen, S
Magalhaes, JA
Murphy, JR
Seiff, A
Wilson, G
机构
[1] OREGON STATE UNIV,COLL OCEAN & ATMOSPHER SCI,CORVALLIS,OR 97331
[2] NASA,AMES RES CTR,MOFFETT FIELD,CA 94035
[3] RISO NATL LAB,DK-4000 ROSKILDE,DENMARK
[4] SAN JOSE STATE UNIV FDN,SAN JOSE,CA
[5] ARIZONA STATE UNIV,TEMPE,AZ
关键词
D O I
10.1126/science.278.5344.1752
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment measured the vertical density, pressure, and temperature structure of the martian atmosphere from the surface to 160 km, and monitored surface meteorology and climate for 83 sols (1 sol = 1 martian day = 24.7 hours). The atmospheric structure and the weather record are similar to those observed by the Viking 1 lander (VL-1) at the same latitude, altitude, and season 21 years ago, but there are differences related to diurnal effects and the surface properties of the landing site. These include a cold nighttime upper atmosphere; atmospheric temperatures that are 10 to 12 degrees kelvin warmer near the surface; light slope-controlled winds; and dust devils, identified by their pressure, wind, and temperature signatures. The results are consistent with the warm, moderately dusty atmosphere seen by VL-1.
引用
收藏
页码:1752 / 1758
页数:7
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