PLANETARY-SCALE WAVE STRUCTURE IN THE MARTIAN ATMOSPHERE

被引：57
作者：
CONRATH, BJ
机构：
来源：
ICARUS | 1981年 / 48卷 / 02期
关键词：
D O I：
10.1016/0019-1035(81)90107-X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：246 / 255
页数：10
相关论文
共 23 条
[1]  
BARNES JR, 1981, J ATMOS SCI, V38, P225, DOI 10.1175/1520-0469(1981)038<0225:MDITMA>2.0.CO
[2]  
2
[3]  
BARNES JR, 1980, J ATMOS SCI, V37, P2002, DOI 10.1175/1520-0469(1980)037<2002:TSAOMD>2.0.CO
[4]  
2
[5]   PROPAGATION OF PLANETARY-SCALE DISTURBANCES FROM LOWER INTO UPPER ATMOSPHERE [J].
CHARNEY, JG ;
DRAZIN, PG .
JOURNAL OF GEOPHYSICAL RESEARCH, 1961, 66 (01) :83-+
[6]   ATMOSPHERIC AND SURFACE PROPERTIES OF MARS OBTAINED BY INFRARED SPECTROSCOPY ON MARINER-9 [J].
CONRATH, B ;
CURRAN, R ;
HANEL, R ;
KUNDE, V ;
MAGUIRE, W ;
PEARL, J ;
PIRRAGLIA, J ;
WELKER, J ;
BURKE, T .
JOURNAL OF GEOPHYSICAL RESEARCH, 1973, 78 (20) :4267-4278
[7]   THERMAL STRUCTURE OF MARTIAN ATMOSPHERE DURING DISSIPATION OF DUST STORM OF 1971 [J].
CONRATH, BJ .
ICARUS, 1975, 24 (01) :36-46
[8]  
CONRATH BJ, 1976, J ATMOS SCI, V33, P2430, DOI 10.1175/1520-0469(1976)033<2430:IOPSTO>2.0.CO
[9]  
2
[10]  
CONRATH BJ, 1977, INVERSION METHODS AT
123