WINDBLOWN DUST ON MARS

被引:98
作者
SAGAN, C
POLLACK, JB
机构
[1] Laboratory for Planetary Studies, Cornell University, Center for Radiophysics and Space Research, Ithaca
关键词
D O I
10.1038/223791a0
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 wave of darkening in the Martian springtime, which some say may have a biological explanation, can be explained in terms of windblown dust. © 1969 Nature Publishing Group.
引用
收藏
页码:791 / &
相关论文
共 28 条
[1]  
[Anonymous], 1962, PHOTOGRAPHIC STORY M
[2]  
BAGNOLD RA, 1941, PHYSICS BLOWN SAND D
[3]  
BAGNOLD RA, 1941, PHYSICS BLOWN SAND D, P76
[4]  
DEVAUCOULEURS G, 1954, PHYSICS PLANET MARS
[5]  
DOLLFUS A, 1965, ANN ASTROPHYS, V28, P722
[6]  
DOLLFUS A, 1957, ANN ASTROPHYS S4
[7]  
FOCAS JH, 1961, ANN ASTROPHYS, V24, P309
[8]   AN APPROXIMATE CALCULATION OF RADIATIVE HEATING AND RADIATIVE EQUILIBRIUM IN MARTIAN ATMOSPHERE [J].
GIERASCH, P ;
GOODY, R .
PLANETARY AND SPACE SCIENCE, 1967, 15 (10) :1465-&
[9]   A STUDY OF THERMAL AND DYNAMICAL STRUCTURE OF MARTIAN LOWER ATMOSPHERE [J].
GIERASCH, P ;
GOODY, R .
PLANETARY AND SPACE SCIENCE, 1968, 16 (05) :615-&
[10]  
Ives R.L., 1947, B AM METEOROL SOC, V28, P168, DOI DOI 10.1175/1520-0477-28.4.168