| contributor author | Gierasch, P. J. | |
| contributor author | Goody, R. M. | |
| date accessioned | 2017-06-09T14:16:47Z | |
| date available | 2017-06-09T14:16:47Z | |
| date copyright | 1973/03/01 | |
| date issued | 1973 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-16315.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4152085 | |
| description abstract | We have used Carrier's model of a terrestrial hurricane, with modified thermodynamic drive, to describe the 1971 Great dust storm on Mars. The model predicts the course of development and the time elapsing in three different phases: growth, mature and decay. All predictions correspond reasonably well with the observed phenomenon. We also offer explanations for the rarity of the storms and the time of year and location at which they most commonly commence. | |
| publisher | American Meteorological Society | |
| title | A Model of a Martian Great Dust Storm | |
| type | Journal Paper | |
| journal volume | 30 | |
| journal issue | 2 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1973)030<0169:AMOAMG>2.0.CO;2 | |
| journal fristpage | 169 | |
| journal lastpage | 179 | |
| tree | Journal of the Atmospheric Sciences:;1973:;Volume( 030 ):;issue: 002 | |
| contenttype | Fulltext | |
