| contributor author | McElroy, Michael B. | |
| date accessioned | 2017-06-09T14:14:30Z | |
| date available | 2017-06-09T14:14:30Z | |
| date copyright | 1968/07/01 | |
| date issued | 1968 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-15460.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4151135 | |
| description abstract | Models for the Venus atmosphere and ionosphere are presented and compared with data obtained in the S-band occultation experiment on Mariner 5. Good agreement is found between model and experiment if the Venus atmosphere is composed of essentially pure CO2. An upper limit of about 10% is derived for the N2 mixing rate. It is argued that atomic oxygen is a minor constituent in the upper atmosphere of Venus. | |
| publisher | American Meteorological Society | |
| title | The Upper Atmosphere of Venus in Light of the Mariner 5 Measurements | |
| type | Journal Paper | |
| journal volume | 25 | |
| journal issue | 4 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1968)025<0574:TUAOVI>2.0.CO;2 | |
| journal fristpage | 574 | |
| journal lastpage | 577 | |
| tree | Journal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 004 | |
| contenttype | Fulltext | |
