| contributor author | Owen, Tobias | |
| contributor author | Mason, Harold P. | |
| date accessioned | 2017-06-09T14:15:02Z | |
| date available | 2017-06-09T14:15:02Z | |
| date copyright | 1969/09/01 | |
| date issued | 1969 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-15657.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4151353 | |
| description abstract | Assuming that the shapes of weak methane lines are determined by hydrogen and helium and helium collisional broadening, the value of H/He in the Jovian atmosphere is found to be much greater than unity. A preliminary interpretation of differences in the amount of absorption by a strong methane band over the disk of the planet leads to an estimation of height differences of 18 km over the Great Red Spot and 12 km over the equatorial zone. The yellow coloration observed on Jupiter and Saturn in compared with the properties of ammonium sulfide (NH4)2S, a compound that may occur in the atmospheres of these planets. | |
| publisher | American Meteorological Society | |
| title | New Studies of Jupiter's Atmosphere | |
| type | Journal Paper | |
| journal volume | 26 | |
| journal issue | 5 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1969)026<0870:NSOJA>2.0.CO;2 | |
| journal fristpage | 870 | |
| journal lastpage | 873 | |
| tree | Journal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 005 | |
| contenttype | Fulltext | |