| contributor author | Gautier, Daniel | |
| contributor author | Grossman, Kenneth | |
| date accessioned | 2017-06-09T14:16:26Z | |
| date available | 2017-06-09T14:16:26Z | |
| date copyright | 1972/05/01 | |
| date issued | 1972 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-16185.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4151940 | |
| description abstract | By using a numerical iterative method, it is demonstrated that the mixing ratio H2/He on the giant planets can be inferred from spectral measurements of the intensity emitted by these planets in the far infrared range. The method is successfully applied to synthetic spectra of Saturn computed from atmospheric thermal models. The effect of random and systematic measurement errors on the determination of the mixing ratio is also studied. | |
| publisher | American Meteorological Society | |
| title | A New Method for the Determination of the Mixing Ratio Hydrogen to Helium in the Giant Planets | |
| type | Journal Paper | |
| journal volume | 29 | |
| journal issue | 4 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1972)029<0788:R>2.0.CO;2 | |
| journal fristpage | 788 | |
| journal lastpage | 792 | |
| tree | Journal of the Atmospheric Sciences:;1972:;Volume( 029 ):;issue: 004 | |
| contenttype | Fulltext | |
