| contributor author | Hays, P. B. | |
| contributor author | Roble, R. G. | |
| date accessioned | 2017-06-09T14:14:42Z | |
| date available | 2017-06-09T14:14:42Z | |
| date copyright | 1968/11/01 | |
| date issued | 1968 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-15537.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4151220 | |
| description abstract | The distortions to the image and spectrum of a star being observed during occultation from a satellite are discussed. The primary distortions are shown to be due to refractive dispersion, small and large particle scattering, and absorption by various atmospheric gases. Representative stellar spectra in both the visible and ultraviolet are presented, and various features relating to specific atmospheric constituents are discussed. The possibility of recovering information concerning atmospheric composition from stellar spectra is considered and several distinct processes are used for illustration. | |
| publisher | American Meteorological Society | |
| title | Stellar Spectra and Atmospheric Composition | |
| type | Journal Paper | |
| journal volume | 25 | |
| journal issue | 6 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1968)025<1141:SSAAC>2.0.CO;2 | |
| journal fristpage | 1141 | |
| journal lastpage | 1153 | |
| tree | Journal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 006 | |
| contenttype | Fulltext | |
