| contributor author | Frederick, J. E. | |
| contributor author | Hays, P. B. | |
| contributor author | Guenther, B. W. | |
| contributor author | Heath, D. F. | |
| date accessioned | 2017-06-09T14:19:54Z | |
| date available | 2017-06-09T14:19:54Z | |
| date copyright | 1977/12/01 | |
| date issued | 1977 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-17403.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4153294 | |
| description abstract | Backscatter ultraviolet data obtained by the Explorer E satellite imply very large ozone column abundances above 56 km in the tropics during mid-day. The number of molecules in a vertical column decays by a factor of 2?3 after the solar zenith angle exceeds 75° in the evening. An increase of similar magnitude occurs after sunrise. Such behavior implies the presence of a greater source of odd oxygen than is included in current photochemical theories. Ozone profiles deduced between altitudes of 50 and 62 km when the solar zenith angle exceeds 80° are in reasonable agreement with past rocket results. | |
| publisher | American Meteorological Society | |
| title | Ozone Abundances in the Lower Mesosphere Deduced from Backscattered Solar Radiances | |
| type | Journal Paper | |
| journal volume | 34 | |
| journal issue | 12 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1977)034<1987:OAITLM>2.0.CO;2 | |
| journal fristpage | 1987 | |
| journal lastpage | 1994 | |
| tree | Journal of the Atmospheric Sciences:;1977:;Volume( 034 ):;issue: 012 | |
| contenttype | Fulltext | |
