Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8143220 | Planetary and Space Science | 2015 | 15 Pages |
Abstract
An outcome of this analysis is the finding that the slant unit optical depth varies more rapidly with solar zenith angle in the afternoon as compared to morning, with lowest values at local noon. A variation of this level is also observed with latitude. Both are indicative of the presence of overlying haze above the clouds, and the morning afternoon asymmetry suggests different photochemical processes in destruction and production of the haze.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Sanjay S. Limaye, W.J. Markiewicz, R. Krauss, N. Ignatiev, T. Roatsch, K.D. Matz,