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Detailed Reference Information |
Akabane, T., Iwasaki, K., Saito, Y. and Narumi, Y. (1990). Blue clearing of Syrtis Major at the 1982 opposition. Journal of Geophysical Research 95: doi: 10.1029/90JB00157. issn: 0148-0227. |
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The degree of the blue clearing at Syrtis Major in the 1982 apparition shows dual components of variations. The phase-dependent part increases as Mars approaches the opposition, and the diurnal component reaches a maximum near local noon at Syrtis Major. The phase-dependent part is attributed to the opposition effect of the surrounding bright areas, and the diurnal variation is due to morning and evening clouds in the tropics. The opacity of the morning cloud is approximately unity in the early morning and decreases to null at about local noon. ¿American Geophysical Union 1990 |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Surface materials and properties |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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