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The occulation of Hyd -20º 51695 by Uranus on 1982 May 1

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dc.contributor.author Pandey, A. K.
dc.contributor.author Mahra, H. S.
dc.contributor.author Mohan, V.
dc.date.accessioned 2010-08-18T09:53:19Z
dc.date.available 2010-08-18T09:53:19Z
dc.date.issued 1984
dc.identifier.citation This article downloaded from ADS en_US
dc.identifier.uri http://hdl.handle.net/123456789/734
dc.description.abstract The observe emersion event of the occulation of the star Hyd -20º51695 by Uranus on 1982 May 1 has been used to evaluate the temperature of the Uranian upper atmosphere. Assuming an isothermal atmosphere the scale height comes out to be 48 ± 7 km which corresponds to an isothermal temperature of 105 ± 16K for the Uranian upeer atmosphere containing 90% hydrogen and 10% helium by number. From the inverted temperature profile, the mean temperature of the Uranian upper atmosphere comes out to be 100 ± 25 K for the altitude range 20 km above to 100 km below the half=light level. A comparison of all available independent determinations of mean atmospheric temperature since 1977 March suggests that the mean temperature of the Uranian upper atmosphere is changing with time. There is an increasing trend during the period 1977 to 1980 and a decreasing trend during the period 1980 to 1982. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries basi12-258
dc.subject Occulation, Uranus, Planetary atmoshphere en_US
dc.title The occulation of Hyd -20º 51695 by Uranus on 1982 May 1 en_US
dc.type Article en_US


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