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Pluto’s atmospheric structure from the July 2007 stellar occultation

✍ Scribed by Olkin, Catherine B.; Young, Leslie A.; French, Richard G.; Young, Eliot F.; Buie, Marc W.; Howell, Robert R.; Regester, Jeffrey; Ruhland, Catherine R.; Natusch, Tim; Ramm, David J.

Book ID
124109706
Publisher
Elsevier Science
Year
2014
Tongue
English
Weight
814 KB
Volume
239
Category
Article
ISSN
0019-1035

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We have analyzed all photometric observations of the 9 June 1988 occultation of the star P8 by Pluto in order to derive the radius of Pluto and certain parameters of its atmosphere. Our analysis is based on a "haze" model; but where relevant, we also discuss the thermal gradient model. With either m