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A possible atmosphere for Pluto

✍ Scribed by Michael H. Hart


Book ID
107765159
Publisher
Elsevier Science
Year
1974
Tongue
English
Weight
352 KB
Volume
21
Category
Article
ISSN
0019-1035

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We apply scintillation theory to stellar signal fluctuations in the high-resolution, high signal/noise, dualwavelength data from the MMT observation of the 2007 March 18 occultation of P445.3 by Pluto. A welldefined high wavenumber cutoff in the fluctuations is consistent with viscous-thermal dissip