Abstract
A coordinated program to observe Jupiter at high spatial resolution in the 5-micrometer wavelength region was undertaken to support Voyager 1 imaging and infrared radiation experiment targeting. Jupiter was observed over a 5-month period from Palomar and Mauna Kea observatories. The frequency of observations allowed the selection of interesting areas for closer Voyager examination and also provided good short-term monitoring of variations in cloud morphology. Significant global changes in the 5-micrometer distribution are seen over this time period.
Original language | English (US) |
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Pages (from-to) | 1007-1008 |
Number of pages | 2 |
Journal | Science |
Volume | 204 |
Issue number | 4396 |
DOIs | |
State | Published - 1979 |
ASJC Scopus subject areas
- General