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) |
|---|---|
| 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