Publication Date:
1979-06-01
Description:
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.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Terrile, R J -- Capps, R W -- Backman, D E -- Becklin, E E -- Cruikshank, D P -- Beichman, C A -- Brown, R H -- Westphal, J A -- New York, N.Y. -- Science. 1979 Jun 1;204(4396):1007-8.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17800441" target="_blank"〉PubMed〈/a〉
Print ISSN:
0036-8075
Electronic ISSN:
1095-9203
Topics:
Biology
,
Chemistry and Pharmacology
,
Computer Science
,
Medicine
,
Natural Sciences in General
,
Physics
Permalink