SOLAR AND THERMAL-RADIATION IN JUPITER ATMOSPHERE - INITIAL RESULTS OF THE GALILEO PROBE NET FLUX RADIOMETER

Citation
La. Sromovsky et al., SOLAR AND THERMAL-RADIATION IN JUPITER ATMOSPHERE - INITIAL RESULTS OF THE GALILEO PROBE NET FLUX RADIOMETER, Science, 272(5263), 1996, pp. 851-854
Citations number
14
Categorie Soggetti
Multidisciplinary Sciences
Journal title
ISSN journal
00368075
Volume
272
Issue
5263
Year of publication
1996
Pages
851 - 854
Database
ISI
SICI code
0036-8075(1996)272:5263<851:SATIJA>2.0.ZU;2-#
Abstract
The Galileo probe net flux radiometer measured radiation within Jupite r's atmosphere over the 125-kilometer altitude range between pressures of 0.44 bar and 14 bars. Evidence for the expected ammonia cloud was seen in solar and thermal channels down to 0.5 to 0.6 bar. Between 0.6 and 10 bars large thermal fluxes imply very low gaseous opacities and provide no evidence for a deep water cloud. Near 8 bars the water vap or abundance appears to be about 10 percent of what would be expected for a solar abundance of oxygen. Below 8 bars, measurements suggest an increasing water abundance with depth or a deep cloud layer. Ammonia appears to follow a significantly subsaturated profile above 3 bars. U nexpectedly high absorption of sunlight was found at wavelengths great er than 600 nanometers.