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Icarus 171 (2004) 153170 www.elsevier.com/locate/icarus
 

Summary: Icarus 171 (2004) 153170
www.elsevier.com/locate/icarus
Updated Galileo probe mass spectrometer measurements of carbon,
oxygen, nitrogen, and sulfur on Jupiter
Michael H. Wong a,
, Paul R. Mahaffy b
, Sushil K. Atreya c
, Hasso B. Niemann b
,
Tobias C. Owen d
a Astronomy Department, University of California at Berkeley, Berkeley, CA 94720-3411, USA
b Atmospheric Experiment Branch (Code 915), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
c Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA
d Institute for Astronomy, University of Hawaii, Honolulu, HI 96822, USA
Received 22 September 2003; revised 2 April 2004
Available online 24 June 2004
Abstract
The in situ measurements of the Galileo Probe Mass Spectrometer (GPMS) were expected to constrain the abundances of the cloud-
forming condensible volatile gases: H2O, H2S, and NH3. However, since the probe entry site (PES) was an unusually dry meteorological
system--a 5-m hotspot--the measured condensible volatile abundances did not follow the canonical condensation-limited vertical profiles

  

Source: Atreya, Sushil - Department of Atmospheric, Oceanic and Space Science, University of Michigan

 

Collections: Physics