Low order effect of CRAND input in the Jovian atmosphere

Details Low order effect of CRAND input in the Jovian atmosphere Low order effect of CRAND input in the Jovian atmosphere

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977moon...17..123s&link_type=abstract

The Moon, vol. 17, Oct. 1977, p. 123-131.

Computer Science

Abundance, Atmospheric Models, Cosmic Ray Albedo, Jupiter Atmosphere, Neutron Decay, Atmospheric Composition, Helium Isotopes, Hydrogen, Neutron Distribution

Scientific paper

Modeling of the Jovian atmosphere shows that cosmic-ray-induced albedo neutron decay is inadequate to account for Pioneer 10 and 11 projected electron levels on Jupiter. High-energy solar protons must also be excluded as an important neutron-decay source. Analysis of neutron-flux data near the top of the Jovian atmosphere can lead to the determination of He/H2 and He-3/He-4 ratios for the Jovian atmosphere.

Affiliated with

Also associated with

No associations

Rating

Low order effect of CRAND input in the Jovian atmosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low order effect of CRAND input in the Jovian atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low order effect of CRAND input in the Jovian atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-746969