Published October 1977
| Version v1
Journal article
Low order effect of crand input in the Jovian atmosphere
Description
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 3He/4He ratios for the Jovian atmosphere
Additional details
Additional titles
- Augmented title (English)
- atmospheric models
Identifiers
- DOI
- 10.1007/bf00640903;
Publishing Information
- Journal Title
- The Moon
- Journal Volume
- 17
- Journal Issue
- 2
- Series
- Moon.
- Journal Page Range
- 123-131
- ISSN
- 0027-0903
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 9361738
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COMPARATIVE EVALUATIONS; COSMIC RADIATION; DECAY; EARTH PLANET; HELIUM 3; HELIUM 4; HYDROGEN; ISOTOPE RATIO; JUPITER PLANET; LEVELS; NEUTRON FLUX; NEUTRON LEAKAGE; NEUTRONS; NUCLEAR MODELS; PLANETARY ATMOSPHERES
- Descriptors DEC
- ATMOSPHERES; BARYONS; ELEMENTARY PARTICLES; ELEMENTS; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; FERMIONS; HADRONS; HELIUM ISOTOPES; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; MATHEMATICAL MODELS; NONMETALS; NUCLEI; NUCLEONS; PLANETS; RADIATION FLUX; RADIATIONS; STABLE ISOTOPES
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent