Published September 1974
| Version v1
Journal article
Cosmic ray energy changes
Creators
- 1. Monash Univ., Clayton (Australia). Dept. of Mathematics
- 2. Tasmania Univ., Sandy Bay (Australia). Dept. of Physics
Description
The purpose of this paper is to provide a new expression for < ṗ > the average time-rate-of-change of momentum of cosmic-ray particles propagating in the interplanetary region. The expression derived replaces the previously used adiabatic deceleration formula and it is arrived at by a rearrangement and reinterpretation of the well known equation of transport for cosmic-rays. Thus, although we provide a new expression for < ṗ > we maintain the equation of transport and do not render invalid results for differential intensity and differential current density of cosmic-ray particles obtained by its solution (Jokipii 1971; Gleeson 1972).
Additional details
Identifiers
Publishing Information
- Journal Title
- Publications of the Astronomical Society of Australia
- Journal Volume
- 2
- Journal Issue
- 5
- Series
- Proc. Astron. Soc. Aust.
- Journal Page Range
- 297-299
- ISSN
- 1323-3580
Conference
- Title
- 8. Annual general meeting of the Astronomical Society of Australia.
- Dates
- 22 May 1974.
- Place
- Sandy Bay, Australia.
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 6188865
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CONTINUITY EQUATIONS; COSMIC RAY PROPAGATION; DENSITY; ENERGY DEPENDENCE; INTERSTELLAR SPACE; LINEAR MOMENTUM; PRIMARY COSMIC RADIATION; TRANSPORT THEORY
- Descriptors DEC
- COSMIC RADIATION; DIFFERENTIAL EQUATIONS; EQUATIONS; IONIZING RADIATIONS; PHYSICAL PROPERTIES; RADIATIONS; SPACE
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent