Published April 1988
| Version v1
Report
Predicting the arrival times of solar particles
Creators
Description
A procedure has been developed to generate a computerized time-intensity profile of the solar proton intensity expected at the earth after the occurrence of a significant solar flare on the sun. This procedure is a combination of many pieces of independent research and theoretical results. Many of the concepts used were first reported by Smart and Shea (1979) and are summarized by Smart and Shea (1985). Extracts from the general procedure that relate to predicting the expected onset time and time of maximum at the earth after the occurrence of a solar flare are presented
Additional details
Publishing Information
- Imprint Title
- Interplanetary particle environment. Proceedings of a conference
- Imprint Pagination
- 165 p.
- Journal Page Range
- p. 101-110.
- Report number
- N--89-28454
Conference
- Title
- Conference on interplanetary particle environment.
- Dates
- 16-17 Mar 1987.
- Place
- Pasadena, CA (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22017797
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- COMPUTER CALCULATIONS; COSMIC RAY FLUX; FORECASTING; HEAVY IONS; INTERPLANETARY MAGNETIC FIELDS; MATHEMATICAL MODELS; SOLAR ACTIVITY; SOLAR CORONA; SOLAR FLARES; SOLAR PARTICLES; SOLAR PROTONS; THEORETICAL DATA
- Descriptors DEC
- ATMOSPHERES; BARYONS; CATIONS; CHARGED PARTICLES; DATA; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; INFORMATION; IONS; MAGNETIC FIELDS; NUCLEONS; NUMERICAL DATA; PROTONS; RADIATION FLUX; RADIATIONS; SOLAR ATMOSPHERE; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES; STELLAR RADIATION
Optional Information
- Secondary number(s)
- NASA-CR--185461; JPL-PUBL--88-28; NAS--1.26:185461; CONF-8703326--.