Published September 1983
| Version v1
Journal article
High-energy solar protons
Creators
Description
Problems of solar particle acceleration in large-scale solar flares are discussed. Direct measurements of the first income of high-energy protons from large-scale solar flares made with the use of the ''Prognoz'' satellites detected a delay of energy protons outcome from solar corona as compared with the flare explosive phase. The effect of delay of energy solar particle injection into interplanetary space can be explained by the fact that proton acceleration up to the energies E > 100 MeV takes place not during explosion phase, but later, and it can serve as a testimony in favour of solar cosmic ray acceleration in large-scale flares in two stages
Additional details
Additional titles
- Original title (Russian)
- Солнечные протоны высоко энергии
Publishing Information
- Journal Title
- Kosm. Issled.
- Journal Volume
- 21
- Journal Issue
- 5
- Series
- Kosm. Issled.
- Journal Page Range
- 731-736
- ISSN
- 0023-4206
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 15032010
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCELERATION; ENERGETIC SOLAR PARTICLES; MEV RANGE; PROGNOZ SATELLITES; PROTONS; SOLAR FLARES
- Descriptors DEC
- BARYONS; CATIONS; CHARGED PARTICLES; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONS; NUCLEONS; RADIATIONS; SATELLITES; SOLAR ACTIVITY; SOLAR RADIATION; STELLAR FLARES; STELLAR RADIATION
Optional Information
- Notes
- For English translation see the journal Cosmic Research (USA).