Published December 15, 1986
| Version v1
Journal article
A new approach for predicting proton events
Description
A statistical, comparative study to investigate the association of particle emission with 315 two-ribbon (TR) and 1964 non-two-ribbon [normal, (N)] flares, occurring during 1976-80 is carried out. The important results obtained are (i) the N-subflares do not give rise to any particle (electrons, protons and α-nuclei) emission at all. (ii) Association of TR flares with electrons (1-5 MeV) and low energy protons (0.16-0.32 MeV) is 8-10 times higher as compared with that of N-flares. (iii) The TR-flares show good correlation with high energy protons (13.7-80 MeV) and α-nuclei (11-90 MeV nucl-1) while N-flares do not show any association. This implies that TR-flares are strong flares and only they can emit energetic particles. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 223
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 877-884
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 18067148
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; CORRELATIONS; COSMIC RADIATION; MAGNETIC FIELDS; SOLAR ALPHA PARTICLES; SOLAR ELECTRONS; SOLAR FLARES; SOLAR PROTONS
- Descriptors DEC
- ALPHA PARTICLES; BARYONS; CATIONS; CHARGED PARTICLES; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HELIUM IONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONIZING RADIATIONS; IONS; LEPTONS; NUCLEONS; PROTONS; RADIATIONS; SOLAR ACTIVITY; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR FLARES; STELLAR RADIATION