The energy spectra and other properties of the great proton events during 22-nd solar cycle

Advances in Space Research

Volumn 17, Issue 4-5, 1996, Pages 167-170

  Belov, A V ^a   Eroshenko, E A ^a  

^a PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0043039466     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00562-S     Document Type: Article

References (9)

1. A comparison of the magnitude of the 29 September 1989 high energy event with solar cycle 17, 18, and 19 events
2. The evolution of the anisotropy of solar neutron decay protons during the 19 October 1989 Solar Cosmic Ray Event
3. Solar Neutron Event on 24 May 1990
4. Solar Flare Generated Neutrons Observed by NMs on 24 May 1990
5. Observation of High Energy Gamma-Rays From the Sun with the Gamma-1 Telescope (E 〉 30 MeV)
6. The proton spectra of the four remarkable GLE in 22 solar cycle
7. The Energy Spectra of the Accelerated Particles Near the Earth and in the Source in 15 June 1991 Enhancement
8. The neutron flare 24 May 1990