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Volumn 21, Issue 6, 2003, Pages 1295-1302

Latitudinal and radial variation of > 2 GeV/n protons and alpha-particles at solar maximum: ULYSSES COSPIN/KET and neutron monitor network observations

Author keywords

Interplanetary physics (cosmic rays; energetic particles); Space plasma physics (charged particle motion and acceleration)

Indexed keywords

COSMIC RAY; PLASMA; SOLAR PHENOMENA;

EID: 0042347778     PISSN: 09927689     EISSN: None     Source Type: Journal    
DOI: 10.5194/angeo-21-1295-2003     Document Type: Article
Times cited : (13)

References (18)
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    • Latitudinal and radial variation of >2 GeV/n protons derived by Ulysses-COSPIN/KET and neutron monitor network observations
    • Durban, South Africa, Space Research Unit, Potchefstroom University for CHE, Potchefstroom
    • Heber, B., Belov, A. V., Raviart, A., Paizis, C., Eroshenko, E. A., Yanke, V., Dröge, W., Green, G., and Röhrs, K.: Latitudinal and radial variation of >2 GeV/n protons derived by Ulysses-COSPIN/KET and neutron monitor network observations, in: Proc. 25th Int. Cosmic Ray Conf., Durban. South Africa, Vol. 2, 85-88, Space Research Unit, Potchefstroom University for CHE, Potchefstroom. 1997.
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    • Effects of particle drift on cosmic ray transport, I. General properties, application to solar modulation
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.