Some features of the sources of relativistic particles at the Sun in the solar cycles 21-23

Advances in Space Research

Volumn 38, Issue 3, 2006, Pages 411-417

  Vashenyuk, E V ^a   Balabin, Yu V ^a   Perez Peraza, J ^b   Gallegos Cruz, A ^c   Miroshnichenko, L I ^d  

^a POLAR GEOPHYSICAL INSTITUTE   (Russian Federation)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^c INSTITUTO POLITÉCNICO NACIONAL   (Mexico)

^d PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

Acceleration; Energetic spectrum; GLE; Modeling; Relativistic solar protons

Indexed keywords

ACCELERATION; ELECTRIC FIELDS; ELEMENTARY PARTICLES; HIGH ENERGY PHYSICS; SUN; TURBULENCE;

ENERGETIC SPECTRUM; GROUND LEVEL ENHANCEMENTS (GLE); MAGNETIC TRAP; RELATIVISTIC SOLAR PROTONS; SOFT ENERGY SPECTRUM;

SPACE RESEARCH;

EID: 33750205955     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.05.012     Document Type: Article

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