Features of the 11-year variation of galactic cosmic rays in different periods of solar magnetic cycles

Advances in Space Research

Volumn 35, Issue 4, 2005, Pages 677-681

  Siluszyk, M ^a   Iskra, K ^a   Modzelewska, R ^a   Alania, M V ^a,b  

^a SIEDLCE UNIVERSITY OF NATURAL SCIENCES AND HUMANITIES   (Poland)

^b Georgian Academy of Science MNodia Institute of Geophysics   (Georgia)

Author keywords

11 year variations of Galactic cosmic rays; Galactic cosmic rays intensity; Interplanetary magnetic field; Solar wind; Turbulance

Indexed keywords

DIFFUSION; ELECTRONS; FREQUENCIES; MAGNETIC FIELDS; MATHEMATICAL MODELS; MODULATION; TURBULENCE;

11-YEAR VARIATIONS OF GALACTIC COSMIC RAYS; GALACTIC COSMIC RAYS INTENSITY; INTERPLANETARY MAGNETIC FIELDS; SOLAR WINDS;

COSMIC RAYS;

EID: 20444496948     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.02.037     Document Type: Conference Paper

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