Modeling and experimental study of the 27-day variation of galactic cosmic-ray intensity for a solar wind velocity depending on heliolongitude

Advances in Space Research

Volumn 45, Issue 3, 2010, Pages 421-428

  Alania, M V ^a,b   Modzelewska, R ^a   Wawrzynczak, A ^a  

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

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

Author keywords

27 day variation; Cosmic rays; Magnetic field; Solar wind

Indexed keywords

COSMOLOGY; MAGNETIC FIELDS; MAXWELL EQUATIONS; SOLAR WIND; WIND;

27-DAY VARIATION; CORRELATION COEFFICIENT; GALACTIC COSMIC RAYS; INTERPLANETARY MAGNETIC FIELDS; MODEL CALCULATIONS; SOLAR WIND VELOCITY; SPATIAL VARIATIONS; THREE DIMENSIONAL (3-D) MODELING;

COSMIC RAYS;

EID: 73649147021     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2009.08.009     Document Type: Article

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