Prediction of galactic cosmic ray intensity variation for a few (up to 10-12) years on the basis of convection-diffusion and drift model

Annales Geophysicae

Volumn 23, Issue 9, 2005, Pages 3003-3007

  Dorman, L I ^a,b  

^a TEL AVIV UNIVERSITY   (Israel)

^b PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

Interplanetary physics (Galactic cosmic rays; Long term variation; Modeling and forecasting)

Indexed keywords

SOLAR PHENOMENA; SOLAR WIND;

EID: 30744436327     PISSN: 09927689     EISSN: 14320576     Source Type: Journal    
DOI: 10.5194/angeo-23-3003-2005     Document Type: Article

References (12)

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