High-rigidity Forbush decreases: Due to CMEs or shocks?

Astronomy and Astrophysics

Volumn 555, Issue , 2013, Pages

  Arunbabu, K P ^a   Antia, H M ^b,c   Dugad, S R ^b,c   Gupta, S K ^b,c   Hayashi, Y ^d   Kawakami, S ^d   Mohanty, P K ^b,c   Nonaka, T ^d   Oshima, A ^e   Subramanian, P ^a  

^a INDIAN INSTITUTE OF SCIENCE EDUCATION AND RESEARCH   (India)

^b TATA INSTITUTE OF FUNDAMENTAL RESEARCH   (India)

^c GRAPES 3 Experiment Cosmic Ray Laboratory   (India)

^d Osaka Prefecture University   (Japan)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Cosmic rays; Sun: coronal mass ejections (CMEs)

Indexed keywords

CORONAL MASS EJECTION; CUT-OFF RIGIDITY; FORBUSH DECREASE; FREE PARAMETERS; MUON TELESCOPE; SHEATH REGIONS; SUN: CORONAL MASS EJECTION; TURBULENCE LEVEL;

CHARGED PARTICLES; FINITE DIFFERENCE METHOD; RIGIDITY; SOLAR WIND; TURBOMACHINERY;

COSMIC RAYS;

EID: 84880386747     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220830     Document Type: Article

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