Full Halo Coronal Mass Ejection and Cosmic Ray Intensity

Journal Title: UNKNOWN - Year 2015, Vol 4, Issue 3

Abstract

In this work we have studied the effect of different types of full halo Coronal Mass Ejection on the cosmic ray intensity for the period of 1996-2004. It is found that the cosmic ray intensity depressed to minimum after three days of the onset of the symmetric and outlines asymmetric full halo CMEs and four days after the onset of brightness asymmetric full halo event of Coronal mass Ejection.

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  • EP ID EP356905
  • DOI -
  • Views 105
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How To Cite

(2015). Full Halo Coronal Mass Ejection and Cosmic Ray Intensity. UNKNOWN, 4(3), -. https://europub.co.uk./articles/-A-356905