Full Halo Coronal Mass Ejection and Cosmic Ray Intensity

Amita Jain, Mukesh K. Jothe, Mahendra Singh

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.

Keywords: Coronal mass Ejection, Cosmic Rays Intensity, Solar Atmosphere, Full Halo Coronal Mass ejections, Geomagnetic Field

How to Cite?: Amita Jain, Mukesh K. Jothe, Mahendra Singh, "Full Halo Coronal Mass Ejection and Cosmic Ray Intensity", Volume 4 Issue 3, March 2015, International Journal of Science and Research (IJSR), Pages: 273-274, https://www.ijsr.net/getabstract.php?paperid=SUB151803, DOI: https://dx.doi.org/10.21275/SUB151803