Association between averages hssw and sssw with dst and proton flux during 2005 – 2009
International Journal of Development Research
Association between averages hssw and sssw with dst and proton flux during 2005 – 2009
Received 12th October, 2017; Received in revised form 26th November, 2017; Accepted 20th December, 2017; Published online 31st January, 2018
Copyright © 2018, Rajesh Mathpal and Lalan Prasad. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
In the present study we investigate the relationship among HSSW and SSSW with interplanetary parameters Dst and proton flow pressure for the time interval 2005 -2009. The present study investigates by means of stastical method employed for average values. The solar wind is classified into two categories- • High speed solar winds (HSSW) which have value > 450. • Slow speed solar winds (SSSW) which have value < 450. We got the emergence of charged particles from sun varies and the variation causes change in various solar activities. The proton flux associated with both HSSW and SSSW depends upon solar cycle, it enhances as solar cycle progress, goes to a maximum values (which is approx in the mid of solar cycle) and then decreases.
