Relationship Between Rising Phase of Solar Cycle 23rd and 24th with Respect to Geoeffectiveness

Author:

Bhatt Beena,Chandra Harish

Abstract

The current article demonstrates the geoeffectiveness of solar flare associated Coronal mass ejection (CME) accompanied with Deca-hectometric (DH) type II radio bursts by comparing the set of events in the rising phase of solar cycle 23rd (1996–2001) and 24th (2009–2014). Our observations are: (i) Solar cycle 23rd have high Dst index than the solar cycle 24th except for the year 1999. (ii) Dst has its peak between 3rd to 5th day after the CME onset for both the solar cycles. (iii) The correlation coefficient between Interplanetary magnetic fields (IMF) and Dst is good for both the solar cycles. (iv) Solar cycle 23rd have very strong correlation between CRI and Dst as compare to solar cycle 24th. Thus, our predictions show that solar cycle 23rd is more geoeffective than solar cycle 24th.

Publisher

American Scientific Publishers

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. 23rd solar cycle: Solar activity parameters and associated Forbush decreases;Advances in Space Research;2023-01

2. Geoeffectiveness Prediction of CMEs;Frontiers in Astronomy and Space Sciences;2021-05-20

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