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

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.

Geoeffectiveness Prediction of CMEs

“…Comparing the last two solar cycles, the 23rd one has been more geoeffective than the 24th one (Bhatt and Chandra, 2020). Solar cycle 24 was characterized by low flare activity and the main contribution to geoeffective events was made by CMEs (Bruevich and Yakunina, 2020).…”