Statistical Study of Geo-Effectiveness of Planar Magnetic Structures Evolved within ICME’s

Author:

Ghag Kalpesh1ORCID,Sathe Bhagyashri1ORCID,Raghav Anil1ORCID,Shaikh Zubair2ORCID,Mishra Digvijay1,Bhaskar Ankush3ORCID,Pant Tarun Kumar3,Dhamane Omkar1ORCID,Tari Prathmesh1ORCID,Pathare Prachi1ORCID,Pawaskar Vinit1ORCID,Kumbhar Kishor1ORCID,Hilbert Greg1

Affiliation:

1. Department of Physics, University of Mumbai, Vidyanagari, Santacruz (E), Mumbai 400098, India

2. Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA

3. Space Physics Laboratory, Vikram Sarabhai Space Centre, ISRO, Thiruvananthapuram 695022, India

Abstract

Interplanetary coronal mass ejections (ICME) are large-scale eruptions from the Sun and prominent drivers of space weather disturbances, especially intense/extreme geomagnetic storms. Recent studies by our group showed that ICME sheaths and/or magnetic clouds (MC) could be transformed into a planar magnetic structure (PMS) and speculate that these structures might be more geo-effective. Thus, we statistically investigated the geo-effectiveness of planar and non-planar ICME sheaths and MC regions. We analyzed 420 ICME events observed from 1998 to 2017, and we found that the number of intense (−100 to −200 nT) and extreme (<−200 nT) geomagnetic storms are large during planar ICMEs (almost double) compared to non-planar ICMEs. In fact, almost all the extreme storm events occur during PMS molded ICME crossover. The observations suggest that planar structures are more geo-effective than non-planar structures. Thus, the current study helps us to understand the energy transfer mechanism from the ICME/solar wind into the magnetosphere, and space-weather events.

Publisher

MDPI AG

Subject

General Physics and Astronomy

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