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Study of Stealth CMEs and associated ICMEs

Published online by Cambridge University Press:  27 November 2018

Miral Bhatt ,
Nandita Srivastava  and
Ravindra Jadhav
Miral Bhatt
Affiliation:
C U Shah University, Surendranagar, India, email: bhattmiral.19@gmail.com
Nandita Srivastava
Affiliation:
Udaipur Solar Observatory, Physical Research Laboratory, Udaipur, India, email: nandita@prl.res.in
Ravindra Jadhav
Affiliation:
Gujarat Science College, Ahmedabad, India.
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Abstract

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Generally Coronal Mass Ejections (CMEs) are large eruptions of plasma and magnetic field from the Sun into interplanetary space. CMEs are most frequently associated with a variety of phenomena occurring in the lower corona before, during and after onset of eruption and generally are visible in coronagraph observation. Stealth CMEs do not obviously exhibit any of the low-coronal signatures (LCS) like solar flares, flows, jets, coronal dimmings or brightenings, filament eruptions or the formation of flare loop arcades. In this study, five stealth CMEs are selected using LASCO/SOHO CME catalogue and associated ICMEs (Interplanetaty CMEs) are identified using data from STEREO, ACE and WIND.

Keywords

Coronal Mass EjectionsStealth CMEsLCSICMEs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 89 - 90
Copyright
Copyright © International Astronomical Union 2018 

References

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