2020
DOI: 10.1051/0004-6361/202037528
|View full text |Cite
|
Sign up to set email alerts
|

Non-interacting coronal mass ejections and solar energetic particles near the quadrature configuration of Solar TErrestrial RElations Observatory

Abstract: We present our results on the correlation of non-interacting coronal mass ejections (CMEs) and solar energetic particles (SEPs). A statistical analysis was conducted on 25 SEP events and the associated CME and flare during the ascending phase of solar cycle 24, i.e., 2009–2013, which marks the quadrature configuration of Solar TErrestrial RElations Observatory (STEREO). The complete kinematics of CMEs is well studied near this configuration of STEREO. In addition, we have made comparison studies of STEREO and … Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2021
2021
2023
2023

Publication Types

Select...
5

Relationship

1
4

Authors

Journals

citations
Cited by 5 publications
(1 citation statement)
references
References 55 publications
0
1
0
Order By: Relevance
“…To obtain the shock magnetosonic Mach number, M ms , the shock speed, V s , should be divided by the upstream magnetosonic wave speed, V ms1 : One should note that the combination of Eqs. ( 3) and ( 4) has no resemblance to the expression used by Ravishankar & Michalek (2020).…”
Section: Introductionmentioning
confidence: 99%
“…To obtain the shock magnetosonic Mach number, M ms , the shock speed, V s , should be divided by the upstream magnetosonic wave speed, V ms1 : One should note that the combination of Eqs. ( 3) and ( 4) has no resemblance to the expression used by Ravishankar & Michalek (2020).…”
Section: Introductionmentioning
confidence: 99%