On Some Properties of SEP Effective CMEs
Joint Authors
Gupta, Anshu
Narain, Udit
Mittal, Nishant
Negi, P. S.
Source
ISRN Astronomy and Astrophysics
Issue
Vol. 2011, Issue 2011 (31 Dec. 2011), pp.1-6, 6 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2011-12-25
Country of Publication
Egypt
No. of Pages
6
Main Subjects
Abstract EN
Solar energetic particles (SEP) are believed to originate from two different sources, solar flares and coronal mass ejections (CMEs).
The large SEP events constitute a serious radiation hazard.
The high-energy solar proton data obtained from NOAA Space Environment Services Center are used to investigate some statistical properties such as speed, apparent width, acceleration, latitude, mass, kinetic energy, and occurrence rate of SEP effective CMEs observed during the period 1997–2006 covering the solar cycle 23.
It is found that SEP effective CMEs are nearly halo in nature, and they follow solar cycle variation.
Such CMEs have higher speeds than those of non-SEP effective CMEs.
American Psychological Association (APA)
Mittal, Nishant& Gupta, Anshu& Negi, P. S.& Narain, Udit. 2011. On Some Properties of SEP Effective CMEs. ISRN Astronomy and Astrophysics،Vol. 2011, no. 2011, pp.1-6.
https://search.emarefa.net/detail/BIM-493819
Modern Language Association (MLA)
Mittal, Nishant…[et al.]. On Some Properties of SEP Effective CMEs. ISRN Astronomy and Astrophysics No. 2011 (2011), pp.1-6.
https://search.emarefa.net/detail/BIM-493819
American Medical Association (AMA)
Mittal, Nishant& Gupta, Anshu& Negi, P. S.& Narain, Udit. On Some Properties of SEP Effective CMEs. ISRN Astronomy and Astrophysics. 2011. Vol. 2011, no. 2011, pp.1-6.
https://search.emarefa.net/detail/BIM-493819
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-493819
