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Space Weather – Sun Earth Relations

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dc.contributor.author Sundararaman, K
dc.date.accessioned 2011-05-20T12:14:25Z
dc.date.available 2011-05-20T12:14:25Z
dc.date.issued 2011-03
dc.identifier.citation International Journal of Astronomy and Astrophysics, Vol. 1, No. 1, pp. 10-14 en
dc.identifier.uri http://hdl.handle.net/2248/5482
dc.description.abstract Sun, a star of spectral type G2 is the main source of energy to the Earth. Being close to the Earth, Sun pro-duces a resolvable disk of great detail, which is not possible for other stars. Solar flares and coronal mass ejections are the enigmatic phenomena that occur in the solar atmosphere and regularly bombard the Earth’s environment in addition to the solar wind. Thus it becomes important for us not only to understand these physical processes of the Sun, but in addition how these activities affect the Earth and it’s surrounding. Thus a branch of study called ‘Space Weather’ had emerged in the recent past, which connects the Sun Earth rela-tions. This paper details about the solar activity and associated energetic phenomena that occur in the at-mosphere of the Sun and their influence on the Earth. en
dc.language.iso en en
dc.publisher Scientific Research Publishing en
dc.relation.uri http://dx.doi.org/10.4236/ijaa.2011.11003 en
dc.relation.uri http://www.scirp.org/journal/PaperInformation.aspx?paperID=4374
dc.rights © Scientific Research Publishing en
dc.subject Sun en
dc.subject Sunspot en
dc.subject Prominence en
dc.subject Solar Flare en
dc.subject Coronal Mass Ejection en
dc.title Space Weather – Sun Earth Relations en
dc.type Article en


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