dc.contributor.author |
Venkatakrishnan, P |
|
dc.date.accessioned |
2009-10-16T11:19:25Z |
|
dc.date.available |
2009-10-16T11:19:25Z |
|
dc.date.issued |
1985-10-05 |
|
dc.identifier.citation |
Current Science, Vol. 54, No. 19, pp. 959 - 963 |
en |
dc.identifier.issn |
0011-3891 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4869 |
|
dc.description.abstract |
Observations of the solar chromosphere in selected spectral lines reveal a large number of inhomogeneities. These inhomogeneities owe their origin to local a large enhancement of the Photospheric magnetic fields. The detection of chromospheric inhomogeneities in other sun-like stars can be considered as the evidence for magnetic structures in such stars. This article gives a brief description of solar chromospheric structures as well as the evidence for similar inhomogeneities in stellar chromospheres. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://www.ias.ac.in/j_archive/currsci/54/vol54contents.html |
en |
dc.rights |
© Indian Academy of Sciences |
en |
dc.subject |
Chromospheric |
en |
dc.subject |
In-homogeneities |
en |
dc.subject |
Dynamics |
en |
dc.title |
Chromospheric inhomogeneities: origins and dynamics |
en |
dc.type |
Article |
en |