dc.contributor.author |
Hasan, S. S |
|
dc.date.accessioned |
2009-05-20T13:45:04Z |
|
dc.date.available |
2009-05-20T13:45:04Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
H. M. Antia, A. Bhatnagar, P. Ulmschneider., eds., Lecture Notes in Physics, Vol. 619, pp. 173 - 201 |
en |
dc.identifier.isbn |
978-3-540-01528-4 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4478 |
|
dc.description |
Restricted Access |
|
dc.description |
The original publication is available at springerlink.com |
|
dc.description.abstract |
Activity on the Sun is associated with magnetic fields, involving a complex interaction between the field and plasma. In this review I focus on three fundamental aspects of magnetic activity: (a) the generation, storage and emergence of magnetic fields from the solar interior; (b) the nature of the surface magnetic fields, especially in the form of small-scale flux tubes; and (c) dynamical processes in flux tubes and heating of the magnetic chromosphere. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.ispartofseries |
Lecture Notes in Physics; Vol. 619 |
|
dc.relation.uri |
http://dx.doi.org/10.1007/3-540-36963-5 |
en |
dc.rights |
© Springer |
|
dc.subject |
Magnetic Flux Tubes |
en |
dc.subject |
Sun |
en |
dc.title |
Magnetic flux tubes and activity on the sun |
en |
dc.type |
Article |
en |