Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4478
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dc.contributor.authorHasan, S. S-
dc.date.accessioned2009-05-20T13:45:04Z-
dc.date.available2009-05-20T13:45:04Z-
dc.date.issued2003-
dc.identifier.citationH. M. Antia, A. Bhatnagar, P. Ulmschneider., eds., Lecture Notes in Physics, Vol. 619, pp. 173 - 201en
dc.identifier.isbn978-3-540-01528-4-
dc.identifier.urihttp://hdl.handle.net/2248/4478-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractActivity 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.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesLecture Notes in Physics; Vol. 619-
dc.relation.urihttp://dx.doi.org/10.1007/3-540-36963-5en
dc.rights© Springer-
dc.subjectMagnetic Flux Tubesen
dc.subjectSunen
dc.titleMagnetic flux tubes and activity on the sunen
dc.typeArticleen
Appears in Collections:IIAP Publications

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