Please use this identifier to cite or link to this item:
Title: Evolution of magnetic fields in the solar atmosphere
Authors: Ravindra, B
Keywords: Sun;activity- Sun;coronal mass ejections (CMEs) ­ -Sun;oscil- lations ­ Sun;magenetic fields
Issue Date: Sep-2005
Publisher: Astronomical Society of India
Citation: BASI, Vol. 33, No. 3, pp. 333-336
Abstract: The Sun affects the terrestrial climate and weather as well as near Earth space by its high energy radiation and particle emissions. It is now becoming clear that the solar magnetic field, which controls all the physical processes in the solar atmosphere, is the driver for these two processes. In this thesis we have studied the role of the evolution of magnetic fields in the production of enhanced high energy radiation and particle emission from the Sun.
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
3305333_336.PDF108.69 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.