Estimation of the amount of heating for the solar coronal loops and kernels

dc.contributor.author	Chandra, S
dc.date.accessioned	2005-12-06T09:14:32Z
dc.date.available	2005-12-06T09:14:32Z
dc.date.issued	1984-06
dc.identifier.citation	BASI, Vol. 12, No. 2, pp. 152-161	en
dc.identifier.uri	http://hdl.handle.net/2248/618
dc.description.abstract	We have investigated the amount of heating due to an external source for some coronal loops and kernels in the line-dipole and the point dipole geometrics under nonstatic conditions. Two forms for the external source are considered. It is found that the amount of heating for the line dipole geometry is larger than that for the point-dipole geometry. Further, the amount of heating is larger when the source is extended one (large value of gama). The heating for the second form of the source is found larger than that for the first form in the line-dipole geometry, whereas in the point-dipole geometry the reverse is true.	en
dc.format.extent	627076 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Heating - Coronal loops	en
dc.subject	Kernels	en
dc.subject	The Sun	en
dc.title	Estimation of the amount of heating for the solar coronal loops and kernels	en
dc.type	Article	en