Quiet Sun Chromospheric Network Magnetic Field

dc.contributor.author	Ravindra, B
dc.date.accessioned	2008-06-03T12:12:09Z
dc.date.available	2008-06-03T12:12:09Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 297 - 298	en
dc.identifier.uri	http://hdl.handle.net/2248/2397
dc.description.abstract	The 3-D structure of quiet Sun chromospheric network magnetic field is studied by comparing the observed and computed chromospheric magnetograms. The comparison shows that the best correlation occurs at 1800 km above the photosphere at which the Fe I 8688 line forms.	en
dc.format.extent	70875 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..297R	en
dc.subject	Sun	en
dc.subject	Network	en
dc.subject	Magnetic field	en
dc.title	Quiet Sun Chromospheric Network Magnetic Field	en
dc.type	Article	en