An Operator Perturbation Method of Polarized Line Transfer V. Diagnosis of Solar Weak Magnetic Fields

dc.contributor.author	Nagendra, K. N
dc.contributor.author	Frisch, H
dc.contributor.author	Faurobeet-Scholl, M
dc.contributor.author	Paletou, F
dc.date.accessioned	2008-08-12T08:56:43Z
dc.date.available	2008-08-12T08:56:43Z
dc.date.issued	2000-12
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 255 - 258	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/3072
dc.description.abstract	We present an application of the PALI (Polarized Approximate Lambda Iteration) method to the resonance scattering in spectral lines formed in the presence of weak magnetic fields. The method is based on an operator perturbation approach, and can efficiently give solutions for oriented vector magnetic fields in the solar atmosphere.	en
dc.format.extent	108579 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000JApA...21..255N	en
dc.subject	Polarization	en
dc.subject	Magnetic Fields	en
dc.subject	Radiative Transfer	en
dc.subject	Stars:Atmospheres	en
dc.subject	Methods: Numerical	en
dc.title	An Operator Perturbation Method of Polarized Line Transfer V. Diagnosis of Solar Weak Magnetic Fields	en
dc.type	Article	en