Solar polarization: proceedings of an international workshop held in St. Petersburg, Russia, 8–12 May, 1995

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7570

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DC Field	Value	Language
dc.contributor.author	Stenflo, J. O (editor)	-
dc.contributor.author	Nagendra, K. N (editor)	-
dc.date.accessioned	2021-02-07T04:23:30Z	-
dc.date.available	2021-02-07T04:23:30Z	-
dc.date.issued	1996	-
dc.identifier.citation	xi, 432p.	en_US
dc.identifier.isbn	978-0-7923-3985-4	-
dc.identifier.uri	http://hdl.handle.net/2248/7570	-
dc.description	© Kluwer Academic Publishers The original publication is available at Springer http://dx.doi.org/10.1007/978-94-009-0231-2	en_US
dc.description.abstract	Much progress has been made in recent years in understanding the complex physics of polarized radiation in the sun and stars. This physics includes vector radiative transfer and spectral line formation in the presence of magnetic fields, scattering theory and coherence effects, partial redistribution and turbulent magnetic fields, numerical techniques and Stokes inversion, as well as concepts for polarimetric imaging with a precision limited only by photon statistics. The present volume gives a comprehensive and up-to-date account of this rapidly evolving field of science.	en_US
dc.language.iso	en	en_US
dc.publisher	Kluwer Academic Publishers	en_US
dc.subject	Corona	en_US
dc.subject	Solar flare	en_US
dc.subject	Solar prominence	en_US
dc.subject	solar spectra	en_US
dc.title	Solar polarization: proceedings of an international workshop held in St. Petersburg, Russia, 8–12 May, 1995	en_US
dc.type	Book	en_US
Appears in Collections:	Books Publication by IIAP

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