Magnetic mappers of the quiet solar atmosphere

Bibcode
2007msfa.conf..311T
Trujilo-Bueno, J.
Referencia bibliográfica

"Modern solar facilities - advanced solar science, Proceedings of a Workshop held at Göttingen September 27-29, 2006 ISBN 978-3-938616-84-0 382 pages, many illustrations, soft-bound, Price: 23.- Euros Published by Universitätsverlag Göttingen (http://univerlag.uni-goettingen.de The online edition (PDF, 12 MB) is available free of charge at: http://webdoc.sub.gwdg.de/univerlag/2007/solar_science_book.pdf, p.311"

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0
2007
Número de autores
1
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
0
Descripción
The magnetic sensitivity of the solar spectrum is caused by the Zeeman effect and by a variety of less familiar physical mechanisms by means of which a magnetic field can create and destroy spectral line polarization. This paper highlights how plasma diagnostic tools based on them could help us to explore the magnetism of the quiet regions of the solar photosphere and chromosphere. A few suggestions for increasing the discovery potential of some telescopes and polarimeters are also given.
Tipo
Sin árbitro

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