Polarisation and magnetic fields in cool stars and the Sun: a session in memory of Meir Semel

Martínez González, M.J., and Marsden, S.C. (2013) Polarisation and magnetic fields in cool stars and the Sun: a session in memory of Meir Semel. Astronomische Nachrichten, 334 (1-2). pp. 164-167.

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Abstract

Astrophysical plasmas and magnetic fields are inextricably coupled to each other. But magnetic fields are elusive; they cannot be fully characterized with standard (spectroscopic) observational techniques. Fortunately, polarisation, the third fundamental property of light, encodes all the quantitative information on the magnetism of the objects we observe. This splinter session brought together the solar and stellar spectropolarimetric communities to discuss some of the fundamental unsolved questions of solar and stellar magnetism and the future of spectropolarimetric observations.

Item ID: 32896
Item Type: Article (Research - C1)
ISSN: 1521-3994
Keywords: stars: activity, stars: atmospheres, stars: chromospheres, stars: magnetic fields, sun: atmosphere, sun: chromosphere, sun: magnetic fields
Date Deposited: 30 Apr 2014 09:59
FoR Codes: 02 PHYSICAL SCIENCES > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems @ 100%
SEO Codes: 97 EXPANDING KNOWLEDGE > 970102 Expanding Knowledge in the Physical Sciences @ 100%
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