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The magnetic field in the solar atmosphere
DOI: 10.1007/s00159-014-0078-7 Bibcode: 2014A&ARv..22...78W

Solanki, Sami K.; Wiegelmann, Thomas; Thalmann, Julia K.

This publication provides an overview of magnetic fields in the solar atmosphere with the focus lying on the corona. The solar magnetic field couples the solar interior with the visible surface of the Sun and with its atmosphere. It is also responsible for all solar activity in its numerous manifestations. Thus, dynamic phenomena such as coronal m…

2014 Astronomy and Astrophysics Review
Hinode SOHO 151
Solar magnetic fields as revealed by Stokes polarimetry
DOI: 10.1007/s00159-013-0066-3 Bibcode: 2013A&ARv..21...66S

Stenflo, J. O.

Observational astrophysics started when spectroscopy could be applied to astronomy. Similarly, observational work on stellar magnetic fields became possible with the application of spectro-polarimetry. In recent decades there have been dramatic advances in the observational tools for spectro-polarimetry. The four Stokes parameters that provide a c…

2013 Astronomy and Astrophysics Review
Hinode SOHO 85
Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
DOI: 10.1007/s00159-011-0035-7 Bibcode: 2011A&ARv..19...35W

Llebaria, A.; Auchère, F.; Feng, L. +12 more

Coronal plumes, which extend from solar coronal holes (CH) into the high corona and—possibly—into the solar wind (SW), can now continuously be studied with modern telescopes and spectrometers on spacecraft, in addition to investigations from the ground, in particular, during total eclipses. Despite the large amount of data available on these promi…

2011 Astronomy and Astrophysics Review
Hinode SOHO 63