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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