Spicules and their on-disk counterparts, the main driver for solar chromospheric heating?

The question how the outer solar atmosphere is heated from solar photospheric temperatures of about 5800K up to solar chromospheric and coronal temperatures of about 20.000K and millions of degrees respectively, remained without any satisfying answer for centuries. On 4 May 2005, I recorded several...

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Veröffentlicht in:	arXiv.org 2020-05
1. Verfasser:	Puschmann, Klaus Gerhard
Format:	Artikel
Sprache:	eng
Schlagworte:	Fabry-Perot interferometers Heating Paths Photosphere Solar atmosphere Solar corona Solar limb Solar wind Spicules Sun Time series
Online-Zugang:	Volltext
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