Results 111 to 120 of about 318 (133)

Flow of Material at the Chromosphere-Corona Transition Zone of the Sun

Space Science Reviews, 1982
Early models of the Chromosphere-Corona transition zone of the Sun considered it to be a static plane-parallel region. From these it became clear that the layer was extremely thin and had an important role in the conduction of energy from the Corona. More recent observations show mass motions of order 10 km s -1, which means that heating and cooling of
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Differential rotation: the chromosphere to the quiet chromosphere

Monthly Notices of the Royal Astronomical Society, 2023
J C Xu, Jinglan Xie
exaly  

The solar chromosphere and corona: Quiet Sun

Planetary and Space Science, 1977
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The Solar Chromosphere and Corona: Quiet Sun

Physics Bulletin, 1976
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Spicules and downflows in the solar chromosphere

Astronomy and Astrophysics, 2021
Souvik Bose, Jayant Joshi, Vasco M J Henriques   +2 more
exaly  

An optically thin view of the flaring chromosphere: non-thermal widths in a chromospheric condensation during an X-class solar flare

Monthly Notices of the Royal Astronomical Society, 2023
Graham S Kerr
exaly  

New View of the Solar Chromosphere

Annual Review of Astronomy and Astrophysics, 2019
Mats Carlsson, Bart De Pontieu, Viggo Hansteen   +2 more
exaly  

The Solar Chromosphere and Corona: Quiet Sun

Physics Today, 1976
R. G. Athay, Jacques M. Beckers
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Multiwavelength Studies of MHD Waves in the Solar Chromosphere

Space Science Reviews, 2015
David B Jess, Richard J Morton, Samuel D T Grant   +2 more
exaly  

High-frequency acoustic waves are not sufficient to heat the solar chromosphere

Nature, 2005
Mats Carlsson
exaly