Title of article
Quiet sun XUV and EUV spectroscopy Original Research Article
Author/Authors
P. Lemaire، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2007
Pages
6
From page
1876
To page
1881
Abstract
The two XUV–EUV spectrometers on SOHO have collected a large amount of data in the 6000–106 K solar plasma temperature range. These data have allowed us to greatly enhance our knowledge of the processes acting in the solar atmosphere, from the chromosphere to the corona. Some results on the quiet Sun structure (network, quiet Sun versus coronal hole), on the dynamics (velocities, waves, transient events), and the main characteristics of the quiet Sun atmosphere are presented and discussed.
Keywords
Sun , Chromosphere–corona transition region , Chromosphere
Journal title
Advances in Space Research
Serial Year
2007
Journal title
Advances in Space Research
Record number
1131658
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