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A Solar Plage Model
Published online by Cambridge University Press: 03 August 2017
Abstract
An investigation of a solar plage based on observations of UV, visible, and IR spectral lines is presented. Using model calculations, we have established distributions of the main physical parameters (temperature, density, turbulent velocity) in both plage and quiet-Sun atmospheres. Details of the models are presented and the role of magnetic pressure is discussed.
- Type
- Part 1: Infrared Diagnostics of the Solar Atmosphere and Solar Activity
- Information
- Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 29 - 33
- Copyright
- Copyright © Kluwer 1994
References
- 3
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