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http://hdl.handle.net/2248/3801
Title: | Spatial profiles of lines in active region loops |
Authors: | Krishan, V |
Keywords: | Coronal Loops Line Shape Solar Activity Effects Solar Corona Solar Spectra Ultraviolet Spectra Astronomical Models Magnetic Field Configurations Magnetohydrodynamic Turbulence Plasma Turbulence Solar Physics Temperature Distribution |
Issue Date: | Oct-1983 |
Publisher: | Springer |
Citation: | Solar Physics, Vol. 88, No. 1 - 2, pp. 155 - 161 |
Abstract: | From the statistical treatment of magnetohydrodynamically turbulent plasma, a steady-state density, temperature and magnetic field structure is derived for a coronal loop emitting in UV and EUV range. Spatial variation of line flux is presented for the lines C II, C III, O IV, O VI, Ne VII, and Mg X. It is found that the hotter lines which are emitted near the surface of the loop have larger spatial extents compared to the lines originating in the cool core of the loop, in agreement with the observations. |
URI: | http://hdl.handle.net/2248/3801 |
ISSN: | 0038-0938 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Spatial profiles of lines in active region loops | 495.79 kB | Adobe PDF | View/Open |
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