Please use this identifier to cite or link to this item: 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
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Appears in Collections:IIAP Publications

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