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Distorted Wave Calculations: Application to Astrophysics and Tokamak Plasma

Published online by Cambridge University Press:  12 April 2016

A.K. Bhatia
A.K. Bhatia*
Affiliation:
Laboratory for Astronomy and Solar Physics NASA/Goddard Space Flight Center Greenbelt, Maryland 20771, USA

Extract

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During the last few years, observations of solar phenomena have been carried out by rocket flights, manned satellites like Skylab, unmanned satellites like Orbiting Solar Observatories and more recently Solar Maximum Mission. The wavelengths, line intensities and line profiles in UV and X-ray regions of the solar spectra have been measured. The spectroscopic data obtained are of high spatial and spectral resolution. The goal is to understand the physical properties of the emitting plasma and determine the electron temperatures, densities and volume of the emitting plasma from UV and X-ray spectra.

Type
Session 4. Theoretical Spectroscopy
Information
International Astronomical Union Colloquium , Volume 86: Eighth International Colloquium on Ultraviolet and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas , 1984 , pp. 92 - 99
Copyright
Copyright © Naval Research Laboratory 1984. Publication courtesy of the Naval Research Laboratory, Washington, DC.

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