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Measurements of Mass Flow in the Transition Region and Inner Corona

Published online by Cambridge University Press:  14 August 2015

Gary J. Rottman
Gary J. Rottman*
Affiliation:
The Laboratory for Atmospheric and Space Physics University of Colorado Boulder, Colorado U.S.A.

Abstract

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A recent sounding rocket experiment has provided high spectral resolution line profiles across the solar disk. The objective of this experiment is to provide information on the systematic velocity fields at the base of the corona by observing the displacement, width and shape of EUV emission lines.

Type
Part V. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 375 - 378
Copyright
Copyright © Reidel 1980 

References

Cushman, G.W., and Rense, W.A.: 1976, Astrophys. J. Letters 207, No. 1, Part II, L-61.CrossRefGoogle Scholar