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Measurements of Mass Flow in the Transition Region and Inner Corona
Published online by Cambridge University Press: 14 August 2015
Abstract
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