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Plasma Velocities in the Solar Corona and Transition Region

Published online by Cambridge University Press:  14 March 2005

G.V. Yakunina ,
G.A. Porfir'eva  and
A.B. Delone
G.V. Yakunina
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij Prospekt 13, Moscow 119992, Russia, email: [email protected]
G.A. Porfir'eva
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij Prospekt 13, Moscow 119992, Russia, email: [email protected]
A.B. Delone
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij Prospekt 13, Moscow 119992, Russia, email: [email protected]
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Abstract

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A short compilation of results of spectral observations of nonthermal velocities $\xi$ in a wide range of temperatures in X-ray, EUV, UV and visual wave-lengths has been made. Relationship between the $\xi$ and electron temperature T for chromosphere, quiet and active corona, coronal holes (CHs) and flaring plasma is considered.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 405 - 408
Copyright
© 2004 International Astronomical Union