A comparison between the CaII(k${\mathsf{_3}}$), H$_{\mathsf{\alpha}}$, SOHO/MDI and radio-enhanced temperature regions of the Sun-Reference-Cited by-同舟云学术

A comparison between the CaII(k${\mathsf{_3}}$), H$_{\mathsf{\alpha}}$, SOHO/MDI and radio-enhanced temperature regions of the Sun

Published:2003-04-23 Issue:3 Volume:402 Page:1103-1113
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Riehokainen A.,Valtaoja E.,Pohjolainen S.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20030221/pdf

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3. Gopalswamy, N., Schmal, E. J., & Kundu, M. R. 1992, Proc. First SOHO Workshop, Coronal Streamers, Coronal Loops and Coronal and Solar Wind Composition, 113

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