Direct evidence for chromospheric evaporation in a well-observed compact flare-Reference-Cited by-同舟云学术

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Direct evidence for chromospheric evaporation in a well-observed compact flare

Published:1982-01 Issue:11 Volume:2 Page:145-149
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Canfield R.C.,Gunkler T.A.,Hudson H.S.,Acton L.W.,Leibacher J.W.,Kiplinger A.L.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference15 articles.

1. Comparison of Solar X-Ray Line Emission with Microwave Emission during Flares

2. Theoretical model of flares and prominences

3. Symp. High Energy Phenomena in the Sun;Sturrock,1973

4. A single loop of 21 January 1974 flare

5. High-resolution X-ray spectra of solar flares. IV - General spectral properties of M type flares

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1. Detection of Acceleration Processes During the Initial Phase of the 12 June 2010 Flare;Solar Physics;2012-08-21

2. Interaction and eruption of two filaments observed byHinode,SOHO, andSTEREO;Research in Astronomy and Astrophysics;2012-02-23

3. Eruptive prominence associated with limb flare of 25 January 1991;Astrophysics and Space Science;1996

4. Eruptive Prominence Associated with Limb Flare of 25 January 1991;International Astronomical Union Colloquium;1996

5. A circuit model for filament eruptions and two-ribbon flares;Solar Physics;1989

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