Relative Timing of Soft X-Ray Nonthermal Line Broadening and Hard X-Ray Emission in Solar Flares-Reference-Cited by-同舟云学术

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Relative Timing of Soft X-Ray Nonthermal Line Broadening and Hard X-Ray Emission in Solar Flares

Published:1998-02-20 Issue:2 Volume:494 Page:L235-L238
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Alexander David,Harra-Murnion Louise K.,Khan Josef I.,Matthews Sarah A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference24 articles.

1. Alfv�n turbulence and the time dependence of non-thermal line broadening in flares

2. Particle acceleration and the decay of soft X-ray non-thermal line broadening in solar flares

3. Solar flare spectral diagnosis: Present and future

4. Antonucci, E. 1998, Flare Dynamics, ed. K. T. Strong, J. L. R. Saba, J. T. Schmelz, & B. Haisch (New York: Springer), chap. 4

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2. The existence of hot X-ray onsets in solar flares;Astronomy & Astrophysics;2023-11

3. Flare-productive active regions;Living Reviews in Solar Physics;2019-05-21

4. Electron Heating by Kinetic Alfvén Waves in Coronal Loop Turbulence;The Astrophysical Journal;2019-01-22

5. The Duration of Energy Deposition on Unresolved Flaring Loops in the Solar Corona;The Astrophysical Journal;2018-04-03

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