The beam-driven chromospheric evaporation model of solar flares - A model not supported by observations from nonimpulsive large flares-Reference-Cited by-同舟云学术

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The beam-driven chromospheric evaporation model of solar flares - A model not supported by observations from nonimpulsive large flares

Published:1990-11 Issue: Volume:364 Page:322
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Feldman U.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 30 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A Statistical Investigation of the Neupert Effect in Solar Flares Observed with ASO-S/HXI;Solar Physics;2024-05

2. The Stellar CME–Flare Relation: What Do Historic Observations Reveal?;The Astrophysical Journal;2019-05-31

3. Energetics and morphology of powerful impulsive solar flares;Astronomy Letters;2012-10

4. Non-thermal “Burst-on-Tail” of Long-Duration Solar Event on 26 October 2003;Solar Physics;2012-09-07

5. An Observational Overview of Solar Flares;Space Science Reviews;2011-08-11

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