Physical conditions in the cool parts of prominences and spicules - The effects of model atom level truncation on the derived plasma parameters-Reference-Cited by-同舟云学术

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Physical conditions in the cool parts of prominences and spicules - The effects of model atom level truncation on the derived plasma parameters

Published:1986-06 Issue: Volume:305 Page:546
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Landman D. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 12 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. Evidence for the Two-fluid Scenario in Solar Prominences;The Astrophysical Journal;2019-03-13

2. The Na i and Sr ii Resonance Lines in Solar Prominences;Solar Physics;2017-06-16

3. Multi-Wavelength Eclipse Observations of a Quiescent Prominence;Solar Physics;2014-01-23

4. Physics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling;Space Science Reviews;2010-02-20

5. Steady 2D prominence-like solutions of the MHD equations with field-aligned compressible flow;Astronomy & Astrophysics;2005-01

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