The coronal atmosphere above solar active regions - Comparison of high spatial resolution soft X-ray and centimetric observations
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 52 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. New Evidence that Magnetoconvection Drives Solar–Stellar Coronal Heating;The Astrophysical Journal;2017-07-05
2. The Relationship Between Solar Coronal X-Ray Brightness and Active Region Magnetic Fields: A Study Using High-Resolution Hinode Observations;Solar Physics;2015-02-11
3. The altitude structure of the coronal magnetic field of AR 10933;Astronomy Reports;2012-10
4. Forward Modeling of Active Region Coronal Emissions. I. Methods and Testing;The Astrophysical Journal Supplement Series;2008-12
5. Two Unusual Episodes of ≈13-Day Variations II. Implications for the Solar Radio Flux Density, F10.7 cm;Solar Physics;2005-06
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