The flaring and quiescent components of the solar corona
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:200809355/pdf
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1. Properties of Flare-imminent versus Flare-quiet Active Regions from the Chromosphere through the Corona. II. Nonparametric Discriminant Analysis Results from the NWRA Classification Infrastructure (NCI);The Astrophysical Journal;2023-01-01
2. X-ray activity of the young solar-like star Kepler-63 and the structure of its corona;Astronomy & Astrophysics;2022-05
3. Impulsive Coronal Heating from Large-scale Magnetic Rearrangements: From IRIS to SDO/AIA;The Astrophysical Journal;2019-08-26
4. Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties;The Astrophysical Journal;2017-08-29
5. The Slowly Varying Corona. I. Daily Differential Emission Measure Distributions Derived from EVE Spectra;The Astrophysical Journal;2017-08-03
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