Observation and Modeling of High-temperature Solar Active Region Emission during the High-resolution Coronal Imager Flight of 2018 May 29-Reference-Cited by-同舟云学术

Observation and Modeling of High-temperature Solar Active Region Emission during the High-resolution Coronal Imager Flight of 2018 May 29

Published:2020-06-12 Issue:1 Volume:896 Page:51
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Warren Harry P.^ORCID,Reep Jeffrey W.^ORCID,Crump Nicholas A.,Ugarte-Urra Ignacio^ORCID,Brooks David H.^ORCID,Winebarger Amy R.^ORCID,Savage Sabrina^ORCID,Pontieu Bart De^ORCID,Peter Hardi^ORCID,Cirtain Jonathan W.^ORCID,Golub Leon^ORCID,Kobayashi Ken,McKenzie David,Morton Richard^ORCID,Rachmeler Laurel^ORCID,Testa Paola^ORCID,Tiwari Sanjiv^ORCID,Walsh Robert

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab917c/pdf

Reference83 articles.

1. Constraints on Active Region Coronal Heating

2. THE VERTICAL-CURRENT APPROXIMATION NONLINEAR FORCE-FREE FIELD CODE—DESCRIPTION, PERFORMANCE TESTS, AND MEASUREMENTS OF MAGNETIC ENERGIES DISSIPATED IN SOLAR FLARES

3. Evidence for Nonuniform Heating of Coronal Loops Inferred from Multithread Modeling ofTRACEData

4. MODEL FOR ALFVÉN WAVE TURBULENCE IN SOLAR CORONAL LOOPS: HEATING RATE PROFILES AND TEMPERATURE FLUCTUATIONS

5. INFERENCE OF HEATING PROPERTIES FROM “HOT” NON-FLARING PLASMAS IN ACTIVE REGION CORES. I. SINGLE NANOFLARES

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