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Coronal radiative losses
Taku Yonemoto Why Is the Sun's Corona So Hot?
EBTEL Paper 2
Magnetically Coupled Atmosphere, Fast Sausage MHD Waves, and Forced
2014) Where Is the Chromospheric Response to Conductive Energy Input from a Hot Pre- Flare Coronal Loop? Astrophysical Journal, 789 (1
Approximations for Radiative Cooling and Heating in the Solar
Arxiv:1502.07401V1 [Astro-Ph.SR] 25 Feb 2015
Solar and Stellar Magnetic Activity
A Closer Look at a Coronal Loop Rooted in a Sunspot Umbra
19800016770.Pdf
Approximations for Radiative Cooling and Heating in the Solar Chromosphere
X-Ray Evidence for Flare Density Variations and Continual Chromospheric Evaporation in Proxima Centauri
Diagnosing the Prominence-Cavity Connection in the Solar Corona
Liuw0814.Pdf (8.308Mb)
NSO Scientific Papers 1985-1999
Bibliography from ADS File: Schrijver.Bib August 16, 2021 1
1 Enthalpy-Based Thermal Evolution of Loops: II. Improvements to The
Chromospheric Emission, Rotation and X-Ray Coronae of Late-Type Stars R
20102201.Pdf
Top View
Evolution of Active Regions
Catastrophic Cooling of Loops PJ Cargill and SJ Bradshaw 1
Northumbria Research Link
Stellar Magnetic Activity
Arxiv:1210.3625V1 [Astro-Ph.SR] 12 Oct 2012 Sheffield S3 7RH, UK E-Mail: Robertus@Sheffield.Ac.Uk 2 M
The Distribution of Emission Measure, and of Heating Budget, Among the Loops in the Corona
MHD Waves in Energy Balance of the Solar Wind and the Solar Corona
1 Enthalpy-Based Thermal Evolution of Loops
Tungsten Ions in Plasmas: Statistical Theory of Radiative-Collisional Processes
Excitation of Flare-Induced Waves in Coronal Loops and the Effects Of
The Coronal Heating Problem
From Radio to X-Ray: the Quiescent Atmosphere of the Dme Flare Star
On the Nature and Genesis of EUV Waves: a Synthesis of Observations from SOHO, STEREO, SDO, and Hinode
The Role of Asymmetries in Thermal Non-Equilibrium