The Energetics of White-light Flares Observed bySDO/HMI andRHESSI
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/16/i=11/a=177/pdf
Reference37 articles.
1. Non-thermal collisional excitation and ionization by electron beams: Effect on the atmospheric energy balance and white-light emission in solar flares
2. Radiative Hydrodynamic Models of the Optical and Ultraviolet Emission from Solar Flares
3. Height structure of X-ray, EUV, and white-light emission in a solar flare
4. The deduction of energy spectra of non-thermal electrons in flares from the observed dynamic spectra of hard X-ray bursts
5. RADIATIVE HYDRODYNAMIC SIMULATION OF THE CONTINUUM EMISSION IN SOLAR WHITE-LIGHT FLARES
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1. Modern analytical models of electrons acceleration and propagation in solar flares;Physics-Uspekhi;2021-08
2. The Statistical Relationship between White-light Emission and Photospheric Magnetic Field Changes in Flares;The Astrophysical Journal;2020-11-24
3. Response of SDO/HMI Observables to Heating of the Solar Atmosphere by Precipitating High-energy Electrons;The Astrophysical Journal;2020-04-09
4. Investigation of White-light Emission in Circular-ribbon Flares;The Astrophysical Journal;2018-11-12
5. Observations of white-light flares in NOAA active region 11515: high occurrence rate and relationship with magnetic transients;Astronomy & Astrophysics;2018-05
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