[HTML][HTML] Flare observations
AO Benz - Living reviews in solar physics, 2017 - Springer
Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays
beyond 1 GeV. This review focuses on recent observations in EUV, soft and hard X-rays …
beyond 1 GeV. This review focuses on recent observations in EUV, soft and hard X-rays …
Implications of X-ray observations for electron acceleration and propagation in solar flares
GD Holman, MJ Aschwanden, H Aurass… - Space science …, 2011 - Springer
High-energy X-rays and γ-rays from solar flares were discovered just over fifty years ago.
Since that time, the standard for the interpretation of spatially integrated flare X-ray spectra at …
Since that time, the standard for the interpretation of spatially integrated flare X-ray spectra at …
Recent advances in understanding particle acceleration processes in solar flares
We review basic theoretical concepts in particle acceleration, with particular emphasis on
processes likely to occur in regions of magnetic reconnection. Several new developments …
processes likely to occur in regions of magnetic reconnection. Several new developments …
Measurements of the coronal acceleration region of a solar flare
S Krucker, HS Hudson, L Glesener… - The Astrophysical …, 2010 - iopscience.iop.org
ABSTRACT The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and
the Nobeyama Radioheliograph (NoRH) are used to investigate coronal hard X-ray and …
the Nobeyama Radioheliograph (NoRH) are used to investigate coronal hard X-ray and …
Hard X-ray emission from the solar corona
S Krucker, M Battaglia, PJ Cargill, L Fletcher… - The Astronomy and …, 2008 - Springer
This review surveys hard X-ray emissions of non-thermal electrons in the solar corona.
These electrons originate in flares and flare-related processes. Hard X-ray emission is the …
These electrons originate in flares and flare-related processes. Hard X-ray emission is the …
Electron power-law spectra in solar and space plasmas
Particles are accelerated to very high, non-thermal energies in solar and space plasma
environments. While energy spectra of accelerated electrons often exhibit a power law, it …
environments. While energy spectra of accelerated electrons often exhibit a power law, it …
Hard X-ray emissions from partially occulted solar flares
S Krucker, RP Lin - The Astrophysical Journal, 2008 - iopscience.iop.org
Observations of solar flares partially occulted by the solar limb provide diagnostics of
coronal hard X-ray (HXR) emissions in the absence of generally much brighter emissions …
coronal hard X-ray (HXR) emissions in the absence of generally much brighter emissions …
[图书][B] New millennium solar physics
MJ Aschwanden - 2019 - Springer
An introduction into the subject of solar physics has been previously presented in the
textbook Physics of the Solar Corona by the same author, which covered most of the science …
textbook Physics of the Solar Corona by the same author, which covered most of the science …
Electron acceleration by cascading reconnection in the solar corona. II. Resistive electric field effects
We investigate electron acceleration by electric fields induced by cascading reconnections
in current sheets trailing coronal mass ejections via a test particle approach in the framework …
in current sheets trailing coronal mass ejections via a test particle approach in the framework …
The sub-arcsecond hard X-ray structure of loop footpoints in a solar flare
The newly developed X-ray visibility forward fitting technique is applied to the RHESSI data
of a limb flare to investigate the energy and height dependence on sizes, shapes, and …
of a limb flare to investigate the energy and height dependence on sizes, shapes, and …