Global energetics of solar flares. V. Energy closure in flares and coronal mass ejections
In this study we synthesize the results of four previous studies on the global energetics of
solar flares and associated coronal mass ejections (CMEs), which include magnetic …
solar flares and associated coronal mass ejections (CMEs), which include magnetic …
High-resolution imaging of solar flare ribbons and its implication on the thick-target beam model
S Krucker, HS Hudson, NLS Jeffrey… - The Astrophysical …, 2011 - iopscience.iop.org
We report on high-resolution optical and hard X-ray observations of solar flare ribbons seen
during the GOES X6. 5 class white-light flare of 2006 December 6. The data consist of …
during the GOES X6. 5 class white-light flare of 2006 December 6. The data consist of …
[图书][B] Hard X-ray Imaging of Solar Flares
The idea for this book emerged over a number of years as the authors participated in various
research projects related to analysis and interpretation of data from NASA's RHESSI Small …
research projects related to analysis and interpretation of data from NASA's RHESSI Small …
Radiative hydrodynamic modelling and observations of the X-class solar flare on 2011 March 9
MB Kennedy, RO Milligan, JC Allred… - Astronomy & …, 2015 - aanda.org
Aims. We investigated the response of the solar atmosphere to non-thermal electron beam
heating using the radiative transfer and hydrodynamics modelling code RADYN. The …
heating using the radiative transfer and hydrodynamics modelling code RADYN. The …
Acceleration, magnetic fluctuations, and cross-field transport of energetic electrons in a solar flare loop
Plasma turbulence is thought to be associated with various physical processes involved in
solar flares, including magnetic reconnection, particle acceleration, and transport. Using …
solar flares, including magnetic reconnection, particle acceleration, and transport. Using …
Wave-particle interactions in non-uniform plasma and the interpretation of hard X-ray spectra in solar flares
Context. High-energy electrons accelerated during solar flares are abundant in the solar
corona and in interplanetary space. Commonly, the number and energy of non-thermal …
corona and in interplanetary space. Commonly, the number and energy of non-thermal …
Thermal and nonthermal hard X-ray source sizes in solar flares obtained from RHESSI observations-I. Observations and evaluation of methods
A Warmuth, G Mann - Astronomy & Astrophysics, 2013 - aanda.org
Context. In solar flares, a large amount of thermal and nonthermal energy is released
impulsively in the form of heated plasma and accelerated particles. These processes can be …
impulsively in the form of heated plasma and accelerated particles. These processes can be …
Triangulation of Hard X-Ray Sources in an X-Class Solar Flare with ASO-S/HXI and Solar Orbiter/STIX
DF Ryan, P Massa, AF Battaglia, E Dickson, Y Su… - Solar Physics, 2024 - Springer
Abstract HXI on ASO-S and STIX onboard Solar Orbiter are the first simultaneously
operating solar hard X-ray imaging spectrometers. ASO-S's low Earth orbit and Solar …
operating solar hard X-ray imaging spectrometers. ASO-S's low Earth orbit and Solar …
Hard X-ray footpoint sizes and positions as diagnostics of flare accelerated energetic electrons in the low solar atmosphere
M Battaglia, EP Kontar - The Astrophysical Journal, 2011 - iopscience.iop.org
The hard X-ray (HXR) emission in solar flares comes almost exclusively from a very small
part of the flaring region, the footpoints of magnetic loops. Using RHESSI observations of …
part of the flaring region, the footpoints of magnetic loops. Using RHESSI observations of …
Global energetics of solar flares and coronal mass ejections
We investigate the global energetics and energy closure of various physical processes that
are energetically important in solar flares and coronal mass ejections (CMEs), which …
are energetically important in solar flares and coronal mass ejections (CMEs), which …