An observational overview of solar flares
We present an overview of solar flares and associated phenomena, drawing upon a wide
range of observational data primarily from the RHESSI era. Following an introductory …
range of observational data primarily from the RHESSI era. Following an introductory …
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 …
Quasi-periodic fast-mode wave trains within a global EUV wave and sequential transverse oscillations detected by SDO/AIA
We present the first unambiguous detection of quasi-periodic wave trains within the broad
pulse of a global EUV wave (so-called EIT wave) occurring on the limb. These wave trains …
pulse of a global EUV wave (so-called EIT wave) occurring on the limb. These wave trains …
Double coronal hard and soft X-ray source observed by RHESSI: evidence for magnetic reconnection and particle acceleration in solar flares
W Liu, V Petrosian, BR Dennis… - The Astrophysical …, 2008 - iopscience.iop.org
We present data analysis and interpretation of an M1. 4 class flare observed with the
Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) on 2002 April 30. This …
Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) on 2002 April 30. This …
Temporal evolution of chromospheric evaporation: case studies of the M1. 1 flare on 2014 September 6 and X1. 6 flare on 2014 September 10
With observations from the Interface Region Imaging Spectrograph, we track the complete
evolution of∼ 11 MK evaporation flows in an M1. 1 flare on 2014 September 6 and an X1. 6 …
evolution of∼ 11 MK evaporation flows in an M1. 1 flare on 2014 September 6 and an X1. 6 …
The existence of hot X-ray onsets in solar flares
Context. It is well known among the scientific community that solar flare activity often begins
well before the main impulsive energy release. However, a consistent explanation for this …
well before the main impulsive energy release. However, a consistent explanation for this …
An extreme solar event of 20 January 2005: properties of the flare and the origin of energetic particles
VV Grechnev, VG Kurt, IM Chertok, AM Uralov… - Solar Physics, 2008 - Springer
The famous extreme solar and particle event of 20 January 2005 is analyzed from two
perspectives. Firstly, using multi-spectral data, we study temporal, spectral, and spatial …
perspectives. Firstly, using multi-spectral data, we study temporal, spectral, and spatial …
Observational signatures of electron-driven chromospheric evaporation in a white-light flare
We investigate observational signatures of explosive chromospheric evaporation during a
white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis …
white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis …
Observations of conduction driven evaporation in the early rise phase of solar flares
M Battaglia, L Fletcher, AO Benz - Astronomy & Astrophysics, 2009 - aanda.org
Context. The classical flare picture features a beam of electrons, which were accelerated in
a site in the corona, hitting the chromosphere. The electrons are stopped in the dense …
a site in the corona, hitting the chromosphere. The electrons are stopped in the dense …