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 …
The Neupert effect: What can it tell us about the impulsive and gradual phases of solar flares?
BR Dennis, DM Zarro - Solar Physics, 1993 - Springer
The Neupert effect is the name given to the correlation observed in many flares between the
time-integrated microwave and hard X-ray emissions and the soft X-ray emission light curve …
time-integrated microwave and hard X-ray emissions and the soft X-ray emission light curve …
Millisecond radio spikes: Invited review
AO Benz - Solar Physics, 1986 - Springer
Millisecond spikes of the solar radio emission are known for more than two decades. They
have recently seen a surge in interest of theoreticians who are fascinated by their high …
have recently seen a surge in interest of theoreticians who are fascinated by their high …
Energy partition in two solar flare/CME events
Using coordinated observations from instruments on the Advanced Composition Explorer
(ACE), the Solar and Heliospheric Observatory (SOHO), and the Ramaty High Energy Solar …
(ACE), the Solar and Heliospheric Observatory (SOHO), and the Ramaty High Energy Solar …
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 …
[HTML][HTML] Solar electron beams detected in hard X-rays and radio waves
Solar Electron Beams Detected in Hard X-Rays and Radio Waves ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
Radio spikes and the fragmentation of flare energy release
AO Benz - Solar physics, 1985 - Springer
Decimetric radio events with large numbers of spikes during the impulsive phase of flares
have been selected. In the observing range of 100 to 1000 MHz some flares have of the …
have been selected. In the observing range of 100 to 1000 MHz some flares have of the …
Energetic electrons in impulsive and extended solar flares as deduced from flux correlations between hard X-rays and microwaves
T Kosugi, BR Dennis, K Kai - … Journal, Part 1 (ISSN 0004-637X) …, 1988 - adsabs.harvard.edu
The peak flux relationship between hard X-rays and microwaves from solar flares is studied
using about 400 events simultaneously recorded with the hard X-ray burst spectrometer on …
using about 400 events simultaneously recorded with the hard X-ray burst spectrometer on …
Observations and nonlinear force-free field modeling of active region 10953
Y Su, A van Ballegooijen, BW Lites… - The Astrophysical …, 2009 - iopscience.iop.org
We present multiwavelength observations of a simple bipolar active region (NOAA 10953),
which produced several small flares (mostly B class and one C8. 5 class) and filament …
which produced several small flares (mostly B class and one C8. 5 class) and filament …