Extreme solar events
EW Cliver, CJ Schrijver, K Shibata… - Living Reviews in Solar …, 2022 - Springer
We trace the evolution of research on extreme solar and solar-terrestrial events from the
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
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 …
The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches
A new data product from the Helioseismic and Magnetic Imager (HMI) onboard the Solar
Dynamics Observatory (SDO) called Space-weather HMI Active Region Patches (SHARP s) …
Dynamics Observatory (SDO) called Space-weather HMI Active Region Patches (SHARP s) …
Evolution of magnetic field and energy in a major eruptive active region based on SDO/HMI observation
We report the evolution of the magnetic field and its energy in NOAA active region 11158
over five days based on a vector magnetogram series from the Helioseismic and Magnetic …
over five days based on a vector magnetogram series from the Helioseismic and Magnetic …
Flare-productive active regions
Strong solar flares and coronal mass ejections, here defined not only as the bursts of
electromagnetic radiation but as the entire process in which magnetic energy is released …
electromagnetic radiation but as the entire process in which magnetic energy is released …
The origin, early evolution and predictability of solar eruptions
Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …
Longitudinal magnetic field changes accompanying solar flares
JJ Sudol, JW Harvey - The Astrophysical Journal, 2005 - iopscience.iop.org
Abstract We have used Global Oscillation Network Group (GONG) magnetograms to
characterize the changes in the photospheric longitudinal magnetic field during 15 X-class …
characterize the changes in the photospheric longitudinal magnetic field during 15 X-class …
[CARTE][B] Plasma astrophysics, part II: reconnection and flares
BV Somov - 2012 - books.google.com
This two-part book is devoted to classic fundamentals and current practices and
perspectives of modern plasma astrophysics. This second part discusses the physics of …
perspectives of modern plasma astrophysics. This second part discusses the physics of …
The magnetic field in the solar atmosphere
This publication provides an overview of magnetic fields in the solar atmosphere with the
focus lying on the corona. The solar magnetic field couples the solar interior with the visible …
focus lying on the corona. The solar magnetic field couples the solar interior with the visible …
Automatic short-term solar flare prediction using machine learning and sunspot associations
R Qahwaji, T Colak - Solar Physics, 2007 - Springer
In this paper, a machine-learning-based system that could provide automated short-term
solar flare prediction is presented. This system accepts two sets of inputs: McIntosh …
solar flare prediction is presented. This system accepts two sets of inputs: McIntosh …