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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 …
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 …
[Књига][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 …
Magnetic reconnection during the post-impulsive phase of a long-duration solar flare: bidirectional outflows as a cause of microwave and X-ray bursts
Magnetic reconnection plays a crucial role in powering solar flares, production of energetic
particles, and plasma heating. However, where the magnetic reconnections occur, how and …
particles, and plasma heating. However, where the magnetic reconnections occur, how and …
Solar Flare Spectroscopy
L Fletcher - Annual Review of Astronomy and Astrophysics, 2024 - annualreviews.org
This review covers the techniques, observations, and inferences of solar flare spectroscopy.
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …
A model of acceleration of anomalous cosmic rays by reconnection in the heliosheath
We discuss a model of cosmic ray acceleration that accounts for the observations of
anomalous cosmic rays (ACRs) by Voyager 1 and 2. The model appeals to fast magnetic …
anomalous cosmic rays (ACRs) by Voyager 1 and 2. The model appeals to fast magnetic …
Nonequilibrium Processes in the Solar Corona, Transition Region, Flares, and Solar Wind (Invited Review)
We review the presence and signatures of the non-equilibrium processes, both non-
Maxwellian distributions and non-equilibrium ionization, in the solar transition region …
Maxwellian distributions and non-equilibrium ionization, in the solar transition region …
Particle acceleration in a transient magnetic reconnection event
Context. In the present paper, we investigate particle acceleration by direct electric field in
solar flares. Aims. Proton and electron kinetics are considered based on MHD simulations of …
solar flares. Aims. Proton and electron kinetics are considered based on MHD simulations of …
Cosmic Electrodynamics
GD Fleishman, IN Toptygin - Astrophysics and Space Science Library, 2013 - Springer
Astrophysics is a highly important part of the modern vision of the world around us. Over the
past century, it has transformed the very foundation and basic philosophical concepts on the …
past century, it has transformed the very foundation and basic philosophical concepts on the …
Early-stage coronal hard X-ray source in solar flares in the collapsing trap model
AN Shabalin, YE Charikov… - The Astrophysical …, 2022 - iopscience.iop.org
A bright hard X-ray coronal source observed at the early stage of solar flares is considered.
The plasma density in a quiet corona is not enough to explain the hard X-ray …
The plasma density in a quiet corona is not enough to explain the hard X-ray …