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[HTML][HTML] Solar flares: magnetohydrodynamic processes
This paper outlines the current understanding of solar flares, mainly focused on
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …
Evolution of active regions
The evolution of active regions (AR) from their emergence through their long decay process
is of fundamental importance in solar physics. Since large-scale flux is generated by the …
is of fundamental importance in solar physics. Since large-scale flux is generated by the …
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) …
[HTML][HTML] Basic topology of twisted magnetic configurations in solar flares
Basic topology of twisted magnetic configurations in solar flares ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …
It will be completely retired in October 2019. This page will automatically redirect to the new …
Heating of the solar chromosphere and corona by Alfvén wave turbulence
ABSTRACT A three-dimensional magnetohydrodynamic (MHD) model for the propagation
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …
Magnetic fields in the solar convection zone
Y Fan - Living Reviews in Solar Physics, 2021 - Springer
It has been a prevailing picture that active regions on the solar surface originate from a
strong toroidal magnetic field stored in the overshoot region at the base of the solar …
strong toroidal magnetic field stored in the overshoot region at the base of the solar …
Critical issues for understanding particle acceleration in impulsive solar flares
This paper, a review of the present status of existing models for particle acceleration during
impulsive solar flares, was inspired by a week‐long workshop held in the Fall of 1993 at …
impulsive solar flares, was inspired by a week‐long workshop held in the Fall of 1993 at …
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 …
[ספר][B] Particle acceleration and kinematics in solar flares: a synthesis of recent observations and theoretical concepts (invited review)
MJ Aschwanden, MJ Aschwanden - 2002 - Springer
We review the physical processes of particle acceleration, injection, propagation, trap**,
and energy loss in solar flare conditions. An understanding of these basic physical …
and energy loss in solar flare conditions. An understanding of these basic physical …
A model for solar polar jets
We propose a model for the jetting activity that is commonly observed in the Sun's corona,
especially in the open-field regions of polar coronal holes. Magnetic reconnection is the …
especially in the open-field regions of polar coronal holes. Magnetic reconnection is the …