The relationship between solar radio and hard X-ray emission
This review discusses the complementary relationship between radio and hard X-ray
observations of the Sun using primarily results from the era of the Reuven Ramaty High …
observations of the Sun using primarily results from the era of the Reuven Ramaty High …
Incoherent solar radio emission
A Nindos - Frontiers in Astronomy and Space Sciences, 2020 - frontiersin.org
Incoherent solar radio radiation comes from the free-free, gyroresonance, and
gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb …
gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb …
Fast gyrosynchrotron codes
GD Fleishman, AA Kuznetsov - The Astrophysical Journal, 2010 - iopscience.iop.org
Radiation produced by charged particles gyrating in a magnetic field is highly significant in
the astrophysics context. Persistently increasing resolution of astrophysical observations …
the astrophysics context. Persistently increasing resolution of astrophysical observations …
Magnetic-island contraction and particle acceleration in simulated eruptive solar flares
The mechanism that accelerates particles to the energies required to produce the observed
high-energy impulsive emission in solar flares is not well understood. Drake et al. proposed …
high-energy impulsive emission in solar flares is not well understood. Drake et al. proposed …
Implosion of coronal loops during the impulsive phase of a solar flare
We study the relationship between implosive motions in a solar flare, and the energy
redistribution in the form of oscillatory structures and particle acceleration. The flare …
redistribution in the form of oscillatory structures and particle acceleration. The flare …
The Young Binary DQ Tau: a hunt for X-ray emission from colliding magnetospheres
KV Getman, PS Broos, DM Salter… - The Astrophysical …, 2011 - iopscience.iop.org
The young high-eccentricity binary DQ Tau exhibits powerful recurring millimeter-band (mm)
flaring attributed to collisions between the two stellar magnetospheres near periastron, when …
flaring attributed to collisions between the two stellar magnetospheres near periastron, when …
Three-dimensional simulations of gyrosynchrotron emission from mildly anisotropic nonuniform electron distributions in symmetric magnetic loops
AA Kuznetsov, GM Nita… - The Astrophysical …, 2011 - iopscience.iop.org
Microwave emission of solar flares is formed primarily by incoherent gyrosynchrotron
radiation generated by accelerated electrons in coronal magnetic loops. The resulting …
radiation generated by accelerated electrons in coronal magnetic loops. The resulting …
Flare quasi-periodic pulsations with growing periodicity
VE Reznikova, K Shibasaki - Astronomy & Astrophysics, 2011 - aanda.org
We conducted a wavelet analysis of the flare intensity variations for the long duration flare
on 2005 August 22 observed with the Nobeyama Radioheliograph at frequencies 17 and 34 …
on 2005 August 22 observed with the Nobeyama Radioheliograph at frequencies 17 and 34 …
Magnetic field measurements in a limb solar flare by hydrogen, helium and ionized calcium lines
We present simultaneous magnetic field measurements for the limb solar flare of 1981 July
17 using of the Ca II K, Hδ, He I 4471.5 Å and Hβ lines. For two moments during the flare …
17 using of the Ca II K, Hδ, He I 4471.5 Å and Hβ lines. For two moments during the flare …
Comparative study of electric currents and energetic particle fluxes in a solar flare and Earth magnetospheric substorm
A Artemyev, I Zimovets, I Sharykin… - The Astrophysical …, 2021 - iopscience.iop.org
Magnetic field line reconnection is a universal plasma process responsible for the
conversion of magnetic field energy to plasma heating and charged particle acceleration …
conversion of magnetic field energy to plasma heating and charged particle acceleration …