Magnetohydrodynamic fast sausage waves in the solar corona
Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …
New Insights from Imaging Spectroscopy of Solar Radio Emission
DE Gary - Annual Review of Astronomy and Astrophysics, 2023 - annualreviews.org
Newly available high-resolution imaging of solar radio emission at many closely spaced
frequencies and times provides new physical insight into the processes, structure, and …
frequencies and times provides new physical insight into the processes, structure, and …
Measurement of magnetic field and relativistic electrons along a solar flare current sheet
In the standard model of solar flares, a large-scale reconnection current sheet is postulated
to be the central engine for powering the flare energy release,–and accelerating particles …
to be the central engine for powering the flare energy release,–and accelerating particles …
Decay of the coronal magnetic field can release sufficient energy to power a solar flare
Solar flares are powered by a rapid release of energy in the solar corona, thought to be
produced by the decay of the coronal magnetic field strength. Direct quantitative …
produced by the decay of the coronal magnetic field strength. Direct quantitative …
Solar science with the Atacama Large Millimeter/Submillimeter Array—a new view of our Sun
Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …
Three-dimensional radio and X-ray modeling and data analysis software: Revealing flare complexity
GM Nita, GD Fleishman, AA Kuznetsov… - The Astrophysical …, 2015 - iopscience.iop.org
Many problems in solar physics require analysis of imaging data obtained in multiple
wavelength domains with differing spatial resolution in a framework supplied by advanced …
wavelength domains with differing spatial resolution in a framework supplied by advanced …
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 …
[PDF][PDF] Multiwave Siberian Radioheliograph
AT Altyntsev, SV Lesovoi, MV Globa, AV Gubin… - Solar-Terrestrial …, 2020 - ru.iszf.irk.ru
The article discusses characteristics, fundamental and applied tasks of the Siberian
Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory …
Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory …
The first flare observation with a new solar microwave spectrometer working in 35–40 GHz
F Yan, Z Wu, Z Shang, B Wang, L Zhang… - The Astrophysical …, 2022 - iopscience.iop.org
The microwave spectrum contains valuable information about solar flares. Yet, the present
spectral coverage is far from complete and broad data gaps exist above 20 GHz. Here we …
spectral coverage is far from complete and broad data gaps exist above 20 GHz. Here we …