On the Issue of the Origin of Type II Solar Radio Bursts
Astrophysical Journal, 2021 Type II solar radio bursts are among the most powerful events in the solar radio emission in the meter wavelength range. It is generally accepted that the agents generating type II radio bursts are magnetohydrodynamic shock waves.
G. Chernov, V. Fomichev
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Time evolution of high-altitude plasma bubbles imaged at geomagnetic conjugate points [PDF]
Annales Geophysicae, 2004 Temporal and spatial evolution of two high-altitude plasma bubbles (evening and midnight) was observed on 4 April 2002, at geomagnetic conjugate points at Sata, Japan (magnetic latitude 24° N), and Darwin, Australia (magnetic latitude 22° S ...
K. Shiokawa +3 more
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Anisotropic Radio-wave Scattering and the Interpretation of Solar Radio Emission Observations [PDF]
Astrophysical Journal, 2019 The observed properties (i.e., source size, source position, time duration, and decay time) of solar radio emission produced through plasma processes near the local plasma frequency, and hence the interpretation of solar radio bursts, are strongly ...
E. P. Kontar +10 more
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An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations
The Astrophysical Journal, 2023 Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions.
Eduard P. Kontar +7 more
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Space weather study through analysis of solar radio bursts detected by a single-station CALLISTO spectrometer [PDF]
Annales Geophysicae, 2021 This article summarises the results of an analysis of solar radio bursts (SRBs) detected by the Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) spectrometer hosted by the University of ...
T. Ndacyayisenga +3 more
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PROGRESS IN THE STUDY OF DECAMETER-WAVELENGTH SOLAR RADIO EMISSION WITH UKRAINIAN RADIO TELESCOPES. Part 1. (Invited paper) [PDF]
Radio Physics and Radio Astronomy, 2023 Subject and Purpose. Results are presented of the solar corona investigations performed with the world famous Ukrainian radio telescopes. The work has been aimed at offering a consistent review of recent achievements in observations of a variety of low ...
A. A. Stanislavsky +3 more
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ORFEES – a radio spectrograph for the study of solar radio bursts and space weather applications
Journal of Space Weather and Space Climate, 2021 Radio bursts are sensitive tracers of non-thermal electron populations in the solar corona. They are produced by electron beams and shock waves propagating through the corona and the heliosphere, and by trapped electron populations in coronal mass ...
Hamini Abdallah +10 more
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Solar Radio Burst Detection Based on the MobileViT-SSDLite Lightweight Model
The Astrophysical Journal Supplement Series, 2023 Real-time detection of solar radio bursts is crucial in solar physics research and space weather forecasting. However, current research on the automatic detection of solar radio bursts is limited to identifying the presence or absence of solar radio ...
Hailan He +4 more
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Automated Detection of Solar Radio Bursts Using a Statistical Method [PDF]
Solar Physics, 2019 Radio bursts from the solar corona can provide clues to forecast space-weather hazards. After recent technology advancements, regular monitoring of radio bursts has increased and large observational datasets are produced. Hence, manual identification and
Dayal Singh +4 more
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Galactic and cosmological fast radio bursts as scaled-up solar radio bursts
Monthly notices of the Royal Astronomical Society, 2020 Fast radio bursts (FRBs) are bright milliseconds radio transients with large dispersion measures. Recently, FRB 200428 was detected in temporal coincidence with a hard X-ray flare from the Galactic magnetar SGR 1935+2154, which supports that at least ...
F. Wang, G. Q. Zhang, Z. Dai
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