- + Temporally resolved Type III solar radio bursts in the frequency range 3-13 MHz by A. Vecchio et al.—Type III radio bursts are the most common coherent radio emission produced by the Sun. They are characterized by a rapid drift in time towards lower f...
- + Spectral cleaving in solar type II radio bursts: Observations and interpretation by A. Koval et al.—Solar eruptive events, such as flares and coronal mass ejections (CMEs), can generate shock waves that propagate through the solar corona. These shock...
- + A Possible Indication of the Insufficiency of Simplistic Homogeneous Models for Estimating Magnetic Fields of CMEs using Gyrosynchrotron Emission by Devojyoti Kansabanik et al.—Coronal mass ejections (CMEs) are large-scale plasma and magnetic field expulsions from the solar corona into the heliosphere. The magnetic field entr...
- + Observations of coronal holes with the Siberian Radio Heliograph by Altyntsev et al.—Coronal holes (CHs) are regions of reduced brightness in solar disk images in extreme ultraviolet (EUV) or soft X-ray emissions corresponding to confi...
- + Generation of Series of Meter/Decimeter III type Bursts During Thermal Phase of Solar Flare by Meshalkina and Altyntsev—It has been established that decimeter type III bursts are generated in the upper corona by electron beams. However, many questions remain about their...
- + Periods and frequency drifts of groups of narrowband decimetric spikes by M. Karlický, J. Dudík and J. Rybák—The narrowband decimetric spikes belong to the most interesting solar radio bursts, because they are connected to the primary flare process. Their br...
- + Time-Profile Study of Type III Solar Radio Bursts Using Parker Solar Probe by Tulsi Thapa and Yihua Yan—Type III solar radio bursts are frequent and powerful radio emissions caused by electron beams travelling through the solar corona into the interplane...
- + The angular and frequency dependence of solar radio burst rise and decay times using multi-spacecraft observations by Nicolina Chrysaphi et al.—Density fluctuations populating the heliosphere interfere with propagating radio photons, altering their trajectories through frequency-dependent effe...
- + A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 24 by Bendict Lawrance et al.—Metric type II radio bursts are a type of solar radio emission characterized by a slowly drifting radio emission observed in dynamic spectra. They are...
- + GUI for the e – CALLISTO Data: Analysis of Type II and Type III Solar Radio Bursts by Yashan Hettiarachchi et al.—Solar radio bursts (SRBs) are sudden peaks in the low-frequency radio emissions originating from the sun. These emissions can also help predict space ...
- + Energetics of compressive waves in the solar corona by Francesco Azzollini et al—Inelastic scattering off moving or oscillating density fluctuations leads to broadening of radio signals propagating in the solar corona and solar win...
- + Data Release of Solar Radio Bursts observed by CBSm at the metric wavelength by Yao Chen et al.—Here we release the spectral data of solar radio bursts recorded by the Chashan Broadband Solar radio spectrograph (CBSm), located in the Chashan moun...
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