- + Spectroscopic Imaging of the Sun with MeerKAT: Opening a New Frontier in Solar Physics by Kansabanik et al.—Since the discovery of solar radio emission in the late 1940s, the Sun has been studied in great detail across a wide range of frequencies from a few ...
- + Weak Solar Radio Bursts from the Solar Wind Acceleration Region Observed by the Parker Solar Probe and Its Probable Emission Mechanism by Ling Chen et al.—The study of solar wind acceleration and coronal heating has been a major challenge in solar physics. The main difficulty is that the collisionless ch...
- + An Interactive Visual Tool for the Anisotropic Scattering of Solar Radio Bursts by Daniel L. Clarkson et al—The turbulent heliosphere has a significant effect on the observed characteristics of radio emission produced in, or viewed through, the solar atmosph...
- + The physics of solar spectral imaging observations in dm-cm wavelengths and space weather by Tan et al.—Recent years, several new generation solar radio telescopes operating in the centimeter decimeter (dm-cm) wavelengths have emerged in the world, inclu...
- + Source positions of an interplanetary type III radio burst and anisotropic radio-wave scattering by X. Chen et al.—Interplanetary solar radio type III bursts provide the means to remotely study and track energetic electrons propagating in the interplanetary medium....
- + Anisotropic density turbulence variation from the low corona to 1 au as deduced from solar radio observations by E. Kontar et al.—Density turbulence in the solar corona and solar wind is evident via the properties of solar radio bursts; angular scattering-broadening of extra-sola...
- + Separating the effects of earthside and far side solar events by Silja Pohjolainen et al.—During times of high solar activity flares and coronal mass ejections (CMEs) occur close in time, sometimes even simultaneously, and it may be difficu...
- + Deciphering Faint Gyrosynchrotron Emission from a Coronal Mass Ejection Using Spectropolarimetric Radio Imaging by Devojyoti Kansabanik, Surajit Mondal and Divya Oberoi—Coronal mass ejections (CMEs) are large-scale expulsion of plasma and magnetic fields from the solar corona into the heliosphere. Magnetic field entra...
- + A New 6-15 GHz Solar Radio Observation System, by Lei Zhang et al.—In the decimeter to centimeter wavelength, solar radio emission during bursts are generally accepted to be generated by gyrosynchrotron. The typical g...
- + Morphology of solar type II bursts caused by shock propagation through turbulent and inhomogeneous coronal plasma by A. Koval et al—Type II solar bursts are radio signatures of shock waves in the solar corona driven by solar flares or coronal mass ejections. Therefore, these bursts...
As of 4/30/24 12:28pm. Last new 4/22/24 2:56am. Score: 309
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