Posted by Eduard Kontar | March 14, 2025 | Science highlights
Magnetic Field Geometry and Anisotropic Scattering Effects to Explain Puzzling LOFAR Solar Radio Burst Observations
by D. L. Clarkson et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3950
by D. L. Clarkson et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3950
Spectral Characteristics of Fundamental–Harmonic Pairs of Interplanetary Type III Radio Bursts Observed by PSP,
by Ling Chen et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3957
Flare Accelerated Electron Transport in Type III Solar Radio Bursts: large-scale transport and super-diffusive beam expansion
by E. P. Kontar et al.
https://www.astro.gla.ac.uk/users/eduard/cesra/?p=3930