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September 2022

Narrowband Spikes Observed During the 13 June 2012 Flare in the 800 – 2000 MHz Range by Marian Karlicky et al

2022-09-06

The solar radio spikes can provide detailed information about plasma processes in solar flares on kinetic scales. Among them, the decimetric spikes belong to the most interesting ones because they are recorded in some cases close to the starting frequency of Type-III bursts and in relation to hard X-ray emissions. Stepanov et al. (1999) and Bárta and Karlický (2001) presented models where spike frequencies correspond to those of the upper-hybrid […]

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active regions (3) Atacama Large Millimeter Array (ALMA) (9) chromosphere (12) CME-CME interaction (3) coronal magnetic field (12) Coronal Mass Ejection (CME) (41) density fluctuations (11) energetic electrons (13) fast magnetoacoustic waves (3) fine spectral structures (4) free-free emission (7) Giant Metrewave Radio Telescope (GMRT) (3) gyrosynchrotron emission (12) ionosphere (4) Langmuir waves (7) Low Frequency Array (LOFAR) (19) microwave emission (11) Murchison Widefield Array (MWA) (9) Nancay Radio Heliograph (NRH) (5) Nobeyama Radioheliograph (NoRH) (7) Parker Solar Probe (PSP) (7) particle acceleration (8) plasma radio emission (6) quiet Sun (8) radio spikes (9) radio wave scattering (11) shock wave (7) simulations (4) Solar and Heliospheric Observatory (SOHO) (3) Solar Dynamics Observatory (SDO) (3) solar energetic particles (SEP) (23) solar flare (28) solar radio emission (19) space weather (4) STEREO (6) submillimeter emission (4) turbulence (13) Type III solar radio bursts (52) Type II solar radio bursts (32) Type I solar radio bursts (6) Type IV solar radio bursts (10) Ukrainian T-shaped radio telescope (UTR-2) (4) Ultraviolet (UV)/extreme ultraviolet (EUV) emissions (5) Wind (spacecraft) (3) zebra-structure (6)
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  • Anisotropic density turbulence variation from the low corona to 1 au as deduced from solar radio observations by E. Kontar et al.

    2023-11-30

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