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solar surge

First detection of metric emission from a solar surge by Costas Alissandrakis et al.*

2022-07-19

Practically all solar phenomena observed in radio wavelengths have their counterpart in other regions of the electromagnetic spectrum. Metric solar bursts are an exception to the above statement. Although we have a basic understanding of their origin, some of their counterparts in other spectral ranges have not been identified, with the exception of the so called “radio CMEs”. This is apparently because metric bursts result from coherent plasma emission, which […]

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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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