Results 21 to 30 of about 1,793,812 (174)
The Astrophysical Journal Letters, 2023 Many particles are accelerated during solar flares. To understand the acceleration and propagation processes of electrons, we require the pitch-angle distributions of the particles.
Keitarou Matsumoto +2 more
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Lightning, Solar Flares and Radio Galaxies [PDF]
Nature, 1966 IN 1925, when it was still believed that a potential of n × 109 V was necessary to cause a lightning flash1a, C. T. R. Wilson put forward the suggestion that the soft cosmic rays up to about 109 eV might be accounted for by runaway electrons in thundercloud fields1b.
openaire +1 more source
Observation of Radio Solar Flares in RNO-G
Proceedings of 39th International Cosmic Ray Conference — PoS(ICRC2025)The Radio Neutrino Observatory - Greenland (RNO-G) is a multipurpose experiment that extends its scope to sciences like solar heliophysics and radioglaciology beyond its primary focus to detect ultra-high energy neutrinos and cosmic rays. In this contribution, we discuss the recent observations of solar flares in RNO-G.
Mohammad Ful Hossain Seikh +79 more
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Hard X-rays, ejecta, and their associated decimetric radio emission in solar flares [PDF]
, 2003 We investigate temporal and spatial correlations in solar flares of hard X-rays (HXR) and decimetric continuum emissions, ejecta, and CMEs. The focus is on three M-class flares, supported by observations from other flares.
Saint-Hilaire, Pascal (author) +1 more
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Solar Radio Bursts Associated with In Situ Detected Energetic Electrons in Solar Cycles 23 and 24
Universe, 2022 The first comprehensive analysis between the in situ detected solar energetic electrons (SEEs) from ACE/EPAM satellite and remotely observed radio signatures in solar cycles (SCs) 23 and 24 (1997–2019) is presented.
Rositsa Miteva +2 more
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Cold Solar Flares. I. Microwave Domain
The Astrophysical Journal, 2023 We identify a set of ∼100 “cold” solar flares and perform a statistical analysis of them in the microwave range. Cold flares are characterized by a weak thermal response relative to nonthermal emission.
Alexandra L. Lysenko +6 more
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A catalogue of white-light flares observed by Yohkoh [PDF]
, 2003 The aspect camera of the Soft X-ray Telescope (SXT) on Yohkoh provided the first systematic survey of white-light flares from an observatory in space. The observations were made in the Fraunhofer g-band at a pixel size of 2.46 arcsec and a typical sample
H. S. Hudson +7 more
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Effects of solar flares on the ionosphere as shown by the dynamics of ionograms recorded in Europe and South Africa [PDF]
Annales Geophysicae, 2019 We have investigated the solar flare effects on ionospheric absorption with the systematic analysis of ionograms measured at midlatitude and low-latitude ionosonde stations under different solar zenith angles.
V. Barta +5 more
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Statistical analysis of solar radio fiber bursts and relations with flares
, 2021 Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although observations and theory of fiber bursts have been studied for decades, their microphysical process, emission mechanism, and especially the physical links with the ...
Baolin Tan +4 more
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Radio bursts of very short duration: Fine structure of solar flare emissions [PDF]
Geofísica Internacional, 2006 The fine time structure of sub-second radio events of solar flare emissions is described on the multichannel polarimeter of Station Basovizza at 237, 327, and 408 MHz frequencies.
R. E. Rodríguez Taboada +1 more
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