Results 1 to 10 of about 20,265 (219)
RADIO EMISSION FROM ACCELERATION SITES OF SOLAR FLARES [PDF]
ApJL, in ...
Li, Yixuan, Fleishman, Gregory D.
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Operational prediction of solar flares using a transformer-based framework [PDF]
Solar flares are explosions on the Sun. They happen when energy stored in magnetic fields around solar active regions (ARs) is suddenly released. Solar flares and accompanied coronal mass ejections are sources of space weather, which negatively affects a
Yasser Abduallah +3 more
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Correlation between active regions’ spectra at high radio frequencies and solar flare occurrences [PDF]
High radio frequencies observations with the Italian network of large single-dish radio telescopes resulted in $$\sim$$ 450 solar images between 2018 and 2023 in K-band frequency range (18–26 GHz).
Sara Mulas +33 more
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Space weather study through analysis of solar radio bursts detected by a single-station CALLISTO spectrometer [PDF]
This article summarises the results of an analysis of solar radio bursts (SRBs) detected by the Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) spectrometer hosted by the University of ...
T. Ndacyayisenga +3 more
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Are There Radio-quiet Solar Flares? [PDF]
ISSN:0038 ...
Benz, Arnold +2 more
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Investigation of the Sudden Solar Ionospheric Disturbance using Radio Telescope [PDF]
Low-frequency radio telescopes are cheap and useful devices for the investigation of terrestrial and extra-terrestrial emissions. These emissions come either from the Sun and the planet Jupiter to terrestrial emissions.
Aqasha Adam +3 more
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Increased solar radiation during solar flare events can cause additional ionization and enhanced absorption of the electromagnetic (EM) waves in the ionosphere leading to partial or even total radio fade-outs.
Attila Buzás +8 more
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M-Class Solar Flares in Solar Cycles 23 and 24: Properties and Space Weather Relevance
A comprehensive statistical analysis on the properties and accompanied phenomena of all M-class solar flares (as measured in soft X-rays) in the last two solar cycles (1996–2019) is presented here with a focus on their space weather potential.
Rositsa Miteva, Susan W. Samwel
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Soil Moisture and Ocean Salinity (SMOS) is an ESA mission observing Earth at 1.4 GHz with full polarimetry. SMOS images are affected by a noise of solar origin produced by the Sun appearing in the antenna's field of view.
M. Flores‐Soriano +2 more
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This work proposes a new indirect method to detect the impact of solar flares on ionospheric sounding measurements, i.e., on the signal-to-noise ratio of ionospheric reflected radio signals. The method allows us to detect and characterize the ionospheric
Victor de Paula +4 more
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