Physics
Scientist
Nauchno-Issledovatel'skii Radiofizicheskii Institut, Gorki, USSR
Correlation between quasiperiodic fluctuations of period longer than 30 min in 3-cm solar radio emission and the development of proton flares
Existence of a relation between quasi-periodic pulsations with periods greater than 30 min in solar 3-cm radio emission and the onset of proton flares
Flare-associated variations in the spectral slope of radio emission (λ≈3 cm) from solar active regions
Flare-associated variations in the spectral slope of radio emission /lambda approximately 3 cm/ from solar active regions
Manifestation of pulsation instability in solar radio emission preceding proton flares
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