A number of meter wavelength solar radio bursts of spectral Type-III have been observed by means of a solar radio spectroscope (40-240 MHz) simultaneously with sudden enhancements of low frequency (164 KHz) field strength (SES's) of Radio Tashkent which are known to take place due to the enhancements of D-layer ionization caused by flare-time solar X-rays. The association between the solar X-ray flares as detected by the SES's and the Type-III meter-wave solar bursts is discussed. It is found that the association of SES's and meter wave solar bursts, which implies the ejection of flare-time electrons towards the photosphere as well as corona, is about 72%
We present some special solar radio bursts and some fine structures on the band of 1.00-7.60 GHz. Fi...
International audienceAims. Using simultaneous X-ray and radio observations from solar flares, we in...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
The paper describes an investigation of the solar radio bursts of spectral type III due to disturban...
256-260Different classes of solar optical flares, microwave bursts at 4995 MHz and sudden ionospheri...
A new acousto-optic radio spectrometer has observed the 1 - 2 GHz radio emission of solar flares wit...
The plasma-magnetic field interaction in the solar corona is caused exploration of suprathermal elec...
International audienceWe report here on the solar origin of distinctive radiation characteristics ob...
89-91Solar Hɑ-Flares reported under a scheme of classification based on their distinctive visual fea...
A preliminary correlation study of the solar burst type III with a type Iv solar burst of has been m...
The Sun is an active source of radio emission which is often associated with the acceleration of ele...
381-401An account is given of the history of solar radio astronomy, starting from the early failures...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
We have studied ionization excesses produced by enhancements of X-ray emission during solar flares u...
The solar flare phenomenon is one of the powerful events on the Sun that had been discovered in 1859...
We present some special solar radio bursts and some fine structures on the band of 1.00-7.60 GHz. Fi...
International audienceAims. Using simultaneous X-ray and radio observations from solar flares, we in...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...
The paper describes an investigation of the solar radio bursts of spectral type III due to disturban...
256-260Different classes of solar optical flares, microwave bursts at 4995 MHz and sudden ionospheri...
A new acousto-optic radio spectrometer has observed the 1 - 2 GHz radio emission of solar flares wit...
The plasma-magnetic field interaction in the solar corona is caused exploration of suprathermal elec...
International audienceWe report here on the solar origin of distinctive radiation characteristics ob...
89-91Solar Hɑ-Flares reported under a scheme of classification based on their distinctive visual fea...
A preliminary correlation study of the solar burst type III with a type Iv solar burst of has been m...
The Sun is an active source of radio emission which is often associated with the acceleration of ele...
381-401An account is given of the history of solar radio astronomy, starting from the early failures...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
We have studied ionization excesses produced by enhancements of X-ray emission during solar flares u...
The solar flare phenomenon is one of the powerful events on the Sun that had been discovered in 1859...
We present some special solar radio bursts and some fine structures on the band of 1.00-7.60 GHz. Fi...
International audienceAims. Using simultaneous X-ray and radio observations from solar flares, we in...
Observations of the solar radio spectrum have been made with high time and frequency resolution. Sp...