An extensive study of the IMP-6 and IMP-8 plasma and radio wave data was performed to try to find electron plasma oscillations associated with type III radio noise bursts and low-energy solar electrons. It is shown that electron plasma oscillations are seldom observed in association with solar electron events and type III radio bursts at 1.0 AU. For the one case in which electron plasma oscillations are definitely produced by the electrons ejected by the solar flare the electric field strength is relatively small. Electromagnetic radiation, believed to be similar to the type III radio emission, is observed coming from the region of the more intense electron plasma oscillations upstream. Quantitative calculations of the rate of conversion of...
Solar type III radio bursts are an important diagnostic tool in the understanding of solar accelerat...
During solar flares a large amount of electrons with energies greater than 20 keV is generated with ...
Energetic electrons associated with solar flares and their relation to type 1 noise activit
Many investigators have suggested that plasma oscillations in the solar corona may be the source of ...
Type III radio bursts observed at kilometric wavelengths (≲ 0.35 MHz) by the OGO-5 spacecraft are co...
Abstract. Type III radio bursts observed at kilometric wavelengths (~< 0.35 MHz) by the OGO-5 spa...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
Context. Solar activity occurs not only in terms of the well-known 11-year Sun spot cycle but also i...
Distinct Kev electron events as observed by satellites near the earth are, in general, associated wi...
All radiation processes described can take place in the solar corona, depending on different physic...
Energetic electrons propagating through the interplanetary medium are shown to excite the one dimens...
The electric field noise phenomena is described which was observed by the S3-A spacecraft near the p...
Abstract Solar type III radio bursts are an important diagnostic tool in the understanding of solar ...
The paper describes an investigation of the solar radio bursts of spectral type III due to disturban...
Abstract Solar type III radio bursts are an important diagnostic tool in the understand-ing of solar...
Solar type III radio bursts are an important diagnostic tool in the understanding of solar accelerat...
During solar flares a large amount of electrons with energies greater than 20 keV is generated with ...
Energetic electrons associated with solar flares and their relation to type 1 noise activit
Many investigators have suggested that plasma oscillations in the solar corona may be the source of ...
Type III radio bursts observed at kilometric wavelengths (≲ 0.35 MHz) by the OGO-5 spacecraft are co...
Abstract. Type III radio bursts observed at kilometric wavelengths (~< 0.35 MHz) by the OGO-5 spa...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
Context. Solar activity occurs not only in terms of the well-known 11-year Sun spot cycle but also i...
Distinct Kev electron events as observed by satellites near the earth are, in general, associated wi...
All radiation processes described can take place in the solar corona, depending on different physic...
Energetic electrons propagating through the interplanetary medium are shown to excite the one dimens...
The electric field noise phenomena is described which was observed by the S3-A spacecraft near the p...
Abstract Solar type III radio bursts are an important diagnostic tool in the understanding of solar ...
The paper describes an investigation of the solar radio bursts of spectral type III due to disturban...
Abstract Solar type III radio bursts are an important diagnostic tool in the understand-ing of solar...
Solar type III radio bursts are an important diagnostic tool in the understanding of solar accelerat...
During solar flares a large amount of electrons with energies greater than 20 keV is generated with ...
Energetic electrons associated with solar flares and their relation to type 1 noise activit