Type III radio bursts observed at kilometric wavelengths (≲ 0.35 MHz) by the OGO-5 spacecraft are compared with > 45 keV solar electron events observed near 1 AU by the IMP-5 and Explorer 35 spacecraft for the period March 1968–November 1969.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/43725/1/11207_2004_Article_BF00165288.pd
Aims. We investigate the conditions under which small-scale energy release events in the low corona ...
During 13th of May 2015, the solar wind is very high velocity, which is 733 kms-1 as compared to 367...
Solar type III radio bursts are the most common impulsive radio signatures from the Sun, stimulated ...
Abstract. Type III radio bursts observed at kilometric wavelengths (~< 0.35 MHz) by the OGO-5 spa...
Type III bursts were observed between 3.5 MHz and 50 kHz by the University of Michigan radio astrono...
IMP-6 spacecraft observations of low frequency radio emission, fast electrons, and solar wind plasma...
An extensive study of the IMP-6 and IMP-8 plasma and radio wave data was performed to try to find el...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
The flux of fast solar electrons and the intensity of the type 111 radio emission generated by these...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
Type III solar radio bursts were observed from 10 MHz to 10 KHz by satellite experiments above the t...
A type III solar burst was observed at seven frequencies between 3.5 MHz and 80 kHz by the Michigan ...
Aims. Type III radio bursts are intense radio emissions triggered by beams of energetic electrons of...
During solar flares a large amount of electrons with energies greater than 20 keV is generated with ...
Distinct Kev electron events as observed by satellites near the earth are, in general, associated wi...
Aims. We investigate the conditions under which small-scale energy release events in the low corona ...
During 13th of May 2015, the solar wind is very high velocity, which is 733 kms-1 as compared to 367...
Solar type III radio bursts are the most common impulsive radio signatures from the Sun, stimulated ...
Abstract. Type III radio bursts observed at kilometric wavelengths (~< 0.35 MHz) by the OGO-5 spa...
Type III bursts were observed between 3.5 MHz and 50 kHz by the University of Michigan radio astrono...
IMP-6 spacecraft observations of low frequency radio emission, fast electrons, and solar wind plasma...
An extensive study of the IMP-6 and IMP-8 plasma and radio wave data was performed to try to find el...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
The flux of fast solar electrons and the intensity of the type 111 radio emission generated by these...
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams prop...
Type III solar radio bursts were observed from 10 MHz to 10 KHz by satellite experiments above the t...
A type III solar burst was observed at seven frequencies between 3.5 MHz and 80 kHz by the Michigan ...
Aims. Type III radio bursts are intense radio emissions triggered by beams of energetic electrons of...
During solar flares a large amount of electrons with energies greater than 20 keV is generated with ...
Distinct Kev electron events as observed by satellites near the earth are, in general, associated wi...
Aims. We investigate the conditions under which small-scale energy release events in the low corona ...
During 13th of May 2015, the solar wind is very high velocity, which is 733 kms-1 as compared to 367...
Solar type III radio bursts are the most common impulsive radio signatures from the Sun, stimulated ...