Initial results of a comparative study of major fast drift kilometric bursts and solar proton events from Sep. 1978 to Feb. 1983 are presented. It was found that only about half of all intense, long duration ( 40 min above 500 sfu) 1 MHz bursts can be associated with F 20 MeV proton events. However, for the subset of such fast drift bursts accompanied by metric Type 2 and/or 4 activity (approximately 40% of the total), the degree of association with 20 MeV events is 80%. For the reverse association, it was found that proton events with J( 20 MeV) 0.01 1 pr cm(-2)s(-1)sr(-1)MeV(-1) were typically (approximately 80% of the time) preceded by intense 1 MHz bursts that exceeded the 500 sfu level for times 20 min (median duration approximately...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
We analyze the high-energy particle emission from the Sun in two extreme solar particle events. in w...
The solar burst of 21 May 1984 presented a number of unique features. The time profile consisted of ...
We have analysed 58 high-energy proton events and 36 temporally related near-relativistic electron e...
We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar p...
Aims. We study selected properties of solar energetic particle (SEP) events as inferred from thei...
From 1996 July through 2001 June, less than half (43/98) of all favorably located (from solar wester...
A catalog of about 118 proton events, 1966-1976, not included in an earlier catalog of 81 events (AF...
Solar energetic particle events observed in space have different properties depending on the class o...
We report on further evidence that solar energetic particles are organized by the kinematic properti...
Solar energetic particle (SEP) events are commonly separated in two categories: numerous “impulsive”...
We study the solar event on 27 September 2001 that consisted of three consecutive coronal mass ejec...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
We analyze the relations between various combinations of peak fluxes and fluences of solar microwave...
Using the ISEE-3 radio astronomy experiment data 37 interplanetary (IP) type II bursts have been ide...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
We analyze the high-energy particle emission from the Sun in two extreme solar particle events. in w...
The solar burst of 21 May 1984 presented a number of unique features. The time profile consisted of ...
We have analysed 58 high-energy proton events and 36 temporally related near-relativistic electron e...
We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar p...
Aims. We study selected properties of solar energetic particle (SEP) events as inferred from thei...
From 1996 July through 2001 June, less than half (43/98) of all favorably located (from solar wester...
A catalog of about 118 proton events, 1966-1976, not included in an earlier catalog of 81 events (AF...
Solar energetic particle events observed in space have different properties depending on the class o...
We report on further evidence that solar energetic particles are organized by the kinematic properti...
Solar energetic particle (SEP) events are commonly separated in two categories: numerous “impulsive”...
We study the solar event on 27 September 2001 that consisted of three consecutive coronal mass ejec...
The search of solar bursts recorded in 1968 and 1970 at 408 MHz shows the presence of bursts not cor...
We analyze the relations between various combinations of peak fluxes and fluences of solar microwave...
Using the ISEE-3 radio astronomy experiment data 37 interplanetary (IP) type II bursts have been ide...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
We analyze the high-energy particle emission from the Sun in two extreme solar particle events. in w...
The solar burst of 21 May 1984 presented a number of unique features. The time profile consisted of ...