Add to ORKGCorrelations between X-ray and type 3 radio emission of solar bursts are described through a bivariate distribution function. Procedures for determining the form of this distribution are described. A model is constructed to explain the correlation between the X-ray spectral index and the ratio of X-ray to radio intensities. Implications of the model are discussed
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
We investigate the relative timing between hard X-ray (HXR) peaks and structures in metric and decim...
Peak fluxes of flare-associated 8–12 Å X-ray bursts occur at or near the time of the maximum energy ...
A large number of hard X-ray events which were recorded by the Hard X-Ray Burst Spectrometer (HXRBS)...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
International audienceContext: Flare-accelerated electrons may produce closely temporarily related h...
Context. Type III bursts and hard X-rays are both produced by flare energetic electron beams. The li...
Aims: Using simultaneous X-ray and radio observations from solar flares, we investigate the link betw...
Type III solar bursts occurring in the absence of solar flares were observed to be accompanied by we...
International audienceAims. Using simultaneous X-ray and radio observations from solar flares, we in...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
We investigate the relative timing between hard X-ray (HXR) peaks and structures in metric and decim...
Peak fluxes of flare-associated 8–12 Å X-ray bursts occur at or near the time of the maximum energy ...
A large number of hard X-ray events which were recorded by the Hard X-Ray Burst Spectrometer (HXRBS)...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
Aims. Using simultaneous X-ray and radio observations from solar flares, we investigate th...
International audienceContext: Flare-accelerated electrons may produce closely temporarily related h...
Context. Type III bursts and hard X-rays are both produced by flare energetic electron beams. The li...
Aims: Using simultaneous X-ray and radio observations from solar flares, we investigate the link betw...
Type III solar bursts occurring in the absence of solar flares were observed to be accompanied by we...
International audienceAims. Using simultaneous X-ray and radio observations from solar flares, we in...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
International audienceContext. Type III bursts and hard X-rays are both produced by flare energetic ...
We investigate the relative timing between hard X-ray (HXR) peaks and structures in metric and decim...
Peak fluxes of flare-associated 8–12 Å X-ray bursts occur at or near the time of the maximum energy ...