Add to ORKGSince the launch of the Gamma Ray Observatory (GRO) in Apr. 1991, the Burst and Transient Source Experiment (BATSE) instrument on GRO has recorded a large number of solar flares. Some of these flares have also been observed by the Gamma-Ray Burst Detector on the Pioneer Venus Orbiter (PVO) and/or by the Solar X-Ray/Cosmic Gamma-Ray Burst Experiment on the Ulysses spacecraft. A preliminary list of common flares observed during the period May-Jun. 1991 is presented and the possible joint studies are indicated
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Soci...
The launch of the Gamma Ray Observatory (GRO) near solar maximum makes solar flare studies early in ...
A balloon-borne X- and gamma-ray instrument was developed, fabricated, and flown. This instrument ha...
The Hard X-Ray Burst Spectrometer (HXRBS) group at GSFC has developed and is maintaining a quick-loo...
The February 16, 1984 (0900 UT) solar flare was very energetic and produced a variety of emissions. ...
Ulysses was launched in October 1990, and its Solar X-ray/Cosmic Gamma-Ray Burst Experiment (GRB) ha...
The Burst and Transient Source Experiment (BATSE) for the Gamma Ray Observatory (GRO) consists of ei...
The objective of this grant was to measure the spatial structure and directivity of the hard X-ray a...
Abstract. The hard X-ray/gamma-ray (HXR/GR) impulsive burst on 1991 June 30 (0255 UT) was associated...
The hard X-ray emission from the “giant” solar flare on 4 November 2003 (~1947 UT) was observed by t...
This report describes work performed under contract NAS5-32584 for Phase 3 of the Compton Gamma Ray ...
Solar flare neutrons and gamma rays are produced by nuclear interactions of flare accelerated ions i...
A list of publications resulting from this program includes 'The Timing of Electron Beam Signatures ...
The hard X-ray component in the impulsive phase of solar flares is reported. Observations from OGO-5...
We have carried out high-spatial-resolution millimeter observations of solar flares using the Berkel...
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Soci...
The launch of the Gamma Ray Observatory (GRO) near solar maximum makes solar flare studies early in ...
A balloon-borne X- and gamma-ray instrument was developed, fabricated, and flown. This instrument ha...
The Hard X-Ray Burst Spectrometer (HXRBS) group at GSFC has developed and is maintaining a quick-loo...
The February 16, 1984 (0900 UT) solar flare was very energetic and produced a variety of emissions. ...
Ulysses was launched in October 1990, and its Solar X-ray/Cosmic Gamma-Ray Burst Experiment (GRB) ha...
The Burst and Transient Source Experiment (BATSE) for the Gamma Ray Observatory (GRO) consists of ei...
The objective of this grant was to measure the spatial structure and directivity of the hard X-ray a...
Abstract. The hard X-ray/gamma-ray (HXR/GR) impulsive burst on 1991 June 30 (0255 UT) was associated...
The hard X-ray emission from the “giant” solar flare on 4 November 2003 (~1947 UT) was observed by t...
This report describes work performed under contract NAS5-32584 for Phase 3 of the Compton Gamma Ray ...
Solar flare neutrons and gamma rays are produced by nuclear interactions of flare accelerated ions i...
A list of publications resulting from this program includes 'The Timing of Electron Beam Signatures ...
The hard X-ray component in the impulsive phase of solar flares is reported. Observations from OGO-5...
We have carried out high-spatial-resolution millimeter observations of solar flares using the Berkel...
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Soci...
The launch of the Gamma Ray Observatory (GRO) near solar maximum makes solar flare studies early in ...
A balloon-borne X- and gamma-ray instrument was developed, fabricated, and flown. This instrument ha...