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  • 1
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    Radial gradients of galactic cosmic ray protons and helium nuclei (1973)
    In:  CASI
    Details
    Publication Date: 2006-03-26
    Description: Variation of the cosmic ray intensity as a function away from the sun and its radial derivative is studied by plotting satellite cosmic ray measurements against sea level neutron monitor data. Results show that the solar modulation cavity extends well beyond 2 AU and that irregularities in the sun's magnetic field are carried outward radially by the solar wind, thus sweeping low energy cosmic rays out of the solar system and at the same time cooling cosmic rays reaching the earth.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci.; p 45-48
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  • 2
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    The anomalous abundance of cosmic-ray nitrogen and oxygen nuclei at low energies (1974)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Recent measurements using the Goddard-University of New Hampshire cosmic-ray telescope on the Pioneer 10 spacecraft have revealed an anomalous spectrum of nitrogen and oxygen nuclei relative to other nuclei such as He and C, in the energy range 3-30 MeV per nucleon. The intensity of nitrogen and oxygen nuclei is enhanced by a factor of up to 20 relative to their abundance in galactic or solar cosmic rays. It is argued that this is most likely a new extrasolar component of cosmic rays.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 187; Feb. 1
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  • 3
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    Pioneer-10 measurements of the differential and integral cosmic-ray gradient between 1 and 3 astronomical units (1973)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 185; Nov. 1
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  • 4
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    Atmospheric secondary and re-entrant albedo protons. (1967)
    In:  Other Sources
    Details
    Publication Date: 2011-08-11
    Description: Balloon sounding data for atmospheric secondary and reentrant albedo proton intensity values, discussing empirical atmospheric secondary proton spectrum
    Keywords: SPACE RADIATION
    Type: JOURNAL OF GEOPHYSICAL RESEARCH
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  • 5
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    High-resolution spectroscopy of two gamma-ray bursts in 1978 November (1980)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: The first results from the ISEE 3 radiatively cooled germanium gamma-ray burst spectrometer are presented. Spectra and time histories from two events on 1978 November 4 and 19 are given. A significant difference in the continuum spectra for the two events was observed. Evidence is presented for two spectral features in the November 19 event, a broad one at about 420 keV and a narrower one at about 740 keV with a suggestion of an accompanying high-energy tail.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 236
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  • 6
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    Neutron stars as sources of gamma-ray bursts: Constraints from X-ray observations of source locations (1982)
    In:  Other Sources
    Details
    Publication Date: 2011-08-18
    Description: Results for three burst locations observed with the imaging proportional counter of the Einstein Observatory are given. The observations are used to determine temperature and accretion constraints for the burst source.
    Keywords: SPACE RADIATION
    Type: Max-Planck Inst. of Physics and Astrophysics Accreting Neutron Stars; p 237-239
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  • 7
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    Search for gamma-ray bursts with coincident balloon flights (1977)
    In:  Other Sources
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    Publication Date: 2011-08-17
    Description: Dual balloon experiments were flown at separations of over 1,500 km in an attempt to determine whether cosmic gamma-ray bursts could be detected in the size region of 10 to the -7th power to several times 10 to the -6th power erg per sq cm, that is, below the apparent bend in the size spectrum of Vela events as described by Strong and Klebesadel. Fluctuations of the counting rates of photons above 150 keV with temporal structures from microseconds to several minutes were compared in order to detect coincident or associated responses from the two instruments. No coincident gamma-ray burst events were detected. Associated counting rate increases were detected, presenting a background, event-confusing problem for any single gamma-ray burst instrument beneath the earth's trapped radiation.
    Keywords: SPACE RADIATION
    Type: Nature; 266; Apr. 21
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  • 8
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    Energetic particles in the Jovian magnetosphere (1974)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Detail account of the Pioneer 10 encounter with Jupiter as viewed by the Goddard-University of New Hampshire cosmic ray experiment. Flux time histories of electrons and protons are given over a wide energy band. These show a marked variation with magnetic latitude. Significant removal of low-energy protons by Io is apparent in the inner magnetosphere (less than or equal to 6 Jovian radii). Proton and electron energy spectra are given at various Jovicentric distances. The electron spectra are remarkably hard and constant in slope in the 0.12 to 8.0-MeV interval, the electron spectral index having a value of 1.5 to 2.0 in the region outside 25 Jovian radii. Proton spectra are shown to transform from a power law with indices in the 3 to 4.2 range to more nearly exponential forms in the inner regions (less than or equal to 40 Jovian radii). Extensive data are presented on the angular distributions of protons and electrons at various locations in the Jovicentric magnetosphere.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 79; Sept. 1
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  • 9
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    The interplanetary acceleration of energetic nucleons (1976)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Corotating proton and electron streams are the dominant type of low-energy (i.e., 0.1-10 MeV per nucleon) particle event observed at 1 AU. The radial dependence of these events has been studied between 1 and 4 AU using essentially identical low-energy detector systems on IMP-7, Pioneer-10, and Pioneer-11. It had been expected that at a given energy, the intensity of these streams would decrease rapidly with heliocentric distance due to the effects of interplanetary adiabatic deceleration. Instead, it is observed that from event to event, the intensity either remains roughly constant or increases significantly (more than an order of magnitude) between 1 and 4 AU. It appears that interplanetary acceleration processes are the most plausible explanation. Several possible acceleration models are discussed.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 203; Feb. 1
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  • 10
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    GRIS observations of the galactic center and the gamma ray galactic diffuse continuum (1992)
    In:  CASI
    Details
    Publication Date: 2013-08-31
    Description: On two flights in 1988, the Gamma-Ray Imaging Spectrometer (GRIS) discovered the galactic center in a high state (greater than 1 x 10(exp -3) ph/(sq cm sec)) of positron annihilation line emission (511 keV) after nearly a decade of failed attempts to confirm the exciting early results of balloon and satellite instruments. These two flights represented the first flights of a new generation of high resolution germanium spectrometers designed to achieve significantly greater sensitivity for astrophysical observations. During the fall flight, an observation of the galactic plane at 335 degrees longitude was also performed. This observation showed a very low level of 511 keV emission (2 +/- 1 x 10(exp -4) ph/(sq cm sec)), confirming the galactic center origin of the line, and a high level of hard x-ray and gamma-ray continuum emission (1 x 10(exp -4) ph/(sq cm sec keV) at 100 keV), which we attribute to galactic diffuse emission. Improved fits to the spectrum of the galactic center are presented with the proposed diffuse component subtracted. We conclude that our galactic center continuum spectrum is consistent with the sum of the 1E1740.7-2942 spectrum observed by SIGMA/GRANAT and our 1 = 335 degree galactic plane spectrum. The predicted diffuse flux should be easily measurable by the Oriented Scintillation Spectrometer Experiment (OSSE) experiment on the Gamma Ray Observatory (GRO).
    Keywords: SPACE RADIATION
    Type: The Compton Observatory Science Workshop; p 438-445
    Format: application/pdf
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