Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond

Details Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203.....j&link_type=abstract

New York, American Institute of Physics (AIP Conference Proceedings, No. 203), 1990, 341 p. For individual items see A92-20527 t

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Conferences, Cosmic Rays, Nasa Space Programs, Earth Observing System (Eos), Energetic Particles, Galactic Cosmic Rays, Gamma Ray Observatory, Heliosphere, Mercury Flights, Mission Planning, Noaa Satellites, Radiation Detectors, Solar Flares, Space Missions, Space Probes, Spectrometers, Superconducting Magnets, Ulysses Mission

Scientific paper

Various papers on particle astrophysics are presented. Individual topics addressed include: the NASA cosmic ray (CR) program for the 1990s and beyond, SAMPEX Mission overview, the Advanced Composition Explorer, Positron Electron Magnet Spectrometer for the Eos Mission, Heavy Nucleus Collector for Space Station, the Astromag Facility, Large Isotope Spectrometer for Astromag, the Solar Probe Mission, the Mercury Dual Orbiter Mission, CRs in the heliosphere, origin of high-energy Galactic CRs, CR studies with the Gamma-Ray Observatory, gamma-ray astronomy at 1 TeV, experimental search for point sources above 1 TeV, the UMC Extensive Air Shower Array, status of the MACRO experiment. Also discussed are: CRs above 1 TeV/n and neutrino astronomy, abundance of ultraheavy nuclei in solar energetic particles, CR studies with an interstellar probe, isotopic composition of CR nuclei beyond the iron peak, experimental studies of CR isotopic composition up to Zr-40, use of accelerators in particle astrophysics, development of long-duration ballooning in Antarctica, Lunar-Based Heavy Nucleus Detector, neutrino astronomy on the moon, gamma rays at airplane altitudes, source composition of CRs.

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