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Cosmic and solar gamma-ray x-ray and particle measurements from high altitude balloons in Antarctica. [SN 1987a]

Conference · · AIP Conference Proceedings (American Institute of Physics); (USA)
OSTI ID:6701284
 [1]
  1. Space Sciences Laboratory, University of California, Berkeley, CA 94720 (USA)
For measurements of cosmic and solar gamma-rays, hard X-rays, and particles, Antarctica offers the potential for very long, 10--20 day, continuous, twenty-four-hour-a-day observations, with balloon flights circling the South Pole during austral summer. For X-ray/gamma-ray sources at high south latitude the overlying atmosphere is minimized, and for cosmic ray measurements the low geomagnetic cutoff permits entry of low rigidity particles. The first Antarctic flight of a heavy ({similar to}2400 lb.) payload on a large (11.6{times}10{sup 6} cu. ft.) balloon took place in January, 1988, to search for the gamma-ray lines of {sup 56}Co produced in the new supernova SN 1987A in the Large Magellanic Cloud. The long duration balloon flights presently planned from Antarctica include those for further gamma-ray/hard X-ray studies of SN 1987A and for the NASA Max '91 program for solar flare studies.
OSTI ID:
6701284
Report Number(s):
CONF-8906234--
Conference Information:
Journal Name: AIP Conference Proceedings (American Institute of Physics); (USA) Journal Volume: 198:1
Country of Publication:
United States
Language:
English