Ariel 6 measurements of ultra-heavy cosmic ray fluxes in the region 34 or = Z or = 48

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Abundance, Cerenkov Radiation, Cosmic Rays, Galactic Radiation, Ariel Satellites, Cerenkov Counters, Particle Tracks, Photomultiplier Tubes, Scintillation Counters

Scientific paper

The Ariel VI satellite was launched by NASA on a Scout rocket on 3rd June 1979 from Wallops Island, Virginia, USA, into a near circular 625 km orbit inclined at 55 deg. It carried a spherical cosmic ray detector designed by a group from Bristol University. A spherical aluminum vessel of diameter 75 cm contains a gas scintillation mixture and a thin spherical shell of Pilot 425 plastic, and forms a single optical cavity viewed by 16 photomultipliers. Particle tracks through the detector may be characterized by their impact parameter p and by whether or not they pass through the cup of plastic scintillator placed between the sphere and the spacecraft body (referred to below as the Anti-Coincidence Detector or ACD). Individual particle charges are determined by separately measuring the gas scintillation and the Cerenkov emission from the plastic shell. This is possible because of the quite different distribution in time of these emissions.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Ariel 6 measurements of ultra-heavy cosmic ray fluxes in the region 34 or = Z or = 48 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ariel 6 measurements of ultra-heavy cosmic ray fluxes in the region 34 or = Z or = 48, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ariel 6 measurements of ultra-heavy cosmic ray fluxes in the region 34 or = Z or = 48 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-754420

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.