Observation of cosmic ray positrons from 5 to 25 GeV

Details Observation of cosmic ray positrons from 5 to 25 GeV Observation of cosmic ray positrons from 5 to 25 GeV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..374g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 374-377 (SEE N85-34006 22-93)

Computer Science

Cerenkov Radiation, Cosmic Rays, Magnetic Rigidity, Particle Density (Concentration), Particle Mass, Particle Trajectories, Positrons, Electron Photon Cascades, Phototubes, Radiant Flux Density, Scintillation Counters, Spectrometers

Scientific paper

The positron data gathered in conjunction with electron data published elsewhere is reported. The basic recognition scheme was to look for low mass positive particles that cause a cascade in a 7 radiation length shower counter. The mass criteria is imposed by selecting particles that were accompanied by Cherenkov light but whose rigidity was below the proton Cherenkov threshold. Thus the proton Cherenkov threshold represents an upper limit to the range of the experiment.

Affiliated with

Also associated with

No associations

Rating

Observation of cosmic ray positrons from 5 to 25 GeV 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 Observation of cosmic ray positrons from 5 to 25 GeV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observation of cosmic ray positrons from 5 to 25 GeV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-754732