Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986izssr..50.2129b&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Tbilisi, Georgian SSR, Apr. 1986) Akademiia Nauk SSSR, Izvestiia, Seriia Fiz
Astronomy and Astrophysics
Astronomy
Elementary Particle Interactions, Gamma Ray Astronomy, Hadrons, X Ray Analysis, Electron Density (Concentration), Halos, Test Chambers
Scientific paper
The Sitora gamma-hadron superfamily was recorded with the Pamir-77/78 carbon X-ray emulsion chamber. The total recorded energy of Sitora was (1.5-2) x 10 to the 4th TeV, while the primary particle energy was 7 x 10 to the 16th eV. Scans of the superfamily at three depths in the chamber are presented, and the dependence of the electron density on the halo radius at three depths the chamber is plotted.
Borisov Anatoly S.
Denisova G. V.
Dunaevskii A. M.
Guseva M. Z.
Zhdanov B. G.
No associations
LandOfFree
Certain characteristics of the Sitora superfamily 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 Certain characteristics of the Sitora superfamily, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Certain characteristics of the Sitora superfamily will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1150408