Results from the Pierre Auger Observatory
The Pierre Auger Observatory is the largest observatory of high-energy cosmic rays. Are being tested the energy spectrum, mass composition and arrival directions of cosmic rays. New detection techniques, radio and microwave measurement presented here.
Подобные документы
- 1. Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
An investigation of the line profile variations (LPV) in spectra of hot stars. The smooth Time Variation Spectra (smTVS) for detection of micro LPV of various nature. Results of using the telescopes of the Caucasus Special Astrophysical Observatory.
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