Download presentation
Presentation is loading. Please wait.
Published byAvis Roberts Modified over 8 years ago
1
Victor Hess in his balloon (1912)
2
Cosmic Rays Produce Muons in the Atmosphere.
4
Types of Cosmic Ray Detectors Scintillator, Water, Array
5
Cosmic Ray Detectors Around the World Pierre Auger, Haverah Park, SPASE, Quarknet
6
RadiationEnergy Photon of light Can be detected by your eye 1 eV Ultra Violet ray from sun Enough to burn your skin 10 eV X-Ray Can pass right through your body 1000 eV = 1 keV Gamma ray detected by the Whipple group's telescopeWhipple group's telescope 10 12 eV = 1 TeV Cosmic Ray detected by the SPASE-2 experimentSPASE-2 10 15 eV = 1 PeV Cosmic Ray detected by the planned Pierre Auger Observatory Pierre Auger Observatory 10 20 eV = 100 EeV Highest energy Cosmic Ray ever recorded 3x10 20 eV This is the amount of energy that you would feel if you dropped a bowling ball on your foot from a height of 1 metre!
7
Primary Cosmic Ray Particle Types 1.Charged particles such as protons or helium nuclei 2.Uncharged particles such as photons
8
Are Active Galactic Nuclei a Source of the Highest Energy Cosmic Rays? (NGC 4261)
9
The Quarknet Scintillation Detector
10
Finding the Muon Lifetime
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.