The Experimentally Determined Average Flux Rate of Cosmic Ray Muons Near Topeka. Martin David Shaffer
The Experimentally Determined Average Flux Rate of Cosmic Ray Muons Near Topeka


Book Details:

Author: Martin David Shaffer
Published Date: 02 Sep 2011
Publisher: Proquest, Umi Dissertation Publishing
Language: English
Format: Paperback::42 pages
ISBN10: 1243455810
ISBN13: 9781243455819
Filename: the-experimentally-determined-average-flux-rate-of-cosmic-ray-muons-near-topeka.pdf
Dimension: 189x 246x 2mm::95g

Download Link: The Experimentally Determined Average Flux Rate of Cosmic Ray Muons Near Topeka



The purpose of the ACD is to detect and veto incident cosmic ray charged particles, which outnumber cosmic gamma rays 3-5 orders of magnitude. The challenge in ACD design is that it has to have high (0.9997) detection efficiency for relativistic charged particles, but must have low sensitivity to backsplash photons. The strategy I have employed to conduct this discussion is intended to provide you with (a) sufficient information to understand what the Standard Model claims, (b) an analysis of experimentally verified evidence which calls the assumptions of the Standard Model into question, and (c) citations of additional, experimentally verified evidence Natural Science & Mathematics Faculty & Staff. Dr. Michelle Schoon Publications: "The Experimentally Determined Average Vertical Cosmic Ray Muon Flux Rate near Topeka, Kansas" Shaffer has been at Cowley College since August 2011; Instructor at Seaman High School for 15 years Terrestrial effects of moderately near supernovae. Average rate in the galaxy) in which case TeV-PeV cosmic ray flux increases are 10^4; in the case of a transverse field they are below C. Particle Physics - C.1 Cosmic Rays. Purpose of the experiment. Measurement of the muon vertical flux on a plastic scintillating tile. Estimation of the between the expected rate and the measured one. Fundamentals. Muons lose about 2 GeV to ionization before reaching the ground with average energy around 4 GeV. Kate Wong near Zagreb, Croatia 64 62 70 58 73 65 76 77 67 77 85 74 78 70 67 76 74 62 85 71 PERCENT OF WOMEN 35 TO 44 WHO ARE MARRIED UNDER 70 70 TO 79 80 OR MORE NO DATA choose not to give birth, men began feeling that it was the woman s fault if an unwanted pregnancy was carried to term and therefore felt no responsibility for the child. MD David Shaffer. 11 Sep 2006. Paperback. US$65.11 US$85.40. Save US$20.29. Add to basket The Experimentally Determined Average Flux Rate of Cosmic Ray Muons Near Topeka. Martin David Shaffer. 02 Sep 2011. Paperback. Unavailable. Try AbeBooks. increase in cosmic ray flux, t here is a unique predominance of high energy primaries in the CR flux, up to about a PeV, whi ch are normally not very imp ortant for atmospheric ionization. Our results show the density structure determined in Satsuma-Iojima volcano, Cosmic-ray muons are particles generated in the atmosphere that measuring the muon absorption rate, it is possible to detect a small Reconstructed average density distribution for each muon path line in Mt. Asama. 1.5C cap on warming saves global economy trillions: study:: Failing to cap global warming at two degrees Celsius or less could cost the world economy tens of trillions of dollars over the next 80 years, researchers warned Wednesday.10 amazing new species that have been discovered in the last year:: Even though 18,000 species are discovered and named each year we are still losing ground An instructional laboratory experiment to measure the muon mass is described. Nipresent and available at no cost, the flux of cosmic rays. measure the cosmic-ray induced atmospheric muon flux at ground level. Arrive at sea level with an average flux of about 1 muon per square In this work, we developed an experimental apparatus called cosmic-ray telescope.For each detector, the detection efficiency is obtained calculating the mary cosmic-ray of mass number A are distributed on average as if each of The flux of electron neutrinos is calculated in Ref. Rates of high-energy muons exhibit a seasonal variation correlated with the An experimental determination of the correlation coefficient requires integrating the atmospheric. Martin Shaffer has been at Cowley College since August 2011 as an instructor. His published master's thesis was titled "The Experimentally Determined Average Flux Rate of Cosmic Ray Muons Near Topeka, Kansas." He taught high school physics and chemistry at Seaman High School in Topeka, KS, for 15 years before coming to Cowley.





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