Flux Variation of Cosmic Muons
Nepal Ramesh, Martin Hawron, Clayton Martin, Abdel Bachri

TL;DR
This study measured cosmic muon flux variations with elevation, temperature, and time, using a portable detector, and found flux increases with elevation but is unaffected by latitude or solar activity.
Contribution
It presents a portable cosmic muon detector setup and provides new empirical data on flux variation with elevation, temperature, and seasonal changes.
Findings
Muon flux increases with elevation
Flux is independent of latitude and solar activity
Flux is anti-correlated with temperature
Abstract
In the current paper, we analyzed the variation of cosmic radiation flux with elevation, time of the year and ambient temperature with the help of a portable cosmic muon detector, the construction of which was completed by a team from Southern Arkansas University (SAU) at Lawrence Berkeley National Laboratory (LBNL). Cosmic muons and gamma rays traverse two synchronized scintillators connected to two photomultiplier tubes (PMT) via light guides, and generate electronic pulses which we counted using a Data Acquisition Board (DAQ). Because muons are the product of collisions between high-energy cosmic rays and atmospheric nuclei, and therefore shower onto earth, the scintillators were arranged horizontally for detection. The elevation measurements were recorded at different locations, starting from 60 feet below sea-level at the Underground Radiation Counting Laboratory at Johnson Space…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Neutrino Physics Research
