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Title:Composition Measurements via Depth of Airshower Maximum at the Telescope Array
Authors:ID Lundquist, Jon Paul (Author)
ID Hanlon, W. (Author), et al.
Files:.pdf jpscp.19.011012.pdf (758,27 KB)
MD5: 17834B8D860E845D92BBBD038F3D3451
 
Language:English
Work type:Not categorized
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:Telescope Array (TA) was designed to answer important questions about the UHECR flux with energies above 10^17 eV such as spectrum, arrival direction, and mass composition. Because the UHECR flux is rapidly falling in this energy region, TA’s large exposure makes it one of the few experiments in the world that can adequately explore these issues. Composition is particularly difficult to measure because mass can not be measured directly due to the low flux. TA’s multiple methods of observing UHECR induced air showers will be explained, as well as how composition can be measured by these methods. Good agreement among the different measurement techniques is found leading to greater confidence in measuring UHECR mass composition and a way to test and understand TA systematic uncertainties.
Keywords:UHECR, cosmic rays, composition
Publication version:Version of Record
Year of publishing:2018
Number of pages:8
Numbering:19, 19
PID:20.500.12556/RUNG-5173-61e14343-014a-ec74-7c4f-1b91d457e117 New window
COBISS.SI-ID:13043203 New window
DOI:10.7566/JPSCP.19.011012 New window
NUK URN:URN:SI:UNG:REP:XCCLXB4A
Publication date in RUNG:29.04.2020
Views:2544
Downloads:103
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Record is a part of a proceedings

Title:Ultra HIgh Energy Cosmic Rays 2016

Record is a part of a journal

Title:JPS Conference Proceedings
Shortened title:JPS Conf. Proc.
Year of publishing:2018

Licences

License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.
Licensing start date:28.04.2020

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