EAS Arrays at High Altitudes Start the Era of UHE <i>γ</i>-ray Astronomy
The evolution of extensive air shower detection as a technique for <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>γ</mi></semantics></math></inline-formula>-ray astronomical instrume...
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פורמט: | Article |
שפה: | English |
יצא לאור: |
MDPI AG
2021-09-01
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סדרה: | Universe |
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גישה מקוונת: | https://www.mdpi.com/2218-1997/7/9/339 |
סיכום: | The evolution of extensive air shower detection as a technique for <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>γ</mi></semantics></math></inline-formula>-ray astronomical instrumentation for the last three decades is reviewed. The first discoveries of galactic PeVatrons by the Large High Altitude Air Shower Observatory demonstrate the importance of this technique in ultra-high energy <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>γ</mi></semantics></math></inline-formula>-ray astronomy. Utilizing this technique, the origins of high energy cosmic rays may be discovered in the near future. |
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ISSN: | 2218-1997 |