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Автор P M Chadwick
Автор K Lyons
Автор T J L McComb
Автор K J Orford
Автор J L Osborne
Автор S M Rayner
Автор I D Roberts
Автор S E Shaw
Автор K E Turver
Дата выпуска 1999-06-01
dc.description Atmospheric Cerenkov telescopes are used to detect electromagnetic showers from primary -rays of energy ~300 GeV up to 10 TeV and to discriminate these from cascades due to hadrons using the Cerenkov images. The geomagnetic field affects the development of showers and is shown to diffuse and distort the images. When the component of the field normal to the shower axis is sufficiently large (>0.4 G) the performance of -ray telescopes may be affected, although corrections should be possible.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Geomagnetic effects on atmospheric Cerenkov images
Тип paper
DOI 10.1088/0954-3899/25/6/312
Electronic ISSN 1361-6471
Print ISSN 0954-3899
Журнал Journal of Physics G: Nuclear and Particle Physics
Том 25
Первая страница 1223
Последняя страница 1233
Аффилиация P M Chadwick; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация K Lyons; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация T J L McComb; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация K J Orford; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация J L Osborne; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация S M Rayner; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация I D Roberts; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация S E Shaw; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
Аффилиация K E Turver; Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham DH1 3LE, UK
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