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Автор G K Garipov
Автор B A Khrenov
Дата выпуска 1994-12-01
dc.description A new instrument, a camera obscura with a number of light apertures (or slits), is suggested for observation of EAS images in Cerenkov light. Its advantages (over mirror-imaging telescopes) are a low night-sky light noise, a wide field of view and absence of aberrations. This camera is effective for measurements of bright objects such as EAS of energies higher than 10<sup>3</sup> TeV. Analysis of EAS images in the 'knee' region of the primary cosmic-ray energy spectrum (E<sub>0</sub> approximately=3*10<sup>3</sup> TeV) could give new information on the expected variation of cosmic-ray composition in this energy region.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Camera obscura for observation of EAS in Cerenkov light
Тип paper
DOI 10.1088/0954-3899/20/12/013
Electronic ISSN 1361-6471
Print ISSN 0954-3899
Журнал Journal of Physics G: Nuclear and Particle Physics
Том 20
Первая страница 1981
Последняя страница 1988
Аффилиация G K Garipov; Inst. of Nucl. Phys., Moscow State Univ., Russia
Аффилиация B A Khrenov; Inst. of Nucl. Phys., Moscow State Univ., Russia
Выпуск 12

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