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The orbital TUS detector simulationстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 13 мая 2020 г.
- Авторы: Grinyuk A., Grebenyuk V., Khrenov B., Klimov P., Lavrova M., Panasyuk M., Sharakin S., Shirokov A., Tkachenko A., Tkachev L., Yashin I.
- Журнал: Astroparticle Physics
- Том: 90
- Год издания: 2017
- Издательство: Elsevier BV
- Местоположение издательства: Netherlands
- Первая страница: 93
- Последняя страница: 97
- DOI: 10.1016/j.astropartphys.2016.09.003
- Аннотация: The TUS space experiment is aimed at studying energy and arrival distribution of UHECR at E > 7 × 10^19 eV by using the data of EAS fluorescent radiation in atmosphere. The TUS mission was launched at the end of April 2016 on board the dedicated “Lomonosov” satellite. The TUSSIM software package has been developed to simulate performance of the TUS detector for the Fresnel mirror optical parameters, the light concentrator of the photo detector, the front end and trigger electronics. Trigger efficiency crucially depends on the background level which varies in a wide range: from 0.2 × 10^6 to 15 × 10^6 ph/(m^2μs sr) at moonless and full moon nights respectively. The TUSSIM algorithms are described and the expected TUS statistics is presented for 5 years of data collection from the 500 km solar-synchronized orbit with allowance for the variability of the background light intensity during the space flight.
- Добавил в систему: Климов Павел Александрович