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Remote Sensing of the Atmosphere by the Ultraviolet Detector TUS Onboard the Lomonosov Satelliteстатья
Статья опубликована в высокорейтинговом журнале
Статья опубликована в журнале из списка Web of Science и/или Scopus- Авторы: Klimov Pavel, Khrenov Boris, Kaznacheeva Margarita, Garipov Gali, Panasyuk Mikhail, Petrov Vasily, Sharakin Sergei, Shirokov Andrei, Yashin Ivan, Zotov Mikhail, Grebenyuk Viktor, Grinyuk Andrei, Lavrova Maria, Tkachenko Artur, Tkachev Leonid, Botvinko Alla, Saprykin Oleg, Puchkov Andrei, Senkovsky Alexander
- Журнал: Remote Sensing
- Том: 11
- Номер: 20
- Год издания: 2019
- Издательство: MDPI
- Местоположение издательства: Basel, Switzerland
- DOI: 10.3390/rs11202449
- Аннотация: The orbital detector TUS (Tracking Ultraviolet Setup) with high sensitivity in near-visible ultraviolet (tens of photons per time sample of 0.8 μ s of wavelengths 300–400 nm from a detector’s pixel field of view) and the microsecond-scale temporal resolution was developed by the Lomonosov-UHECR/TLE collaboration and launched into orbit on 28 April 2016. A variety of different phenomena were studied by measuring ultraviolet signals from the atmosphere: extensive air showers from ultra-high-energy cosmic rays, lightning discharges, transient atmospheric events, aurora ovals, and meteors. These events are different in their origin and in their duration and luminosity. The TUS detector had a capability to conduct measurements with different temporal resolutions (0.8 μ s, 25.6 μ s, 0.4 ms, and 6.6 ms) but the same spatial resolution of 5 km. Results of the TUS detector measurements of various atmospheric emissions are discussed and compared to data from previous experiments.
- Добавил в систему: Климов Павел Александрович