The TIRVIM Fourier Spectrometer for Studying the Martian Atmosphere
- Авторы: Moshkin B.E.1, Grigor’ev A.V.1, Shakun A.V.1, Patsaev D.V.1, Zharkov A.V.1, Vagin V.A.2
-
Учреждения:
- Space Research Institute
- Scientific and Technological Center of Unique Instrumentation
- Выпуск: Том 61, № 1 (2018)
- Страницы: 130-135
- Раздел: Physical Instruments for Ecology, Medicine, and Biology
- URL: https://ogarev-online.ru/0020-4412/article/view/160031
- DOI: https://doi.org/10.1134/S0020441217060070
- ID: 160031
Цитировать
Аннотация
The design and performance features of an IR Fourier-transform spectrometer for studying the Martial atmosphere in the spectrum range of 600–5500 cm–1 during the ExoMars-2016 mission are described. The obtained spectral resolution is in agreement with the theoretical value (0.2 cm–1); the threshold of the instrument sensitivity is approximately 0.1 mW/(m2 sr cm–1).
Об авторах
B. Moshkin
Space Research Institute
Автор, ответственный за переписку.
Email: bmoha@yandex.ru
Россия, Moscow, 117997
A. Grigor’ev
Space Research Institute
Email: bmoha@yandex.ru
Россия, Moscow, 117997
A. Shakun
Space Research Institute
Email: bmoha@yandex.ru
Россия, Moscow, 117997
D. Patsaev
Space Research Institute
Email: bmoha@yandex.ru
Россия, Moscow, 117997
A. Zharkov
Space Research Institute
Email: bmoha@yandex.ru
Россия, Moscow, 117997
V. Vagin
Scientific and Technological Center of Unique Instrumentation
Email: bmoha@yandex.ru
Россия, Moscow, 117342
Дополнительные файлы
