The TIRVIM Fourier Spectrometer for Studying the Martian Atmosphere


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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).

作者简介

B. Moshkin

Space Research Institute

编辑信件的主要联系方式.
Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117997

A. Grigor’ev

Space Research Institute

Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117997

A. Shakun

Space Research Institute

Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117997

D. Patsaev

Space Research Institute

Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117997

A. Zharkov

Space Research Institute

Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117997

V. Vagin

Scientific and Technological Center of Unique Instrumentation

Email: bmoha@yandex.ru
俄罗斯联邦, Moscow, 117342

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