Observation Capability of a Ground-Based Terahertz Radiometer for Vertical Profiles of Oxygen and Water Abundances in Martian Atmosphere
Observation Capability of a Ground-Based Terahertz Radiometer for Vertical Profiles of Oxygen and Water Abundances in Martian Atmosphere
复制标题
地基太赫兹辐射计对火星大气中氧气和水丰度垂直剖面的观测能力
DOI:
10.1109/tgrs.2022.3152271
复制
发表时间:
2022
影响因子:
8.2
通讯作者:
Kasai Yasuko
中科院分区:
文献类型:
--
作者:
Yamada Takayoshi;Baron Philippe;Neary Lori;Nishibori Toshiyuki;Larsson Richard;Kuroda Takeshi;Daerden Frank;Kasai Yasuko
We present the expected performance for a ground-based terahertz (THz) radiometer, a plan to be launched on the TERahertz EXplore-1 (TEREX-1) Mars exploration microspacecraft. The small THz passive radiometer has been developed for the TEREX series of future microspacecrafts. This spacecraft is an opportunity for organizations with limited resources and technology to conduct frequent missions to Mars well suited for resource exploration in contrast to all of the current and past Mars missions of large/giant class missions with fully government lead. The observation frequencies of the TEREX-1 radiometer are 474.64–475.64 and 486.64–487.64 GHz with a 100-kHz resolution, and the double-sideband noise temperature less than 3000 K. A theoretical error analysis is performed with the instrument characteristics to assess for the first time up-looking observations of atmospheric oxygen molecules (O2) and water vapor (H2O). Measurement errors for O2and H2O are 7%–22% and 14%–25% with 8–17- and 5–10-km vertical resolution in the vertical ranges 0–55 and 0–25 km, respectively. TEREX-1 is also capable to measure minor species, O3and H2O2, with a precision better than 30% within two independent layers. We used the integration time of 1 h for all simulations. Our theoretical simulation showed the instrument characteristics of the TEREX-1 sensor are able to observe vertical profiles of O2and H2O abundances with the same level of the large class missions.