TY - JOUR
T1 - Observation Capability of a Ground-Based Terahertz Radiometer for Vertical Profiles of Oxygen and Water Abundances in Martian Atmosphere
AU - Yamada, Takayoshi
AU - Baron, Philippe
AU - Neary, Lori
AU - Nishibori, Toshiyuki
AU - Larsson, Richard
AU - Kuroda, Takeshi
AU - Daerden, Frank
AU - Kasai, Yasuko
N1 - Publisher Copyright:
© 1980-2012 IEEE.
PY - 2022
Y1 - 2022
N2 - 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 O2 and 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, O3 and 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 O2 and H2O abundances with the same level of the large class missions.
AB - 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 O2 and 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, O3 and 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 O2 and H2O abundances with the same level of the large class missions.
KW - Atmospheric observation
KW - Mars
KW - error analysis
KW - lander
KW - terahertz (THz)
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U2 - 10.1109/TGRS.2022.3152271
DO - 10.1109/TGRS.2022.3152271
M3 - Article
AN - SCOPUS:85124822311
SN - 0196-2892
VL - 60
JO - IEEE Transactions on Geoscience and Remote Sensing
JF - IEEE Transactions on Geoscience and Remote Sensing
M1 - 4106311
ER -