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Considering the current absence of such an Interferometer, this paper introduces a novel Mars wind field imaging interferometer. In analyzing the photochemical model of O2 (a1\u0394g) 1.27 \u03bcm molecular airglow radiation in the Martian atmosphere and considering the impact of instrument signal-to-noise ratio (SNR), we have chosen an optical path difference (OPD) of 8.6 cm for the interferometer. The all-solid-state polarized wind imaging interferometer is miniaturized by incorporating two arm glasses as the compensation medium in its construction, achieving the effects of field-widening and temperature compensation. Additionally, an F-P Etalon is designed to selectively filter the desired three spectral lines of O2 dayglow, and its effect is evaluated through simulations. The accuracy of the proposed compact Mars polarized wind imaging interferometer for detecting Mars\u2019 wind field and temperature field has been validated through rigorous theoretical derivation and comprehensive computer simulations. The interferometer boasts several advantages, including its compact and small size, static stability, minimal stray light, and absence of moving parts. It establishes the theoretical, technological, and instrumental engineering foundations for future simultaneous static measurement of Martian global atmospheric wind fields, temperature fields, and ozone concentrations from spacecraft, thereby significantly contributing to the dataset for investigating Martian atmospheric dynamics.<\/jats:p>","DOI":"10.3390\/rs15194881","type":"journal-article","created":{"date-parts":[[2023,10,9]],"date-time":"2023-10-09T05:07:13Z","timestamp":1696828033000},"page":"4881","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":3,"title":["Novel Compact Polarized Martian Wind Imaging Interferometer"],"prefix":"10.3390","volume":"15","author":[{"given":"Chunmin","family":"Zhang","sequence":"first","affiliation":[{"name":"School of Physics, Xi\u2019an Jiaotong Univisity, Xi\u2019an 710049, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-4192-634X","authenticated-orcid":false,"given":"Yanqiang","family":"Wang","sequence":"additional","affiliation":[{"name":"School of Physics, Xi\u2019an Jiaotong Univisity, Xi\u2019an 710049, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Biyun","family":"Zhang","sequence":"additional","affiliation":[{"name":"Pricewaterhouse Coopers (PwC), Xi\u2019an 710054, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Tingyu","family":"Yan","sequence":"additional","affiliation":[{"name":"College of Electronic Engineering, Chengdu University of Information Technology, Chengdu 610225, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Zeyu","family":"Chen","sequence":"additional","affiliation":[{"name":"School of Physics, Xi\u2019an Jiaotong Univisity, Xi\u2019an 710049, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Zhengyi","family":"Chen","sequence":"additional","affiliation":[{"name":"School of Physics, Xi\u2019an Jiaotong Univisity, Xi\u2019an 710049, China"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"1968","published-online":{"date-parts":[[2023,10,9]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"2027","DOI":"10.1007\/s11430-020-9814-7","article-title":"Measurement of Martian atmospheric winds by the O2 1.27 \u03bcm airglow observations using Doppler Michelson Interferometry: A concept study","volume":"64","author":"Yang","year":"2021","journal-title":"Sci. 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