{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,2,13]],"date-time":"2026-02-13T16:38:39Z","timestamp":1771000719452,"version":"3.50.1"},"reference-count":72,"publisher":"MDPI AG","issue":"2","license":[{"start":{"date-parts":[[2024,1,11]],"date-time":"2024-01-11T00:00:00Z","timestamp":1704931200000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"DOI":"10.13039\/501100006769","name":"Russian Science Foundation","doi-asserted-by":"publisher","award":["23-72-01009"],"award-info":[{"award-number":["23-72-01009"]}],"id":[{"id":"10.13039\/501100006769","id-type":"DOI","asserted-by":"publisher"}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Remote Sensing"],"abstract":"<jats:p>Monitoring excited hydroxyl (OH*) airglow is broadly used for characterizing the state and dynamics of the terrestrial atmosphere. Recently, the existence of excited hydroxyl was confirmed using satellite observations in the Martian atmosphere. The location and timing of its detection on Mars were restricted to a winter season at the north pole. We present three-dimensional global simulations of excited hydroxyl over a Martian year. The predicted spatio-temporal distribution of the OH* can provide guidance for future observations, namely by indicating where and when the airglow is likely to be detected.<\/jats:p>","DOI":"10.3390\/rs16020291","type":"journal-article","created":{"date-parts":[[2024,1,11]],"date-time":"2024-01-11T03:21:41Z","timestamp":1704943301000},"page":"291","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":2,"title":["Morphology of the Excited Hydroxyl in the Martian Atmosphere: A Model Study\u2014Where to Search for Airglow on Mars?"],"prefix":"10.3390","volume":"16","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-2893-9082","authenticated-orcid":false,"given":"Dmitry S.","family":"Shaposhnikov","sequence":"first","affiliation":[{"name":"Laboratory of Operational Satellite Monitoring, Moscow Institute of Physics and Technology, 141707 Moscow, Russia"},{"name":"Space Research Institute of the Russian Academy of Sciences, 117485 Moscow, Russia"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-6702-3587","authenticated-orcid":false,"given":"Mykhaylo","family":"Grygalashvyly","sequence":"additional","affiliation":[{"name":"Max Planck Institute for Solar System Research, 37077 G\u00f6ttingen, Germany"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-2713-8977","authenticated-orcid":false,"given":"Alexander S.","family":"Medvedev","sequence":"additional","affiliation":[{"name":"Max Planck Institute for Solar System Research, 37077 G\u00f6ttingen, Germany"}]},{"given":"Gerd Reinhold","family":"Sonnemann","sequence":"additional","affiliation":[{"name":"Max Planck Institute for Solar System Research, 37077 G\u00f6ttingen, Germany"}]},{"given":"Paul","family":"Hartogh","sequence":"additional","affiliation":[{"name":"Max Planck Institute for Solar System Research, 37077 G\u00f6ttingen, Germany"}]}],"member":"1968","published-online":{"date-parts":[[2024,1,11]]},"reference":[{"key":"ref_1","unstructured":"Chamberlain, J.W. 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