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Bow shock oscillations of Mars under weakly disturbed solar wind conditions.

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Title: Bow shock oscillations of Mars under weakly disturbed solar wind conditions.
Authors: Cheng L; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; Space Sciences Laboratory, University of California, Berkeley, CA, USA.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China., Wang Y; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn.; Hefei National Laboratory, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn., Ma Y; Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA., Lillis R; Space Sciences Laboratory, University of California, Berkeley, CA, USA., Halekas J; Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA., Langlais B; Nantes Université, Univ Angers, Le Mans Université, CNRS, Laboratoire de Planétologie et Géosciences, Nantes, France., Zhang T; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China., Zhang A; National Space Science Center, Chinese Academy of Sciences, Beijing, China.; University of Chinese Academy of Sciences, Beijing, China., Wang G; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China., Xiao S; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China., Zou Z; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China., Chi Y; Institute of Deep Space Sciences, Deep Space Exploration Laboratory, Hefei, China., Hao X; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China., Li Y; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China., Pan Z; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China., Liu K; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.
Source: Nature communications [Nat Commun] 2025 Oct 31; Vol. 16 (1), pp. 9649. Date of Electronic Publication: 2025 Oct 31.
Publication Type: Journal Article
Journal Info: Publisher: Nature Pub. Group Country of Publication: England NLM ID: 101528555 Publication Model: Electronic Cited Medium: Internet ISSN: 2041-1723 (Electronic) Linking ISSN: 20411723 NLM ISO Abbreviation: Nat Commun Subsets: MEDLINE; PubMed not MEDLINE
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  Data: Bow shock oscillations of Mars under weakly disturbed solar wind conditions.
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  Data: <searchLink fieldCode="AU" term="%22Cheng+L%22">Cheng L</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; Space Sciences Laboratory, University of California, Berkeley, CA, USA.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Wang+Y%22">Wang Y</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn.; Hefei National Laboratory, University of Science and Technology of China, Hefei, China. ymwang@ustc.edu.cn.<br /><searchLink fieldCode="AU" term="%22Ma+Y%22">Ma Y</searchLink>; Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA.<br /><searchLink fieldCode="AU" term="%22Lillis+R%22">Lillis R</searchLink>; Space Sciences Laboratory, University of California, Berkeley, CA, USA.<br /><searchLink fieldCode="AU" term="%22Halekas+J%22">Halekas J</searchLink>; Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA.<br /><searchLink fieldCode="AU" term="%22Langlais+B%22">Langlais B</searchLink>; Nantes Université, Univ Angers, Le Mans Université, CNRS, Laboratoire de Planétologie et Géosciences, Nantes, France.<br /><searchLink fieldCode="AU" term="%22Zhang+T%22">Zhang T</searchLink>; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China.<br /><searchLink fieldCode="AU" term="%22Zhang+A%22">Zhang A</searchLink>; National Space Science Center, Chinese Academy of Sciences, Beijing, China.; University of Chinese Academy of Sciences, Beijing, China.<br /><searchLink fieldCode="AU" term="%22Wang+G%22">Wang G</searchLink>; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China.<br /><searchLink fieldCode="AU" term="%22Xiao+S%22">Xiao S</searchLink>; Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, China.<br /><searchLink fieldCode="AU" term="%22Zou+Z%22">Zou Z</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Chi+Y%22">Chi Y</searchLink>; Institute of Deep Space Sciences, Deep Space Exploration Laboratory, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Hao+X%22">Hao X</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Li+Y%22">Li Y</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Pan+Z%22">Pan Z</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.<br /><searchLink fieldCode="AU" term="%22Liu+K%22">Liu K</searchLink>; National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China.; CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory, University of Science and Technology of China, Hefei, China.
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  Data: <searchLink fieldCode="JN" term="%22101528555%22">Nature communications</searchLink> [Nat Commun] 2025 Oct 31; Vol. 16 (1), pp. 9649. <i>Date of Electronic Publication: </i>2025 Oct 31.
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