دورية أكاديمية

Formation of lunar swirls by magnetic field standoff of the solar wind.

التفاصيل البيبلوغرافية
العنوان: Formation of lunar swirls by magnetic field standoff of the solar wind.
المؤلفون: Glotch TD; Department of Geosciences, Stony Brook University, Stony Brook, New York 11794-2100, USA., Bandfield JL; Space Science Institute, 4750 Walnut St #205, Boulder, Colorado 80301, USA., Lucey PG; Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, Hawaii 96822, USA., Hayne PO; Jet Propulsion Laboratory, M/S 183-301, 4800 Oak Grove Drive, Pasadena, California 91109, USA., Greenhagen BT; Jet Propulsion Laboratory, M/S 183-301, 4800 Oak Grove Drive, Pasadena, California 91109, USA., Arnold JA; Department of Geosciences, Stony Brook University, Stony Brook, New York 11794-2100, USA., Ghent RR; Department of Earth Sciences, University of Toronto, Toronto, Ontario, Canada M5S 3B1., Paige DA; University of California Los Angeles, Box 951567, Los Angeles, California 90095-1567, USA.
المصدر: Nature communications [Nat Commun] 2015 Feb 04; Vol. 6, pp. 6189. Date of Electronic Publication: 2015 Feb 04.
نوع المنشور: Journal Article; Research Support, Non-U.S. Gov't
اللغة: English
بيانات الدورية: 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: PubMed not MEDLINE
أسماء مطبوعة: Original Publication: [London] : Nature Pub. Group
مستخلص: Lunar swirls are high-albedo markings on the Moon that occur in both mare and highland terrains; their origin remains a point of contention. Here, we use data from the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer to support the hypothesis that the swirls are formed as a result of deflection of the solar wind by local magnetic fields. Thermal infrared data from this instrument display an anomaly in the position of the silicate Christiansen Feature consistent with reduced space weathering. These data also show that swirl regions are not thermophysically anomalous, which strongly constrains their formation mechanism. The results of this study indicate that either solar wind sputtering and implantation are more important than micrometeoroid bombardment in the space-weathering process, or that micrometeoroid bombardment is a necessary but not sufficient process in space weathering, which occurs on airless bodies throughout the solar system.
تواريخ الأحداث: Date Created: 20150205 Date Completed: 20150706 Latest Revision: 20150204
رمز التحديث: 20240628
DOI: 10.1038/ncomms7189
PMID: 25650225
قاعدة البيانات: MEDLINE
الوصف
تدمد:2041-1723
DOI:10.1038/ncomms7189