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dc.contributor.authorYeşiltaş, Mehmet
dc.contributor.authorJaret, Steven
dc.contributor.authorYoung, Jordan
dc.contributor.authorWright, Shawn P.
dc.contributor.authorGlotch, Timothy D.
dc.date.accessioned2021-12-12T17:02:09Z
dc.date.available2021-12-12T17:02:09Z
dc.date.issued2018
dc.identifier.issn2333-5084
dc.identifier.urihttps://doi.org/10.1029/2018EA000369
dc.identifier.urihttps://hdl.handle.net/20.500.11857/3392
dc.description.abstractChemical constituents and their spatial distributions in terrestrial and extraterrestrial samples may provide clues to their formation histories and secondary processes they were subjected to. Most analytical tools are either limited in imaging the interior of samples or they are destructive such that the sample is chemically modified. In this work, we have conducted three-dimensional Raman tomographic imaging experiments on both terrestrial and extraterrestrial samples. The in situ nondestructive analytical technique presented here provides spatial distribution of various chemical constituents from the interior of the samples with high spatial and depth resolution. Raman data were first collected from two-dimensional layers at the surface and at various depths inside the samples by means of confocal Raman imaging. Individual chemical distribution maps were generated for each layer, which were then stacked to form and visualize the three-dimensional distributions. In addition to three-dimensional distributions, Raman spectral information was also collected from each pixel within the measured areas, thus allowing us to also perform detailed spectral investigations of the samples.en_US
dc.description.sponsorshipRIS4E node of NASA's Solar System Exploration Research Virtual Institute (SSERVI)en_US
dc.description.sponsorshipWe are grateful to NASA's Meteorite Working Group for the meteorite sample from the Antarctic meteorite collection, John Luczaj for the pyrite, Sidney Hemming and Troy Rasbury for the rutile, and Martin Schoonen and Hiroshi Ohmoto (Emeritus at Penn State) for the BIF sample. We thank reviewers and the Editor for their constructive comments. We also wish to thank Volkan Eskizeybek and Arife Aktas (Science and Technology Application and Research Center of Canakkale Onsekiz Mart University, Turkey) for their support during the Raman data collection. This work is funded by the RIS<SUP>4</SUP>E node of NASA's Solar System Exploration Research Virtual Institute (SSERVI; PI: T. D. Glotch). The data presented here will be made publicly available via Turkish Spectral Database at http://tsd.klu.edu.tr/.en_US
dc.language.isoengen_US
dc.publisherAmer Geophysical Unionen_US
dc.relation.ispartofEarth and Space Scienceen_US
dc.identifier.doi10.1029/2018EA000369
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectRaman microspectroscopyen_US
dc.subjectmeteoritesen_US
dc.subjectmineralsen_US
dc.subjecttomographyen_US
dc.subjectthree-dimensionalen_US
dc.subjectimagingen_US
dc.titleThree-Dimensional Raman Tomographic Microspectroscopy: A Novel Imaging Techniqueen_US
dc.typearticle
dc.authoridYesiltas, Mehmet/0000-0002-1521-0460
dc.authoridJaret, Steven/0000-0003-1265-9470
dc.authoridWright, Shawn/0000-0001-8776-3235
dc.departmentFakülteler, Lüleburgaz Havacılık ve Uzay Bilimleri Fakültesi, Havacılık ve Uzay Mühendisliği Bölümü
dc.identifier.volume5en_US
dc.identifier.startpage380en_US
dc.identifier.issue8en_US
dc.identifier.endpage392en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.authorscopusid23020484700
dc.authorscopusid56190571100
dc.authorscopusid57203532117
dc.authorscopusid12647543900
dc.authorscopusid6507290607
dc.identifier.wosWOS:000443994000005en_US
dc.identifier.scopus2-s2.0-85052382596en_US
dc.authorwosidYesiltas, Mehmet/G-3735-2013


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