| Metadata Field | Value | Language |
| dc.creator | Jaret, Steven | |
| dc.creator | Woerner, William | |
| dc.creator | Phillips, Brian | |
| dc.creator | Ehm, Lars | |
| dc.creator | Nekvasil, Hanna | |
| dc.creator | Wright, Shawn | |
| dc.creator | Glotch, Timothy | |
| dc.date.accessioned | 2022-11-08T21:46:20Z | |
| dc.date.available | 2022-11-08T21:46:20Z | |
| dc.date.created | 2015 | |
| dc.identifier | 10.1002/2014JE004764 | en_US |
| dc.identifier.uri | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2014JE004764 | en_US |
| dc.identifier.uri | https://aurora.auburn.edu/handle/11200/50459 | |
| dc.identifier.uri | http://dx.doi.org/10.35099/aurora-527 | |
| dc.description.abstract | We present the results of a combined study of shocked labradorite from the Lonar crater, India, using optical microscopy, micro-Raman spectroscopy, nuclear magnetic resonance (NMR) spectroscopy, high-energy X-ray total scattering experiments, and micro-Fourier transform infrared (micro-FTIR) spectroscopy. We show that maskelynite of shock class 2 is structurally more similar to fused glass than to crystalline plagioclase. However, there are slight but significant differencespreservation of original preimpact igneous zoning, anisotropy at infrared wavelengths, X-ray anisotropy, and preservation of some intermediate range orderwhich are all consistent with a solid-state transformation from plagioclase to maskelynite. | en_US |
| dc.publisher | American Geophysical Union | en_US |
| dc.relation.ispartof | JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS | en_US |
| dc.relation.ispartofseries | 2169-9097 | en_US |
| dc.rights | ©American Geophysical Union 2015. This is this the version of record co-published by the American Geophysical Union and John Wiley & Sons, Inc. It is made available under the CC-BY-NC-ND 4.0 license. Item should be cited as: Jaret, S. J., Woerner, W. R., Phillips, B. L., Ehm, L., Nekvasil, H., Wright, S. P., & Glotch, T. D. (2015). Maskelynite formation via solid‐state transformation: Evidence of infrared and X‐ray anisotropy. Journal of Geophysical Research: Planets, 120(3), 570-587. | en_US |
| dc.title | Maskelynite formation via solid-state transformation: Evidence of infrared and X-ray anisotropy | en_US |
| dc.type | Text | en_US |
| dc.type.genre | Journal Article, Academic Journal | en_US |
| dc.citation.volume | 120 | en_US |
| dc.citation.issue | 3 | en_US |
| dc.citation.spage | 570 | en_US |
| dc.citation.epage | 587 | en_US |
| dc.description.status | Published | en_US |
| dc.description.peerreview | Yes | en_US |
| dc.creator.orcid | 0000-0001-5485-0316 | en_US |
| dc.creator.orcid | 0000-0003-1265-9470 | en_US |
| dc.creator.orcid | 0000-0001-8776-3235 | en_US |
