Shining a light on planetary processes using synchrotron powder diffraction

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dc.contributor.authorBrand, HEAen_AU
dc.contributor.authorKimpton, JAen_AU
dc.contributor.authorGu, QFen_AU
dc.date.accessioned2021-10-21T00:20:13Zen_AU
dc.date.available2021-10-21T00:20:13Zen_AU
dc.date.issued2016-03-24en_AU
dc.date.statistics2021-10-14en_AU
dc.description.abstractIntroduction: The Australian Synchrotron is powerful source of electromagnetic radiation that produces photon energies up to 3 GeV. The powder diffraction (PD) beamline at the Australian synchrotron produces bright, highly-collimated X-ray beams that, when combined with the state-of-the-art MYTHEN II microstrip detector, are ideal for time-resolved X-ray powder diffraction experiments requiring rapid, high resolution data collection. In addition, the powder diffraction beamline exploits the unique properties of synchrotron radiation to offer tunable wavelengths (6 - 30 keV, 2.07 - 0.41 Å) to minimise sample absorption and fluorescence, provide high flux and good S/N for increased detection limits. Since beginning user operations in 2008, 490 user experiments have been performed at the powder diffraction beamline. This contribution describes and demonstrates the capabilities offered by the beamline, particularly for planetary sciences and geosciences applications, highlighting the unique in-situ experiments that have not only produced successful scientific outcomes, but have pushed the boundaries in many cases.en_AU
dc.identifier.citationBrand, H. E. A., Kimpton, J. A. & Gu, Q. (2016). Shining a light on planetary processes using synchrotron powder diffraction. Poster presented at the 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA, March 21-25 2016. (No. 1903, pp. 1121). Retrieved from: https://www.hou.usra.edu/meetings/lpsc2016/programAbstracts/view/en_AU
dc.identifier.conferenceenddate25 March 2016en_AU
dc.identifier.conferencename47th Lunar and Planetary Science Conferenceen_AU
dc.identifier.conferenceplaceTexas, USAen_AU
dc.identifier.conferencestartdate21 March 2016en_AU
dc.identifier.otherNo. 1930en_AU
dc.identifier.pagination1121en_AU
dc.identifier.urihttps://www.hou.usra.edu/meetings/lpsc2016/programAbstracts/view/en_AU
dc.identifier.urihttps://apo.ansto.gov.au/dspace/handle/10238/12023en_AU
dc.language.isoenen_AU
dc.publisherUniversities Space Research Associationen_AU
dc.subjectX-ray diffractionen_AU
dc.subjectElectromagnetic radiationen_AU
dc.subjectSynchrotron radiationen_AU
dc.subjectSynchrotronsen_AU
dc.subjectWavelengthsen_AU
dc.subjectFluorescenceen_AU
dc.subjectANSTOen_AU
dc.titleShining a light on planetary processes using synchrotron powder diffractionen_AU
dc.typeConference Posteren_AU
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