Four-Polarisation Camera for Anisotropy Mapping at Three Orientations: Micro-Grain of Olivine
Authors:
- Shuji KamegakiShuji Kamegaki
- Daniel SmithDaniel Smith
- Meguya RyuMeguya Ryu
- Soon Hock NgSoon Hock Ng
- Hsin-Hui HuangHsin-Hui Huang
- Pegah MaasoumiPegah Maasoumi
- Jitraporn VongsvivutJitraporn Vongsvivut
- Daniel MoraruDaniel Moraru
- Tomas KatkusTomas Katkus
- Saulius JuodkazisSaulius Juodkazis
- Junko MorikawaJunko Morikawa
Open Access
Abstract
A four-polarisation camera was used to map the absorbance of olivine micro-grains before and after high-temperature annealing (HTA). It is shown that HTA of olivine xenoliths at above 1200 C in O2 flow makes them magnetised. Different modes of operation of the polariscope with polarisation control before and after the sample in transmission and reflection modes were used. The reflection type was assembled for non-transparent samples of olivine after HTA. The sample for optical observation in transmission was placed on an achromatic, plastic, quarter-wavelength waveplate as a sample holder. Inspection of the sample’s birefringence (retardance), as well as absorbance, was undertaken. The best fit for the transmitted intensity or transmittance T (hence, absorbance ) is obtainable using a simple best fit with only three orientations (from the four orientations measured by the camera). When the intensity of transmitted light at one of the orientations is very low due to a cross-polarised condition (polariser–analyser arrangement), the three-point fit can be used. The three-point fit in transmission and reflection modes was validated for , where the amplitude , offset , and orientation azimuth were extracted for each pixel via the best fit.
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Funding Information
- Australian Research Council (LP190100505, 22K14200, 22H02137, JPMJCR19I3, M18753)
- Japan Society for the Promotion of Science (LP190100505, 22K14200, 22H02137, JPMJCR19I3, M18753)
- Japan Science and Technology Corporation (LP190100505, 22K14200, 22H02137, JPMJCR19I3, M18753)
- Infrared Microspectroscopy (IRM) beamline at the Australian Synchrotron (LP190100505, 22K14200, 22H02137, JPMJCR19I3, M18753)
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