The Oxford Instruments NanoAnaylsis Scientific Paper Award 2024 has been presented to scientists from the UK, South Korea and America for their work. The award recognises the exceptional, cutting-edge research published in peer-reviewed journals in 2023 that included data and results acquired with Oxford Instruments EBSD, EDS, WDS detectors or OmniProbe nanomanipulators.
“I was really pleased to see the sheer number, range and quality of papers submitted for this our second year of the Oxford Instruments NanoAnalysis Scientific Paper Awards,” said Dr Matt Hiscock, Head of Product Science at Oxford Instruments and chief judge. "We certainly had a difficult task to select the winners from such tough competition. I would like to thank everyone who took time to submit a paper entry. This competition clearly highlights the cutting-edge work that is being carried out across a wide range of applications."
“We look forward to reading and judging the entries for next year's Oxford Instruments Scientific Paper Awards".
In this research, Fazlollah Sadeghi and his colleagues Tahereh Zargar, Sang Hoon Kim, Yoon-Uk Heo, Jae Sang Lee, Chang Hee Yim, aimed to investigate the evolution of centerline carbides in a continuously cast martensitic stainless steel after applying a homogenization heat treatment. Due to the segregation of alloying elements into the final melt during solidification, a complex structure of carbide’s network is formed at the final melt. They were able to locate, identify, characterize, and post-process various types of carbides including orthorhombic M7C3, cubic M23C6, and cubic M6C via advanced characterization techniques attached to the scanning and transmission electron microscope such as EDS, WDS, and EBSD provided by Oxford Instruments. Results have shown a decomposition of Cr7C3
to Cr23C6 and formation of Mo6C at the interface with a specific orientation relationship. The microstructure of the centerline segregation consists of retained g-austenite, residual d-ferrite and carbide structures surrounded by α-martensite matrix.
The palaeognath birds’ phylogeny has been recently revised significantly due to the advancement of genomics, providing an opportunity to trace the evolution of modern dinosaur (bird) eggshells.
In this study, Sheng Fen and his colleagues Seung Choi, Mark E Hauber, Lucas J Legendre, Noe-Heon Kim, Yuong-Nam Lee, David J Varricchio, eggshells of all major clades of Palaeognathae (including extinct birds such as moa) are analysed with electron backscatter diffraction (EBSD), which provides detailed microstructural and crystallographic information for eggshells. The palaeognath eggshells could be categorized into ostrich-, rhea-, and tinamou-style morphotypes and rhea-style eggshell appears ancestral form, while respective ostrich-style and tinamou-style morphotypes are interpreted as convergent evolutions. The implications are not only helpful for understanding evolution of modern dinosaur eggshells, but also aid other disciplines such as zooarchaeology.
The timing of dynamical events and the formation timing of the gas giants remains unclear
In this study B. G. Rider-Stokes, R. C. Greenwood, M. Anand, L. F. White, I. A. Franchi, V. Debaille, S. Goderis, L. Pittarello, A. Yamaguchi, T. Mikouchi & P. Claeys at the Open University, studied the microstructure of olivine in a meteorite (through EBSD) that had been measured for oxygen isotopic compositions. The olivine revealed multiple orientations and triple grain boundaries, indicative of recrystallization. This, alongside the isotopic disequilibrium, implied that the olivine formed in a different location in the Solar System compared to the rest of the sample.
It was hypothesized that the meteorite experienced planetary mixing induced by the formation of Jupiter, providing a statistical constraint on its birth.
© Oxford Instruments 2024
