
After your experiment
Following your experiment at the Australian Synchrotron there are certain tasks that users can complete including a user feedback survey and claiming reimbursement for travel expenses.
Showing 261 - 280 of 393 results
Following your experiment at the Australian Synchrotron there are certain tasks that users can complete including a user feedback survey and claiming reimbursement for travel expenses.
Advances in radon measurement technology by ANSTO researchers over the past decade have enabled the improved characterisation of the composition of pristine air masses that reach Antarctica.
In cooperation with ANSTO and for the third year running, the IAEA has recently hosted a two-week online training course for women professionals working in numerous nuclear industries around the world, titled 'Women 4 Nuclear Science in Education and Communications'.
Training hosted and delivered by ANSTO on behalf of the IAEA assisted the Philippine Nuclear Research Institute (PNRI) to prepare for the successful management of a recent nuclear forensics operation.
In space, without the protection of the magnetosphere, the type and dose of radiation is considerably different to what is naturally experienced on earth.
Using nuclear techniques to help sustain Australia's finite groundwater resources
ANSTO part of consortium funded by Federal Government to develop new radioimmunological drugs.
The Medium Energy- X-ray Absorption Spectroscopy beamlines will provide access to XANES and EXAFS data from a bending magnet source, optimised for cutting-edge applications in biological, agricultural and environmental science in an energy range that is not currently available at the Australia Synchrotron.
Consortium will map the 86 billion nerve cells, 100 trillion connections and neurotransmitters in the human brain.
Charcoal particles from recent bushfires in NSW were carried 50 kilometres by the wind, which has significance for fire history reconstruction.
Soft x-rays are generally understood to be x-rays in the energy range 100-3,000 eV. They have insufficient energy to penetrate the beryllium window of a hard x-ray beamline but have energies higher than that of extreme ultraviolet light.