A5110209632- Solar and Space Plasma Dynamics
- Astro and Planetary Science
- Stellar, planetary, and galactic studies
- Planetary Science and Exploration
- Dark Matter and Cosmic Phenomena
- Ionosphere and magnetosphere dynamics
- Spacecraft Design and Technology
- Particle physics theoretical and experimental studies
- Geophysics and Gravity Measurements
- Geomagnetism and Paleomagnetism Studies
- Astrophysics and Star Formation Studies
- Nuclear Physics and Applications
- Astronomy and Astrophysical Research
- Atomic and Subatomic Physics Research
- Particle Detector Development and Performance
- CCD and CMOS Imaging Sensors
- Cold Atom Physics and Bose-Einstein Condensates
- Viral Infectious Diseases and Gene Expression in Insects
- Space exploration and regulation
- Isotope Analysis in Ecology
- 3D Modeling in Geospatial Applications
- Monoclonal and Polyclonal Antibodies Research
- Aeolian processes and effects
- Astronomical Observations and Instrumentation
- Astrophysics and Cosmic Phenomena
Swinburne University of Technology
2022-2023
University College London
2023
ARC Centre of Excellence for Dark Matter Particle Physics
2022
The University of Melbourne
2022
ARC Centre of Excellence for All-sky Astrophysics
2022
ASTRO-3D
2022
Royal Observatory of Belgium
2004-2007
QUAD Engineering (Canada)
2007
University of Birmingham
2003
University of Colorado Boulder
2001
Abstract SABRE (Sodium iodide with Active Background REjection) is a direct detection dark matter experiment based on arrays of radio-pure NaI(Tl) crystals. The aims at achieving an ultra-low background rate and its primary goal to confirm or refute the results from DAMA/LIBRA experiment. Proof-of-Principle phase was carried out in 2020–2021 Gran Sasso National Laboratory (LNGS), Italy. next consists two full-scale experiments: South Stawell Underground Physics Laboratory, Australia, North...
Observations suggest that the interplanetary extensions of coronal mass ejections (iCMEs) may be accelerated or decelerated in their passage through solar wind. Interplanetary scintillation measurements (IPS) can detect iCMEs beyond field view Large‐Angle and Spectrometric Coronagraph coronagraphs provide information on velocities. The European Incoherent Scatter Radar Multi Element Radio Linked Interferometer Network systems, with a covering 10–120 radii, inner regions IPS observations also...
Molecular interferometric imaging (MI2) is a common-path technique for detecting protein binding to surfaces. The experimental metrology limit 10 pm/pixel longitudinal resolution at 0.4-mum diffraction-limited lateral resolution, corresponding 1.7 attogram of protein, which only 8 antibody molecules per pixel, near single-molecule detection. scaling mass sensitivity the 5 fg/mm. We demonstrate microarray application in 128-multiplex immunoassay. Assay applications include prostate specific...
SABRE (Sodium iodide with Active Background REjection) is a direct detection dark matter experiment based on arrays of radio-pure NaI(Tl) crystals. The aims at achieving an ultra-low background rate and its primary goal to confirm or refute the results from DAMA/LIBRA experiment. Proof-of-Principle phase was carried out in 2020-2021 Gran Sasso National Laboratory (LNGS), Italy. next consists two full-scale experiments: South Stawell Underground Physics Laboratory, Australia, North LNGS. This...
Context. With a mass exceeding several 10^4 solar masses and rich dense population of massive stars, supermassive young star clusters represent the most star-forming environment that is dominated by feedback from stars gravitational interactions among stars. Aims. In this paper we present "Extended Westerlund 1 2 Open Clusters Survey" (EWOCS) project, which aims to investigate influence starburst on formation planets, evolution both low high The primary targets project are 2, closest Sun....
We describe a proposed Dust Charge Probe (DCP) experiment to characterize the dust loaded photoelectron sheath on surface of Mars. DCP can provide measurements photoelectric sheath, as well charge, size and velocity distribution wind-entrained particles. Here we discuss expected physical properties detection technique engineering design experiment.
Two scientific instruments for Sun observations are being developed to be part of the payload ESA's second microsatellite, Proba-II (Project On-board Autonomy). PROBA-2 is scheduled launch in early 2007, on a low Earth orbit. Like Proba-1, orbit since October 2001, Proba-2 100-kilogram class spacecraft. PROBA-II will demonstrate new advanced technologies its but also platform subsystems such as star tracker, digital sensor, cool gas generator, solar array concentrator, Li-Ion Battery,...
ABSTRACT We use high-resolution, hydrodynamic, galaxy simulations from the Latte suite of FIRE-2 to investigate inherent variation dark matter in sub-sampled regions around Solar Circle a Milky Way-type analogue and its impact on direct detection. These show that baryonic back reaction, as well assembly history substructures, has lasting impacts matter’s spatial velocity distributions. are experienced ‘gusts’ wind Circle, potentially complicating interpretations detection experiments Earth....
The SABRE (Sodium iodide with Active Background REjection) experiment aims to provide a model independent test of the signal observed by DAMA/LIBRA detecting an annual modulation from dark matter interactions in ultra-high purity NaI(Tl) crystals. consists two detectors: North, located at Laboratori Nazionali del Gran Sasso (LNGS), and South, newly completed Stawell Underground Physics Laboratory (SUPL) Stawell, Australia - first deep underground laboratory Southern Hemisphere. Here we...