Researchers and partners from industry, government, and academia are invited to a free workshop on May 24th 2019 to discuss the future of satellite-based remote sensing of Earth’s water resources and ocean dynamics. The workshop will be held at the Sydney Bureau of Meteorology and streamed live to the web.
In the coming decade, new satellite missions will map Earth’s surface water and sea level (ocean topography) at a resolution that has not been possible before. These observations will provide critical information that is needed to assess water resources on land, track regional sea level changes, monitor coastal processes, and observe small-scale ocean currents and eddies. The first of these satellites, the NASA/CNES Surface Water Ocean Topography (SWOT) mission, is scheduled for launch in late 2021.
The workshop on future high-resolution satellite altimetry is organized by the Australian Bureau of Meteorology and the Australian Surface Water Ocean Topography (AUSWOT) working group, a consortium of researchers and stakeholders from industry, government, and academia that aims to develop Australia’s capability in the field of surface water and ocean topography and address key issues relevant to the Asia-Pacific region.
UNSW Sydney is collaborating with the non-profit Brian Holden Vision Institute and medical device company TeleMedC in a new $445,000 research project to develop a state-of-the-art computational model of tear film dynamics of a blinking eye.
Each time you blink, your eyes replenish the tear film, a thin fluid interface between the surface of the eye and the environment. Although it is less than a tenth the thickness of a human hair, the tear film plays an important role in cleaning and protecting the delicate ocular surface while maintaining clear vision. Chronic breakdown of the tear film is associated with Dry Eye Syndrome, a debilitating disease that affects millions of Australians and up to half those aged over 50.
A critical knowledge gap is the clinical and environmental factors affecting tear film break up in both healthy subjects and dry-eye patients. The project will address this knowledge gap by developing a state-of-the-art computational model of tear film, validated against in vitro and in vivo data, suitable for clinical studies by researchers in both academia and industry.
The new research partnership involves Dr Shane Keating at UNSW’s School of Mathematics & Statistics and Dr Nicole Carnt at UNSW’s School of Optometry & Vision Science, and Prof Arthur Ho at the Brian Holden Vision Institute. The project will be carried out in collaboration with TeleMedC, LCC, a pioneering medical device company that is developing the next generation of ophthalmic diagnostic imaging systems for face-to-face and virtual medical consultations, screening, monitoring and health prevention purposes for remote and urban communities.
UNSW Sydney has awarded a prestigious Scientia PhD scholarship to PhD student Yu Wang to work with Shane, Nicole, and Arthur on developing the computational model of the tear film. The Scientia scholarship scheme aims to harness cutting-edge research to solve complex problems and improve the lives of people in local and global communities. Scientia scholars receive a $200,000 scholarship package in the form of a stipend, travel, and development support over four years. International scholars also receive a tuition fee scholarship worth $200,000. In addition, UNSW Sydney and TeleMedC, LLC have provided $45,000 in support for the project through the Industry Network Seed Fund program.
Friday 7 December is the last day to register for this interdisciplinary workshop sponsored by the Bureau of Meterology, the Australian Meteorological and Oceanographic Society, and UNSW School of Mathematics and Statistics.
Climate scientist and oceanographer Dr Stephen Griffies will deliver a public lecture at the AMSI Summer School at UNSW Sydney on Wednesday 30 January 2019.
Stephen Griffies has been at Princeton University and NOAA’s Geophysical Fluid Dynamics Laboratory since 1993. His research spans a broad spectrum of fundamental and applied areas of ocean and climate science, including numerical modelling, mesoscale and submesoscale dynamics, turbulence parameterizations, Southern Ocean dynamics, Atlantic predictability and variability, sea level science, Lagrangian and watermass analyses, and foundations of ocean fluid mechanics. He is the 2014 recipient of the EGU Fridtjof Nansen medal for oceanographic excellence and is a fellow of the American Geophysical Union.
A Math/Physics View of Ocean Circulation
Abstract: Ocean circulation acts like bloodlines for the planet, moving heat, oxygen, carbon, and nutrients around the world. Furthermore, ocean circulation moderates climate: think of the different climates between a maritime region (Sydney) and a mid-continent region (Alice Springs). Ocean circulation thus affects life both on land and within the ocean. When the ocean circulation slows or speeds, the climate system is affected. Ocean and climate scientists aim to understand the physical mechanisms underlying changes in ocean circulation. What forces cause the changes? How predictable are they? To help answer these questions, oceanographers formulate mathematical equations for the governing physical laws and place the equations on supercomputers for grand simulations. In this talk I will offer a sampling of the research questions confronting ocean scientists who make use of mathematics, physics, and computer simulations. Some of the questions touch upon the most difficult questions facing humanity in the 21st century.
Date: Wednesday 30 January 2019 Time: 7.00pm – approximately 8.30pm (ADST) Light refreshments will be available from 6.00pm Venue: The Science Theatre, F13, Union Road, The University of New South Wales, Kensington Campus, Sydney Address: Gate 2, High Street, The University of New South Wales, Kensington Cost: Free (Register online)