A Stress-relax Model for Stellar Flares. This project aims to improve our ability to predict solar and stellar flares by developing a theoretical model for the build-up and release of magnetic stress in stellar atmospheres. Solar flares are the most energetic events in the solar system, and together with associated coronal mass ejections can create hazardous conditions in our local space environment. Stellar flares are thousands of times more energetic and produce dangerous space weather for exo ....A Stress-relax Model for Stellar Flares. This project aims to improve our ability to predict solar and stellar flares by developing a theoretical model for the build-up and release of magnetic stress in stellar atmospheres. Solar flares are the most energetic events in the solar system, and together with associated coronal mass ejections can create hazardous conditions in our local space environment. Stellar flares are thousands of times more energetic and produce dangerous space weather for exoplanets orbiting flare stars. Expected outcomes include insight into the flare mechanism, and new approaches to flare prediction. The major potential benefit is improved solar and stellar space weather forecasting to protect human safety and infrastructure.Read moreRead less
Understanding the sources of the slow solar wind. This project aims to reveal the origins of the slow solar wind, a continuous stream of plasma emanating from the Sun that fills the solar system and impacts the Earth. This project expects to enhance our understanding of how this solar wind is accelerated and structured using a suite of state-of-the-art computational simulations. In doing this, the project expects to provide critical physical understanding to allow interpretation of data from NA ....Understanding the sources of the slow solar wind. This project aims to reveal the origins of the slow solar wind, a continuous stream of plasma emanating from the Sun that fills the solar system and impacts the Earth. This project expects to enhance our understanding of how this solar wind is accelerated and structured using a suite of state-of-the-art computational simulations. In doing this, the project expects to provide critical physical understanding to allow interpretation of data from NASA and ESA's flagship space missions Parker Solar Probe and Solar Orbiter. Benefits should include enhanced physical understanding that will contribute to the international effort to develop reliable space-weather forecasting systems, critical for space exploration and space-based technology.Read moreRead less
Prediction of coronal mass ejections and their radio emissions. This project aims to explain in detail the motion and properties of coronal mass ejections (CMEs) leaving the sun, the radio emissions they generate, and space weather triggers for the sun and other stars. The project expects to create new knowledge in the fields of space, plasma, and astro-physics and space weather research. Expected outcomes include capabilities to accurately predict CMEs and space weather triggers from the sun to ....Prediction of coronal mass ejections and their radio emissions. This project aims to explain in detail the motion and properties of coronal mass ejections (CMEs) leaving the sun, the radio emissions they generate, and space weather triggers for the sun and other stars. The project expects to create new knowledge in the fields of space, plasma, and astro-physics and space weather research. Expected outcomes include capabilities to accurately predict CMEs and space weather triggers from the sun to Earth and theories for type II and IV solar radio bursts. Benefits include high-level training and enhanced human capital and scientific prominence for Australia.Read moreRead less