Solar radio bursts, the origin and properties of the sun's corona and solar wind, and space weather

太阳射电爆发、日冕和太阳风的起源和特性以及空间天气

• 批准号: DP1095510
• 负责人: Prof Iver Cairns
• 金额: $ 28.21万
• 依托单位: The University of Sydney
• 依托单位国家: 澳大利亚
• 项目类别: Discovery Projects
• 财政年份: 2010
• 资助国家: 澳大利亚
• 起止时间: 2010-05-31 至 2013-12-31
• 项目状态: 已结题
• 来源: https://dataportal.arc.gov.au/RGS/Web/Grants/DP1095510
• 关键词: Solar; radio; bursts; origin; properties

This project uses solar radio bursts to answer fundamental scientific questions about the Sun, predict space weather events at Earth, and motivate theories for the bursts and shocks. It will discover the corona's origin and where the solar wind is accelerated, understand how shocks reform and accelerate particles, and develop quantitative theories for radio bursts. These discoveries and associated high-level training of staff and students will increase Australia's international scientific standing, expertise, infrastructure, and human capital. It involves international collaborations on NASA's $600M STEREO mission and the MWA radio telescope, among others, and supports the new Decadal Plan for Australian Space Science.

该项目使用太阳射电爆发来回答有关太阳的基本科学问题，预测地球上的空间天气事件，并激发关于爆发和冲击的理论。它将发现日冕的起源和太阳风被加速的地方，了解激波如何改造和加速粒子，并开发射电爆发的定量理论。这些发现以及对教职员工和学生的相关高水平培训将提高澳大利亚的国际科学地位、专业知识、基础设施和人力资本。它涉及在NASA耗资6亿美元的立体声任务和MWA射电望远镜等方面的国际合作，并支持新的澳大利亚空间科学十年计划。