Short term visitors programme for astrophysical research at the University of Exeter

埃克塞特大学天体物理研究短期访客计划

• 批准号: PP/D001617/1
• 负责人: Matthew Bate
• 金额: $ 1.61万
• 依托单位: UNIVERSITY OF EXETER
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2006
• 资助国家: 英国
• 起止时间: 2006 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=PP%2FD001617%2F1
• 关键词: Short; term; visitors; programme; astrophysical

There are two groups at the University of Exeter that conduct astrophysical research, the Astrophysics Group in the School of Physics and the Fluids and Magnetohydrodynamics (MHD) Group within the School of Engineering, Computer Science and Mathematics. The primary area of research of the Astrophysics Group is star formation, one of the current priority areas for astronomical research in the United Kingdom (U.K.), while the Fluids and MHD Group conducts research into astrophysical fluid dynamics, in particular dynamo theory and planetary atmospheres. Research on extra-solar planets provides a clear link between the groups. Together, these groups collaborate with many researchers both across the U.K. and overseas. However, Exeter is relatively geographically isolated. In order that these collaborations continue to flourish and that new links be formed it is essential that a short-term visitors programme be maintained at Exeter. This grant application is intended to fund our visitors programme over the next three years.

埃克塞特大学有两个小组进行天体物理学研究，物理学院的天体物理学小组和工程、计算机科学和数学学院的流体和磁流体动力学（MHD）小组。天体物理学组的主要研究领域是恒星形成，这是目前英国天文学研究的优先领域之一，而流体和MHD组则研究天体物理流体动力学，特别是发电机理论和行星大气。对太阳系外行星的研究为这两个群体之间提供了明确的联系。这些小组与英国和海外的许多研究人员合作。然而，埃克塞特在地理上相对孤立。为了使这些合作继续蓬勃发展并形成新的联系，在埃克塞特维持短期访客计划是至关重要的。这项拨款申请旨在资助我们未来三年的访客计划。

项目成果

Modelling solar-like variability for the detection of Earth-like planetary transits II. Performance of the three-spot modelling, harmonic function fitting, iterative nonlinear filtering, and sliding boxcar filtering

模拟类太阳变率以检测类地行星凌日 II。

• DOI: 10.1051/0004-6361:200810726
• 发表时间: 2009
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Bonomo A

Modelling solar-like variability for the detection of Earth-like planetary transits. II) Performance of the three-spot modelling, harmonic function fitting, iterative non-linear filtering and sliding boxcar filtering

模拟类太阳变率以检测类地行星凌日。

• DOI: 10.48550/arxiv.0812.1667
• 发表时间: 2008
• 作者: Bonomo A

Three-dimensional simulations of rotationally-induced line variability from a Classical T Tauri star with a misaligned magnetic dipole

具有未对准磁偶极子的经典 T Tauri 星旋转引起的线变化的三维模拟

• DOI: 10.48550/arxiv.0802.0201
• 发表时间: 2008
• 作者: Kurosawa R