Solar System Physics

太阳系物理学

• 批准号: PP/E001157/1
• 负责人: Manuel Grande
• 金额: $ 295.32万
• 依托单位: Aberystwyth University
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2007
• 资助国家: 英国
• 起止时间: 2007 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=PP%2FE001157%2F1
• 关键词: Solar; System; Physics

At Aberystwyth, we are investigating the complex intercouplings of the inner solar system. The Sun, Earth and planets are linked by the interplanetary medium between them. Eruptions from the Sun result in large three-dimensional clouds of plasma which travel at supersonic speeds through interplanetary space. At Earth, they produce geomagnetic storms which disrupt our communications, endanger astronauts and, on the ground, produce compass deflections and, most visibly, the Northern Lights. The same mechanisms that result in a habitable Earth produce effects which shape the surfaces and atmospheres of the inner planets and give rise to the inhospitable conditions on the Moon, Mercury, Venus and, to a lesser extent, Mars. In order to understand these interlinked processes we need to make state of the art measurements of the environments of the Sun, the Planets and the Space in between. These include ground-based measurements and data from space probes both in orbit and on the surfaces of other planets. We can then develop the theories which explain these observations and enable us to predict when they will occur and how strongly they will affect our inner solar system environment. There is a virtuous circle whereby new observations produce new theories, new questions and hence new experimental techniques which allow us to make the next generation of observations. At Aberystwyth, we are world leaders in each of these stages. Our particular strengths are in X-ray and ultraviolet obserations of the Sun and planets, autonomous robots for exploring planetary surfaces and radar techniques to probe near-Earth and interplanetary space. At Aberystwyth we are the lead investigators for the X-ray instrument currently orbiting the Moon on the SMART-1 spacecraft, and its successor on the Indian Chandrayaan-1 mission due to arrive at the Moon in late 2007. We are also playing a leading role in the preparation of the X-ray instruments on the forthcoming BepiColombo mission to Mercury. Our world-leading robotics software would have given Beagle-2 autonomy in making measurements on the surface of Mars and will now be employed when Europe returns to Mars with the upcoming ExoMars mission. Investigators from Aberystwyth are also part of the teams of scientists behind instruments currently orbitting Venus, Mars and the Earth. Aberystwyth is making a unique step forward in probing the the interplanetary medium by observing the twinkling of stars in radar, known as interplanetary scintillation. At the Earth, we apply the technique of tomography, as used in medical scanning, to take snapshots and build three-dimensional pictures of the Earth's ionosphere. Our theory programme concentrates on understanding how the highly dynamic three-dimensional plasma structures can form on the Sun, erupt and accelerate into interplanetary space, and how these rapidly changing structures interact with the magnetic fields, atmospheres and surfaces of the inner planets. By testing our theories at other planets we improve our understanding of the processes which shape our own environment at the Earth. We build computer simulations of these theories which show us the complicated behaviour of the surface and atmosphere of the Sun, plasma clouds in interplanetary space and planetary atmospheres. The University has made a large-investment in the new technology of three-dimensional visualisation and virtual reality which is the only way to truely visualise and understand what is happening. Aberystwyth is unique in our ability to investigate each and every link in the chain of interaction which link the Sun, Earth and Planets. This puts us in an ideal position to understand how events in the inner solar system shape the environment in which we live.

在阿伯里斯特威斯，我们正在研究太阳系内部复杂的相互耦合。太阳、地球和行星通过它们之间的行星际介质联系在一起。来自太阳的爆发会产生大型的三维等离子云，这些云以超音速穿过行星际空间。在地球上，它们会产生地磁风暴，破坏我们的通信，危及宇航员，在地面上，会产生罗盘偏转，最明显的是，会产生北方光。导致可居住地球的相同机制产生了影响，这些影响塑造了内行星的表面和大气层，并导致月球，水星，金星以及火星上的不适宜居住的条件。为了理解这些相互关联的过程，我们需要对太阳、行星和它们之间的空间的环境进行最先进的测量。这些包括地面测量和来自轨道上和其他行星表面的空间探测器的数据。然后，我们可以发展解释这些观测的理论，并使我们能够预测它们何时发生以及它们将如何强烈地影响我们的太阳系内部环境。这是一个良性循环，新的观察产生新的理论，新的问题，从而产生新的实验技术，使我们能够进行下一代的观察。在阿伯里斯特威斯，我们在每个阶段都是世界领先者。我们的特别优势在于太阳和行星的X射线和紫外线探测，探索行星表面的自动机器人以及探测近地和行星际空间的雷达技术。在阿伯里斯特威斯，我们是目前在SMART-1航天器上绕月球运行的X射线仪器的主要研究人员，以及将于2007年底抵达月球的印度Chandrayaan-1使命的继任者。我们还在为即将进行的BepiColombo水星使命准备X射线仪器方面发挥主导作用。我们世界领先的机器人软件将使小猎犬2号在火星表面进行测量的自主权，现在将在欧洲返回火星与即将到来的ExoMars使命。来自阿伯里斯特威斯的调查人员也是目前围绕金星、火星和地球运行的仪器背后的科学家团队的一部分。阿伯里斯特威斯正在通过雷达观测恒星的闪烁，即行星际闪烁，在探测行星际介质方面迈出了独特的一步。在地球上，我们采用医学扫描中使用的断层摄影技术，拍摄地球电离层的快照和三维照片。我们的理论计划集中于了解高度动态的三维等离子体结构如何在太阳上形成，爆发并加速进入行星际空间，以及这些快速变化的结构如何与内行星的磁场，大气和表面相互作用。通过在其他行星上测试我们的理论，我们提高了对地球环境形成过程的理解。我们建立这些理论的计算机模拟，向我们展示了太阳表面和大气层的复杂行为，行星际空间和行星大气中的等离子体云。大学在三维可视化和虚拟现实的新技术上进行了大量投资，这是真正可视化和理解正在发生的事情的唯一途径。阿伯里斯特威斯是独一无二的，我们有能力调查每一个环节的相互作用链连接太阳，地球和行星。这使我们处于一个理想的位置，以了解内太阳系的事件如何塑造我们生活的环境。

项目成果

Modulation of nightside polar patches by substorm activity

• DOI: 10.5194/angeo-27-3923-2009
• 发表时间: 2009-10
• 期刊: Annales Geophysicae
• 影响因子: 1.9
• 作者: A. Wood;S. E. Pryse;J. Moen

The transterminator ion flow at Venus at solar minimum

太阳极小期金星的终结者离子流

• DOI: 10.1016/j.pss.2012.08.006
• 发表时间: 2012
• 期刊: Planetary and Space Science
• 影响因子: 2.4
• 作者: Wood A