Solar System Consolidated Grant 2019-22

太阳能系统综合拨款 2019-22

• 批准号: ST/S000240/1
• 负责人: Andrew Coates
• 金额: $ 374.23万
• 依托单位: University College London
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FS000240%2F1
• 关键词: Solar; System; Consolidated; Grant; 2019

The aims of the solar system programme at UCL-MSSL are to break new ground in the understanding of the physical processes at work within each of our theme topics: a) solar magnetic activity, its causes, consequences, and influence on the Solar System b) solar wind formation and propagation and evolution through the heliosphere; including the source of the solar wind and understanding which regions on the Sun control the solar wind, and in-situ dynamics of energy transport in space plasmas.c) solar wind interaction with the Earth's magnetosphere; including solar wind physics at kinetic and large scales, reconnection, magnetospheric acceleration and transport processes and processes controlling the aurora and radiation belts d) solar wind and plasma interactions at other planetary environments; including ionospheric processes, comet-plasma interactions, planetary magnetospheric plasma and charged dust populations and processes driving aurorae and X-ray emission in atmospheres and on surfacese) planetary surface formation processes; including cratering chronology and dynamic feature tracking via super-resolution restoration These goals are addressed using data from space- and ground- based instruments, and modelling.

在UCL-MSSL的太阳系计划的目的是在我们的每个主题内工作的物理过程的理解开辟新天地：a）太阳磁场活动，其原因，后果和对太阳系的影响B）太阳风的形成和传播和演变通过日光层;包括太阳风的来源和了解太阳上哪些区域控制太阳风，以及空间等离子体中能量传输的原位动力学。包括动力学和大尺度的太阳风物理学、重连、磁层加速和传输过程以及控制极光和辐射带的过程d）太阳风和等离子体在其他行星环境中的相互作用;包括电离层过程彗星等离子体相互作用行星磁层等离子体和带电尘埃群以及驱动大气层和表面极光和X射线发射的过程;行星表面形成过程;包括陨石坑年表和动态特征跟踪通过超分辨率恢复这些目标是解决使用数据从空间和地面为基础的仪器，和建模。

项目成果

The dust tail gap of C/2014 Q1 (PanSTARRS)

C/2014 Q1 的尘埃尾隙（PanSTARRS）

• DOI: 10.5194/epsc2021-481
• 发表时间: 2021
• 作者: Afghan Q

Radial evolution of thermal and suprathermal electron populations in the slow solar wind from 0.13 to 0.5 au : Parker Solar Probe Observations

0.13 至 0.5 au 的慢速太阳风中热电子和超热电子群的径向演化：帕克太阳探测器观测

• DOI: 10.48550/arxiv.2204.05001
• 发表时间: 2022
• 作者: Abraham J

Oxford Research Encyclopedia of Planetary Science

牛津研究行星科学百科全书

• DOI: 10.1093/acrefore/9780190647926.013.227
• 发表时间: 2021
• 作者: Achilleos N

Magnetospheres in the Solar System

太阳系中的磁层

• DOI: 10.1002/9781119815624.ch29
• 发表时间: 2021
• 作者: Achilleos N

Structural analysis of the dust tail of Comet NEOWISE (C/2020 F3)

NEOWISE彗星（C/2020 F3）尘埃尾的结构分析

• DOI: 10.5194/epsc2022-895
• 发表时间: 2022
• 作者: Afghan Q