MSSL Solar & Planetary Physics Consolidated Grant 2016-2019

MSSL太阳能

• 批准号: ST/N000722/1
• 负责人: Andrew Coates
• 金额: $ 258.63万
• 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: 2016
• 资助国家: 英国
• 起止时间: 2016 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FN000722%2F1
• 关键词: MSSL; Solar; Planetary; Physics; Consolidated

The aims of the solar system programme at MSSL are to break new ground in the understanding of the physical processes at work within each of our theme topics: (a) solar activity and the origin at the Sun of the solar wind and disturbances within it; including coronal mass ejections (CME), flares, filaments and filament eruptions(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(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 populations and processes driving aurorae and X-ray emission (e) planetary surface formation processes; including cratering chronology and dynamic feature tracking via super-resolution restoration

MSSL太阳能系统计划的目的是在我们每个主题主题中工作的实际过程中打破新的基础：（a）太阳能活动和太阳风的太阳和内部骚乱的阳光；包括冠状质量弹出（CME），耀斑，细丝和细丝爆发（b）太阳风形成以及通过地球层传播和进化；包括太阳风的来源和了解太阳上的哪些区域控制太阳风（C）太阳风与地球磁层的相互作用；包括在动力学和大尺度上的太阳风理，重新连接，磁层加速度以及运输过程以及控制着Aurora和辐射带（D）在其他行星环境下太阳风和等离子体相互作用的过程；包括电离层过程，彗星 - 血浆相互作用，行星磁层等离子体种群以及驱动Aurorae和X射线发射（E）行星表面形成过程的过程；包括时间表的遍历和动态特征跟踪通过超分辨率恢复

项目成果

Cassini observations of Saturn's southern polar cusp

卡西尼号对土星南极尖点的观测

• DOI: 10.1002/2015ja021957
• 发表时间: 2016
• 期刊: Space Physics
• 作者: Arridge C

Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence

• DOI: 10.1017/s0022377821000404
• 发表时间: 2021-03
• 期刊: Journal of Plasma Physics
• 影响因子: 2.5
• 作者: Jeffersson A. Agudelo Rueda;D. Verscharen;R. Wicks;C. Owen;G. Nicolaou;A. Walsh;I. Zouganelis;K. Germaschewski;S. Vargas Domínguez

Virtual Planetary Space Weather Services offered by the Europlanet H2020 Research Infrastructure

• DOI: 10.1016/j.pss.2017.04.020
• 发表时间: 2017-01
• 期刊: Planetary and Space Science
• 影响因子: 2.4
• 作者: N. Andr'e;M. Grande;N. Achilleos;M. Barth'el'emy;M. Bouchemit;K. Benson;P. Blelly;E. Budnik;S. Caussarieu;B. Cecconi;T. Cook;V. G'enot;Patrick Guio;A. Goutenoir;B. Grison;R. Hueso;M. Indurain;G. Jones;J. Lilensten;A. Marchaudon;D. Matthiae;A. Opitz;A. Rouillard;I. Stanislawska;J. Souček;C. Tao;L. Tomasik;J. Vaubaillon

Evidence for local particle acceleration in the first recurrent galactic cosmic ray depression observed by Solar Orbiter The ion event on 19 June 2020

太阳轨道飞行器观测到的第一次周期性银河系宇宙线凹陷中局部粒子加速的证据 2020 年 6 月 19 日的离子事件

• DOI: 10.1051/0004-6361/202140966
• 发表时间: 2021
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Aran A

A magnetodisc model service for planetary space weather studies

用于行星空间天气研究的磁盘模型服务

• DOI: 10.1051/swsc/2019022
• 发表时间: 2019
• 期刊: Journal of Space Weather and Space Climate
• 影响因子: 3.3
• 作者: Achilleos N