Solar System Consolidated Grant 2019-22

伦敦大学圣迭戈分校太阳系方案的目的是在我们的每一个主题中对工作中的物理过程的理解方面取得新的进展：a)太阳磁活动、其原因、后果和对太阳系的影响；b)太阳风的形成和通过日光层的传播和演化；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现场动力学。c)太阳风与地球磁层的相互作用；D)其他行星环境中的太阳风和等离子相互作用；(B)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地表极光和X射线发射的过程；(B)行星表面形成过程，包括陨石坑年表和通过超分辨率恢复进行动态特征跟踪；这些目标是利用空间和地面仪器的数据和建模来解决的。

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.