Solar and Heliospheric Physics with the Square Kilometre Array
Valery M. Nakariakov, Mario M. Bisi, Philippa K. Browning, Dalmiro Maia, Eduard P. Kontar, Divya Oberoi, Peter T. Gallagher, Iver H. Cairns, Heather Ratcliffe
The fields of solar radiophysics and solar system radio physics, or radio heliophysics, will benefit immensely from an instrument with the capabilities projected for SKA. Potential applications include interplanetary scintillation (IPS), radio-burst tracking, and solar spectral radio imaging with a superior sensitivity. These will provide breakthrough new insights and results in topics of fundamental importance, such as the physics of impulsive energy releases, magnetohydrodynamic oscillations and turbulence, the dynamics of post-eruptive processes, energetic particle acceleration, the structure of the solar wind and the development and evolution of solar wind transients at distances up to and beyond the orbit of the Earth. The combination of the high spectral, time and spatial resolution and the unprecedented sensitivity of the SKA will radically advance our understanding of basic physical processes operating in solar and heliospheric plasmas and provide a solid foundation for the forecasting of space weather events.
Interplanetary scintillation-informed heliospheric modelling for the MeerKAT Pulsar Timing Array 4.5 yr dataset
Swinburne University of Technology（斯威本科技大学）；OzGrav: The ARC Centre of Excellence for Gravitational Wave Discovery（引力波发现ARC卓越中心）；CSIRO, Space and Astronomy（CSIRO空间与天文学部）
Solar, Heliospheric and Ionospheric Physics: Pathfinders, Precursors and SKAO Perspective
ASTRON - Netherlands Institute for Radio Astronomy（荷兰射电天文研究所）；Indian Institute of Technology, Kanpur（坎普尔印度理工学院）；National Centre for Radio Astrophysics, Tata Institute of Fundamental Research（塔塔基础研究院国家射电天体物理中心）；Dublin Institute for Advanced Studies（都柏林高等研究院）；University of Oslo（奥斯陆大学）；University of Bath（巴斯大学）
VLA cm-wave survey of young stellar objects in the Oph A cluster: constraining extreme UV- and X-ray-driven disk photo-evaporation -- A pathfinder for Square Kilometre Array studies
Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array
University of Amsterdam（阿姆斯特丹大学）；ASTRON, The Netherlands Institute for Radio Astronomy（荷兰射电天文研究所）；Observatoire de Paris（巴黎天文台）；National Astronomical Observatory of Japan（日本国立天文台）；University of Tokyo（东京大学）；California Institute of Technology（加州理工学院）；University of Colorado Boulder（科罗拉多大学博尔德分校）；University of Groningen（格罗宁根大学）
Trinity College Dublin（都柏林三一学院）；Royal Holloway, University of London（伦敦大学皇家霍洛威学院）；University of Manchester（曼彻斯特大学）；Curtin University（科廷大学）；Université d’Orléans（奥尔良大学）；CNRS（法国国家科学研究中心）；Institute of Space Sciences (CSIC-ICE)（空间科学研究所（CSIC-ICE））；Institut d’Estudis Espacials de Catalunya (IEEC)（加泰罗尼亚空间研究研究所（IEEC））；ASTRON, the Netherlands Institute for Radio Astronomy（荷兰射电天文研究所）；National Astronomical Observatories, Chinese Academy of Sciences（中国科学院国家天文台）
Probing Physical Conditions in Classical and Symbiotic Novae with the Square Kilometre Array Observatory
Radboud University（拉博德大学）；Joint Institute for VLBI ERIC（甚长基线干涉测量欧洲研究联盟联合研究所）；ASTRON（荷兰射电天文研究所）；University of Manchester（曼彻斯特大学）；The University of Sydney（悉尼大学）；ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav)（引力波发现卓越研究中心）；Texas Tech University（德克萨斯理工大学）
