用平方公里阵列天文台（SKAO）理解脉冲星磁层
Understanding Pulsar Magnetospheres with the SKAO
AI总结：
介绍用SKAO研究脉冲星磁层，阐述过去十年该领域进展及现代射电望远镜的作用，说明SKAO将通过监测调查等变革此领域，还提及AA*和AA4配置观测机会对解决脉冲星射电发射物理问题的作用。
AI中文摘要：
平方公里阵列（SKA）望远镜将在很宽的射电波段带来无与伦比的灵敏度、南天广阔的视场以及子阵列能力，使其成为研究脉冲星磁层的理想仪器。本章描述了过去十年脉冲星磁层物理学取得的进展，以及现代射电望远镜，特别是SKA前身和探路者的进展如何使之成为可能。解释了SKA望远镜将如何通过大规模监测调查以及对独特源的深入跟踪观测和新发现来变革脉冲星磁层物理学领域。最后，描述了AA*和AA4配置的特定观测机会将如何在未来几年取得解决脉冲星射电发射物理问题所需的进展。
英文摘要：
The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make them the ideal instruments for studying the pulsar magnetosphere. This chapter describes the advances that have been made in pulsar magnetosphere physics over the last decade, and details how these have been made possible through the advances of modern radio telescopes, particularly SKA precursors and pathfinders. It explains how the SKA telescopes would transform the field of pulsar magnetosphere physics through a combination of large-scale monitoring surveys and in-depth follow-up observations of unique sources and new discoveries. Finally, it describes how the specific observing opportunities available with the AA* and AA4 configurations will achieve the advances necessary to solve the problem of pulsar radio emission physics in the coming years.
