Flares and Coronal Mass Ejections (CMEs) are typical eruptions in the solar atmosphere, which are determined by the topology and evolution of their source magnetic fields. Thus, study on the magnetic ...
Magnetic flux ropes are key structures in the solar atmosphere, whose eruptions can lead to the formation of solar flares and coronal mass ejections (CMEs), triggering hazardous space weather. Their ...
The solar active region is the primary source for hazardous space weather events such as major flares and coronal mass ejections (CMEs). Tracking the long-term evolution of active regions from ...
Solar active regions (ARs) are the main sources of major flares and CMEs. Therefore,tracking the ARs from their birth until they gain the ability to produce major activitieswill help us to understand ...
根据《中山大学“智慧大气”大气科学拔尖人才培养创新实验区建设实施方案》，现开展中山大学“智慧大气”大气科学拔尖人才培养创新实验区学生的校内遴选工作。 一、实验区简介 ...
大气科学学院2025年“申请-考核”制博士考生综合考核结果公示（如附件所示）。 公示时间：2025年1月26日－2月1日 公示期间，考生若对综合考核结果有异议，请在公示期内署具真实姓名向中山 ...
The upper atmospheres and ionospheres of terrestrial planets, with special focusing on the distribution of ionospheric components of Martian ionosphere vary with the solar radiation and solar wind ...
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