supported by Strategic Priority Research Program of the Chinese Academy of Sciences No. XDB0560000;National Key R&D Program of China No. 2022YFF0503804;NSFC grants 11933009, 12273107, U2031141 and 12073073;grants associated with the Yunling Scholar Project of Yunnan Province;the Yunnan Province Scientist Workshop of Solar Physics;the Yunnan Key Laboratory of Solar Physics and Space Exploration of Code 202205AG070009;the Special Project for the construction of science and technology innovation centers faced to South Asiaand Southeast Asia-Yunnan International Joint Innovation Platform: “China-Malaysia HF-VHF Advanced Radio Astronomy Technology International Joint Laboratory of Yunnan” (202303AP140003);the support by grants associated with the Yunnan Revitalization Talent Support Program;the Foundation of the Chinese Academy of Sciences (Light of West China Program)。
The propagation of disturbances in the solar atmosphere is inherently three-dimensional(3D), yet comprehensive studies on the spatial structure and dynamics of 3D wave fronts are scarce. Here we conduct high-resolutio...