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Detecting the Oscillation and Propagation of the Nascent Dynamic Solar Wind Structure at 2.6 Solar Radii Using Very Long Baseline Interferometry Radio Telescopes

  • Authors: Maoli Ma, Guifré Molera Calvés, Giuseppe Cimò, Ming Xiong, Peijia Li, Jing Kong, Peijin Zhang, Jiansen He, Lijia Liu, Pradyumna Kummamuru, Chuanpeng Hou, Jasper Edwards, Qinghui Liu, Zhong Chen, Zhanghu Chu, De Wu, Xu Zhao, Zhichao Wang, Songtao Han, Quanquan Zhi, Yingkai Liu, Jonathan Quick, Javier González, Cristina García Miró, Mikhail Kharinov, Andrey Mikhailov, Alexander Neidhardt, Tiziana Venturi, Marco Morsiani, Giuseppe Maccaferri, Bo Xia, Hua Zhang, Longfei Hao

Maoli Ma et al 2022 The Astrophysical Journal Letters 940 .

  • Provider: AAS Journals

Caption: Figure 9.

The geometric diagrams of P points in the sky plane on October 9. The distances are marked at UTC 11:00. P Yg,MEX is the P point closest to the Sun from the LOS between MEX and Yg. Other P points are the closest point to the Sun from TIW to the antennas.

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