Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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 1.

Power density spectra (PSD) of Mars Express (MEX) and Tianwen-1 (TIW) at Ys station at 08:30 on October 9. (I) MEX. (II) TIW and the dynamic signal model. The main carrier of TIW is obscured by the noise. (III) Recovering of the signal of TIW with local correlation.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse