Figure 2 from VLBI Data Processing on Coronal Radio-sounding Experiments of Mars Express

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VLBI Data Processing on Coronal Radio-sounding Experiments of Mars Express

Authors: Maoli Ma*, Guifré Molera Calvés, Giuseppe Cimò, Peijin Zhang, Ming Xiong, Peijia Li, Pradyumna Kummamuru, Zhanghu Chu, Tianyu Jiang, Bo Xia, Kondo Tetsuro, Fengxian Tong, Pablo de Vicente, Jonathan Quick, Hua Zhang, and Zhong Chen

2021 The Astronomical Journal 162 141.

Provider: AAS Journals

Caption: Figure 2.

Power spectra of frequency fluctuation at different solar offsets. The spectra at 4.9–69.9 R_s have a near-power-law shape close to that of the Kolmogorov spectrum in a frequency range [ν_lo, ν_up]. The noise dominates the spectra when ν > ν_up. Data from 2017 July 29 and August 3 were obtained by the local correlation. The PRIDE approach was used on all the rest.

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