Application of the Tianwen-1 DOR Signals Observed by Very Long Baseline Interferometry Radio Telescopes in the Study of Solar Wind Plasma and a Coronal Mass Ejection

Wang, Zhichao1,2; Ma, Maoli1; Liu, Qinghui1; He, Qingbao3; Zheng, Xin1; Liu, Lijia4; Calves, Guifre Molera5

2023-12-01

10.3847/1538-4365/ad077f

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES   影响因子和分区

0067-0049

1538-4365

The Tianwen-1 (TW1) Mars probe experienced solar conjunction for the first time in 2021. The China VLBI Network (CVN) observes the differential one-way ranging (DOR) signals of TW1 throughout its phase. This paper explores the application of CVN observation data to study the solar wind plasma. First, the frequency and phase of the DOR carrier and sidetones at each station are calculated using the Doppler method. Then, the variations in both the differential phase delays (DPD) and the total electron content (TEC) are calculated using the phase of the sidetones. We also statistically analyze the fluctuations in the Delta-DOR (Delta DOR) group delay. The results indicate that the fluctuations of the frequency, phase, Delta DOR group delay, delay rate, and TEC variations of the TW1 signals increase with the decrease of the heliocentric distance. On 2021 November 2, a coronal mass ejection (CME) passed across the ray paths of the telescope beams, when the heliocentric distance and heliographic latitude of the projected position of Mars were 30.6 Rs and 3 degrees, respectively. Our data catch the impact of the CME on the DOR signals. The change of the DPD reaches 170 ps, which is equivalent to 986 TECU. We utilize the cross correlation to analyze the frequency fluctuations at multiple stations, and obtain the propagation direction and velocity variations of the CME. Our analysis indicates that multifrequency DOR signals observed by very long baseline interferometry stations have great application to characterize the electron density variations and propagation of the solar wind plasma.

SCI

英语

其他

National Natural Science Foundation of China["12273098","11973074","42241118","11803069"]

Astronomy & Astrophysics

Astronomy & Astrophysics

WOS:001115387800001

IOP Publishing Ltd

SPACE SCIENCE

2-s2.0-85180117261

Web of Science

1.Shanghai Astron Observ, 80 Nandan Rd, Shanghai, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen 518055, Peoples R China
4.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing, Peoples R China
5.Univ Tasmania, Private Bag 37, Hobart, Tas 7001, Australia

Wang, Zhichao,Ma, Maoli,Liu, Qinghui,et al. Application of the Tianwen-1 DOR Signals Observed by Very Long Baseline Interferometry Radio Telescopes in the Study of Solar Wind Plasma and a Coronal Mass Ejection[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2023,269(2).

Wang, Zhichao.,Ma, Maoli.,Liu, Qinghui.,He, Qingbao.,Zheng, Xin.,...&Calves, Guifre Molera.(2023).Application of the Tianwen-1 DOR Signals Observed by Very Long Baseline Interferometry Radio Telescopes in the Study of Solar Wind Plasma and a Coronal Mass Ejection.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,269(2).

Wang, Zhichao,et al."Application of the Tianwen-1 DOR Signals Observed by Very Long Baseline Interferometry Radio Telescopes in the Study of Solar Wind Plasma and a Coronal Mass Ejection".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 269.2(2023).