1. Vertical Structural Evolution of Ionospheric Holes Triggered by Rocket Launches Observed by the Sanya Incoherent Scatter Radar.
- Author
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Zhao, Linxuan, Ding, Feng, Yue, Xinan, Xu, Su, Wang, Junyi, Cai, Yihui, Li, Mingyuan, Zhang, Ning, Zhou, Xu, Wang, Yonghui, Li, Jianyong, Mao, Tian, Song, Qian, Xiong, Bo, Li, Xiaolin, and Luo, Junhao
- Subjects
GLOBAL Positioning System ,PLASMA chemistry ,PLASMA transport processes ,INCOHERENT scattering ,ROCKET launching - Abstract
This article presents observational results of the vertical structural evolution of ionospheric holes during two rocket launches. A combination of observations from the newly built Sanya incoherent scatter radar (SYISR) and Global Navigation Satellite System networks was employed. The vertical structural evolution of two rocket‐induced ionospheric holes over the SYISR could be divided into three stages. Firstly, 10–11 min after launch, the holes initially appeared in the topside ionosphere. Then, the holes expanded rapidly toward higher and lower altitudes. At ∼30 min after launch, the holes extended to an altitudinal range of ∼200 km to over 700 km. The maximum depletion altitude was 425 km for the afternoon event and 283 km for the midnight event. Finally, the holes recovered slowly, with faster recovery at higher altitudes. Our work contributes to further understanding the vertical structural evolutionary mechanisms of the ionospheric holes and relevant ionospheric processes. Plain Language Summary: When rockets fly in the ionosphere, numerous H2O or H2 molecules in the rocket exhaust rapidly react with the O+ in the background ionosphere and produce positive ions, which then react with electrons and lead to a large electron depletion known as ionospheric holes. The vertical structure of these holes has rarely been observed before. In this study, we observed the full vertical profile and the complete vertical structural evolution of two rocket‐induced ionospheric holes, using the newly built Sanya incoherent scatter radar (SYISR), combined with the Global Navigation Satellite System networks for their horizontal features. These two ionospheric holes occurred in the afternoon and around midnight in local time, with maximum electron depletion of 15% and 83% relative to the background ionosphere, and altitudinal distribution of 255–775 km and 202–535 km over SYISR, respectively. The vertical structural evolution of the holes displays the vertical variations of ionospheric characteristics and crucial ionospheric processes like plasma transport and chemistry. Our study contributes to a deeper understanding of the dynamics process of ionospheric holes as an artificial space weather process, which is of potential significance for monitoring space objects such as rockets. Key Points: Observations of the full vertical profile of the rocket‐induced ionospheric holes were presentedThe holes first appeared in topside ionosphere and then expanded both upwards and downwards to an altitude range of ∼200–∼700 kmThe recovery of electron density is faster for the midnight hole than the daytime one and is faster at high altitude than at low altitude [ABSTRACT FROM AUTHOR]
- Published
- 2024
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