The First Scientific Flight and Observations of the 50 mm Balloon-borne White-light Coronagraph

Abstract A 50 mm balloon-borne white-light coronagraph (BBWLC) to observe white-light solar corona over the altitude range from 1.08 R ⊙ to 1.50 R ⊙ has recently been indigenously developed by Yunnan Observatories in collaboration with Shandong University (in Weihai) and Changchun Institute of Optics, Fine Mechanics and Physics, which will significantly improve the ability of China to detect and measure the inner corona. On 2022 October 4, its first scientific flight took place at the Dachaidan area in Qinghai province of China. We briefly describe the BBWLC mission including its optical design, mechanical structure, pointing system, the first flight and results associated with the data processing approach. Preliminary analysis of the data shows that BBWLC imaged the K-corona with three streamer structures on the west limb of the Sun. To further confirm the coronal signals obtained by BBWLC, comparisons were made with observations of the K-coronagraph of the High Altitude Observatory and the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. We conclude that BBWLC eventually observed the white-light corona in its first scientific flight.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2025-09-25
DOI
https://doi.org/10.1088/1674-4527/ae0bb2
Primary Topic
History and Developments in Astronomy
Type
article
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The First Scientific Flight and Observations of the 50 mm Balloon-borne White-light Coronagraph

Jujia Zhang, Min Huang, Dayang Liu, Guangqian Liu et al.
Research in Astronomy and Astrophysics
History and Developments in Astronomy
article

The First Scientific Flight and Observations of the 50 mm Balloon-borne White-light Coronagraph

Jujia Zhang, Min Huang, Dayang Liu, Guangqian Liu, Tengfei Song, Mingzhe Sun, Yu Liu, Xianyong Bai, Jingyue Wang, Lidong Xia, K. Kang, Xuefei Zhang, Jun Lin, Yan Li, Zhenyu Liu, Mingyu Zhao
article en

Abstract

Abstract A 50 mm balloon-borne white-light coronagraph (BBWLC) to observe white-light solar corona over the altitude range from 1.08 R ⊙ to 1.50 R ⊙ has recently been indigenously developed by Yunnan Observatories in collaboration with Shandong University (in Weihai) and Changchun Institute of Optics, Fine Mechanics and Physics, which will significantly improve the ability of China to detect and measure the inner corona. On 2022 October 4, its first scientific flight took place at the Dachaidan area in Qinghai province of China. We briefly describe the BBWLC mission including its optical design, mechanical structure, pointing system, the first flight and results associated with the data processing approach. Preliminary analysis of the data shows that BBWLC imaged the K-corona with three streamer structures on the west limb of the Sun. To further confirm the coronal signals obtained by BBWLC, comparisons were made with observations of the K-coronagraph of the High Altitude Observatory and the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. We conclude that BBWLC eventually observed the white-light corona in its first scientific flight.

Research in Astronomy and AstrophysicsVol. 25(12)
Kunming University of Science and Technology (CN), Shandong University (CN), Chinese Academy of Sciences (CN), Yunnan Observatories (CN), Aerospace Information Research Institute (CN), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), Southwest Jiaotong University (CN)
Openalex Percentile: Top 82%
History and Developments in Astronomy
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