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First Light for the New 30 m Parabolic Radio Telescope at ArQi: Implications for Space Weather Monitoring

  • Authors: Ming Xiong, 明 熊, Wei Wang, 威 王, Cang Su, 仓 苏, Jin Fan, 瑾 范, Junhui Peng, 俊晖 彭, Jun Cheng, 俊 程, Yanchen Gao, 炎琛 高, Man Zhang, 嫚 张, Yongzhi Ye, 永志 叶, Zhijun Chen, 志军 陈, Zhichao Zhou, 志超 周, Sha Li, 沙 李, Xinhua Zhao, 新华 赵, Liping Yang, 利平 杨, Chengming Tan, 程明 谭, Wenshuai Cheng, 文帅 程, Xueshang Feng, 学尚 冯, Yihua Yan, 毅华 颜

Ming Xiong et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 3.

(a) off-source and (b) on-source profiles of power spectrum density for the vertically and horizontally polarized emissions from 3C446. One dashed black line with an inverse power denotes the 1/f noise associated with the off-source measurement. An animation of spectral profiles during the whole 5 minute transit of 3C446 is provided in the online Journal.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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