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介绍了成像式宇宙噪声接收机在中山站的部署，分析了首批观测数据，得出中山站区宇宙噪声静日曲线。分析表明，观测期间中山站区的宇宙噪声吸收事件夜间与白天显著不同。在夜间，吸收事件呈脉冲式，持续时间为数分钟，吸收区域常在站区北侧出现，沿东西方向伸展；在磁中午附近，吸收事件持续时间在１小时以上，吸收区域南北侧较强，中央较弱。可以认为，夜间吸收区域对应着极光带，其吸收由极光粒子沉降引起；在磁中午，吸收区域对应着极隙区，其吸收可能与极隙区粒子沉降和对流有关。
The deployment of imaging cosmic noise receiver at Zhongshan Station is introduced. The first observations are analyzed and the static curve of cosmic noise at Zhongshan Station is obtained. Analysis shows that during the observation period, the events of cosmic noise absorption in Zhongshan Station area are significantly different at night and daytime. In the night, the absorption event is pulsed, and the duration is several minutes. The absorption area often appears on the north side of the station area and extends along the east-west direction. In the vicinity of noon, the absorption event lasts over 1 hour, Central weak. It can be considered that the absorption area at night corresponds to the auroral zone, and the absorption is caused by the deposition of aurora particles. At noon, the absorption area corresponds to the polar gap and its absorption may be related to the particle settlement and convection in the polar gap.