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IPS Observation System for Miyun 50m Radio Telescope and Its Acceptance Observation

机译:密云50m射电望远镜Ips观测系统及其验收   意见

摘要

Ground-based observation of Interplanetary Scintillation(IPS) is an importantapproach of monitoring solar wind. A ground-based IPS observation system isnewly implemented on 50m radio telescope, Miyun station, National AstronomicalObservatories, Chinese Academy of Sciences(NAOC). This observation system isconstructed for purpose of observing the solar wind speed and scintillationindex by using the normalized cross-spectrum of simultaneous dual-frequency IPSmeasurement. The system consists of a universal dual-frequency front-end and adual-channel multi-function back-end specially designed for IPS. After carefulcalibration and testing, IPS observations on source 3C273B and 3C279 aresuccessfully carried out. The preliminary observation results show that thisnewly developed observation system is capable of doing IPS observation.Thesystem sensitivity for IPS observation can reach over 0.3Jy in terms of IPSpolarization correlator with 4MHz bandwidth and 2s integration time.
机译:行星际闪烁(IPS)的地面观测是监测太阳风的重要方法。在中国科学院国家天文台密云站50m射电望远镜上新实现了地面IPS观测系统。构造该观测系统的目的是通过同时双频IPS测量的标准化互谱来观测太阳风速和闪烁指数。该系统由专门为IPS设计的通用双频前端和ad-channel多功能后端组成。经过仔细的校准和测试后,成功地在源3C273B和3C279上进行了IPS观察。初步的观测结果表明,该新型观测系统能够进行IPS观测。就IPS偏振相关器而言,IPS观测的系统灵敏度可以达到0.3Jy以上,带宽为4MHz,积分时间为2s。

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