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On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory

机译:太阳动力学天文台上的日震和磁成像仪的在轨性能

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摘要

The Helioseismic and Magnetic Imager (HMI) instrument is a major component of NASA's Solar Dynamics Observatory (SDO) spacecraft. Since commencement of full regular science operations on 1 May 2010, HMI has operated with remarkable continuity, e.g. during the more than five years of the SDO prime mission that ended 30 September 2015, HMI collected 98.4% of all possible 45-second velocity maps; minimizing gaps in these full-disk Dopplergrams is crucial for helioseismology. HMI velocity, intensity, and magnetic-field measurements are used in numerous investigations, so understanding the quality of the data is important. This article describes the calibration measurements used to track the performance of the HMI instrument, and it details trends in important instrument parameters during the prime mission. Regular calibration sequences provide information used to improve and update the calibration of HMI data. The set-point temperature of the instrument front window and optical bench is adjusted regularly to maintain instrument focus, and changes in the temperature-control scheme have been made to improve stability in the observable quantities. The exposure time has been changed to compensate for a 20% decrease in instrument throughput. Measurements of the performance of the shutter and tuning mechanisms show that they are aging as expected and continue to perform according to specification. Parameters of the tunable optical-filter elements are regularly adjusted to account for drifts in the central wavelength. Frequent measurements of changing CCD-camera characteristics, such as gain and flat field, are used to calibrate the observations. Infrequent expected events such as eclipses, transits, and spacecraft off-points interrupt regular instrument operations and provide the opportunity to perform additional calibration. Onboard instrument anomalies are rare and seem to occur quite uniformly in time. The instrument continues to perform very well.
机译:日震和磁成像仪(HMI)仪器是NASA太阳动力学天文台(SDO)航天器的主要组件。自2010年5月1日全面进行常规科学运作以来,HMI的运作具有显着的连续性,例如,在截至2015年9月30日的SDO首要任务超过五年的时间内,HMI收集了所有可能的45秒速度图的98.4%;最小化这些全磁盘多普勒图中的间隙对于肝病学至关重要。 HMI速度,强度和磁场测量被用于许多研究中,因此了解数据质量非常重要。本文介绍了用于跟踪HMI仪器性能的校准测量,并详细介绍了主要任务期间重要仪器参数的趋势。定期校准序列提供了用于改善和更新HMI数据校准的信息。定期调节仪器前窗和光学平台的设定点温度,以保持仪器聚焦,并已更改温度控制方案,以提高可观察量的稳定性。更改了曝光时间,以补偿仪器吞吐量降低20%的情况。百叶窗和调谐机构性能的测量结果表明,它们已按预期老化,并继续按照规格运行。定期调整可调谐滤光器元件的参数,以解决中心波长的漂移问题。经常测量不断变化的CCD相机特性(例如增益和平坦场)来校准观测值。诸如日食,过境和航天器偏航点之类的偶发事件会中断常规的仪器操作,并提供执行额外校准的机会。机载仪器异常非常罕见,并且似乎在时间上相当均匀地发生。仪器继续表现良好。

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