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电离层连接探测器的离子速度测量

Ion Velocity Measurements for the Ionospheric Connections Explorer.

作者信息

Heelis R A, Stoneback R A, Perdue M D, Depew M D, Morgan W A, Mankey M W, Lippincott C R, Harmon L L, Holt B J

出版信息

Space Sci Rev. 2017 Oct;212(1-2):615-629. doi: 10.1007/s11214-017-0383-3. Epub 2017 Jul 20.

Abstract

The Ionospheric Connections Explorer (ICON) payload includes an Ion Velocity Meter (IVM) to provide measurements of the ion drift motions, density, temperature and major ion composition at the satellite altitude near 575 km. The primary measurement goal for the IVM is to provide the meridional ion drift perpendicular to the magnetic meridian with an accuracy of 7.5 ms for all daytime conditions encountered by the spacecraft within 15° of the magnetic equator. The IVM will derive this parameter utilizing two sensors, a retarding potential analyzer (RPA) and an ion drift meter (IDM) that have a robust and successful flight heritage. The IVM described here incorporates improvements in the design and operation to produce the most sensitive device that has been fielded to date. It will specify the ion drift vector, from which the component perpendicular to the magnetic field will be derived. In addition it will specify the total ion density, the ion temperature and the fractional ion composition. These data will be used in conjunction with measurements from the other ICON instruments to uncover the important connections between the dynamics of the neutral atmosphere and the ionosphere through the generation of dynamo currents perpendicular to the magnetic field and collisional forces parallel to the magnetic field. Here the configuration and operation of the IVM instrument are described as well as the procedures by which the ion drift velocity is determined. A description of the subsystem characteristics, which allow a determination of the expected uncertainties in the derived parameters, is also given.

摘要

电离层连接探测器(ICON)的有效载荷包括一个离子速度计(IVM),用于测量卫星在近575公里高度处的离子漂移运动、密度、温度和主要离子成分。IVM的主要测量目标是在航天器在磁赤道15°范围内遇到的所有白天条件下,以7.5米/秒的精度提供垂直于磁子午线的子午向离子漂移。IVM将利用两个传感器——一个减速电位分析仪(RPA)和一个离子漂移计(IDM)来推导这个参数,这两个传感器都有可靠且成功的飞行记录。这里描述的IVM在设计和操作上进行了改进,以制造出迄今为止投入使用的最灵敏的设备,并将确定离子漂移矢量,由此推导出垂直于磁场的分量。此外,它还将确定总离子密度、离子温度和离子成分分数。这些数据将与ICON其他仪器的测量数据结合使用,通过产生垂直于磁场的发电机电流和平行于磁场的碰撞力,揭示中性大气动力学与电离层之间的重要联系。本文描述了IVM仪器的配置和操作,以及确定离子漂移速度的程序。还给出了子系统特性的描述,这些特性有助于确定推导参数中预期的不确定性。

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