The Magnetospheric Multiscale Magnetometers

被引:1073
作者
Russell, C. T. [1 ]
Anderson, B. J. [2 ]
Baumjohann, W. [3 ]
Bromund, K. R. [4 ]
Dearborn, D. [1 ]
Fischer, D. [3 ]
Le, G. [4 ]
Leinweber, H. K. [1 ]
Leneman, D. [1 ]
Magnes, W. [3 ]
Means, J. D. [1 ]
Moldwin, M. B. [5 ]
Nakamura, R. [3 ]
Pierce, D. [6 ]
Plaschke, F. [3 ]
Rowe, K. M. [1 ]
Slavin, J. A. [5 ]
Strangeway, R. J. [1 ]
Torbert, R. [7 ]
Hagen, C. [3 ]
Jernej, I. [3 ]
Valavanoglou, A. [3 ]
Richter, I. [8 ]
机构
[1] Univ Calif Los Angeles, 603 Charles Young Dr, Los Angeles, CA 90095 USA
[2] Johns Hopkins Univ, Appl Phys Lab, 11100 Johns Hopkins Rd, Laurel, MD 20723 USA
[3] Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria
[4] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
[5] Univ Michigan, 1032 Green St, Ann Arbor, MI 48109 USA
[6] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[7] Univ New Hampshire, 105 Main St, Durham, NH 03824 USA
[8] Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, Mendelssohnstr 3, D-38106 Braunschweig, Germany
关键词
Magnetosphere; Reconnection; Magnetometer; MAGNETIC-FIELD GRADIENTS; ACCURATE DETERMINATION; NATURAL CONSTRAINTS; VECTOR MEASUREMENTS;
D O I
10.1007/s11214-014-0057-3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The success of the Magnetospheric Multiscale mission depends on the accurate measurement of the magnetic field on all four spacecraft. To ensure this success, two independently designed and built fluxgate magnetometers were developed, avoiding single-point failures. The magnetometers were dubbed the digital fluxgate (DFG), which uses an ASIC implementation and was supplied by the Space Research Institute of the Austrian Academy of Sciences and the analogue magnetometer (AFG) with a more traditional circuit board design supplied by the University of California, Los Angeles. A stringent magnetic cleanliness program was executed under the supervision of the Johns Hopkins University's Applied Physics Laboratory. To achieve mission objectives, the calibration determined on the ground will be refined in space to ensure all eight magnetometers are precisely inter-calibrated. Near real-time data plays a key role in the transmission of high-resolution observations stored on board so rapid processing of the low-resolution data is required. This article describes these instruments, the magnetic cleanliness program, and the instrument pre-launch calibrations, the planned in-flight calibration program, and the information flow that provides the data on the rapid time scale needed for mission success.
引用
收藏
页码:189 / 256
页数:68
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