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Tesseract - a high-stability, low-noise fluxgate sensor designed for constellation applications
Journal article   Open access   Peer reviewed

Tesseract - a high-stability, low-noise fluxgate sensor designed for constellation applications

Kenton Greene, Christian Hansen, B. Barry Narod, Richard Dvorsky and David M. Miles
Geoscientific instrumentation, methods and data systems, Vol.11(2), pp.307-321
08/23/2022
DOI: 10.5194/gi-11-307-2022
url
https://doi.org/10.5194/gi-11-307-2022View
Published (Version of record) Open Access

Abstract

Accurate high-precision magnetic field measurements are a significant challenge for many applications, including constellation missions studying space plasmas. Instrument stability and orthogonality are essential to enable meaningful comparison between disparate satellites in a constellation without extensive cross-calibration efforts. Here we describe the design and characterization of Tesseract - a fluxgate magnetometer sensor designed for low-noise, high-stability constellation applications. Tesseract's design takes advantage of recent developments in the manufacturing of custom low-noise fluxgate cores. Six of these custom racetrack fluxgate cores are securely and compactly mounted within a single solid three-axis symmetric base. Tesseract's feedback windings are configured as a four-square Merritt coil to create a large homogenous magnetic null inside the sensor where the fluxgate cores are held in a near-zero field, regardless of the ambient magnetic field, to improve the reliability of the core magnetization cycle. A Biot-Savart simulation is used to optimize the homogeneity of the field generated by the feedback Merritt coils and was verified experimentally to be homogeneous within 0.42 % along the racetrack cores' axes. The thermal stability of the sensor's feedback windings is measured using an insulated container filled with dry ice inside a coil system. The sensitivity over temperature of the feedback windings is found to be between 13 and 17 ppm degrees C-1. The sensor's three axes maintain orthogonality to within at most 0.015 degrees over a temperature range of -45 to 20 degrees C. Tesseract's cores achieve a magnetic noise floor of 5 pT root Hz(-1) at 1 Hz. Tesseract will be flight demonstrated on the ACES-II sounding rockets, currently scheduled to launch in late 2022 and again aboard the TRACERS satellite mission as part of the MAGIC technology demonstration which is currently scheduled to launch in 2023.
Geology Geosciences, Multidisciplinary Meteorology & Atmospheric Sciences Physical Sciences Science & Technology

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