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The fluxgate magnetometer of the Low Orbit Pearl Satellites (LOPS): overview of in-flight performance and initial results
The Low Orbit Pearl Satellite series consists of six constellations, with each constellation consisting of three identical microsatellites that line up just like a string of pearls. The first constellation of three satellites were launched on 29 September 2017, with an inclination of ∼ 35.5∘ and ∼ 6...
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Published in: | Geoscientific instrumentation, methods and data systems methods and data systems, 2021-09, Vol.10 (2), p.227-243 |
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Main Authors: | , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The Low Orbit Pearl Satellite series consists of six
constellations, with each constellation consisting of three identical
microsatellites that line up just like a string of pearls. The first
constellation of three satellites were launched on 29 September 2017, with
an inclination of ∼ 35.5∘ and ∼ 600 km
altitude. Each satellite is equipped with three identical fluxgate
magnetometers that measure the in situ magnetic field and its low-frequency fluctuations in the Earth's low-altitude orbit. The triple sensor
configuration enables separation of stray field effects generated by the
spacecraft from the ambient magnetic field (e.g., Zhang et al., 2006). This
paper gives a general description of the magnetometer including the instrument
design, calibration before launch, in-flight calibration, in-flight performance, and initial results. Unprecedented spatial coverage
resolution of the magnetic field measurements allow for the investigation of the
dynamic processes and electric currents of the ionosphere and magnetosphere,
especially for the ring current and equatorial electrojet during both
quiet geomagnetic conditions and storms. Magnetic field measurements from LOPS could be important for studying
the method to separate their contributions of the Magnetosphere-Ionosphere (M-I) current system. |
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ISSN: | 2193-0864 2193-0856 2193-0864 |
DOI: | 10.5194/gi-10-227-2021 |