Logo image
The CASSIOPE/e-POP Magnetic Field Instrument (MGF)
Journal article   Open access   Peer reviewed

The CASSIOPE/e-POP Magnetic Field Instrument (MGF)

D. D Wallis, D. M Miles, B. B Narod, J. R Bennest, K. R Murphy, I. R Mann and A. W Yau
Space science reviews, Vol.189(1-4), pp.27-39
10/22/2014
DOI: 10.1007/s11214-014-0105-z
url
https://doi.org/10.1007/s11214-014-0105-zView
Published (Version of record) Open Access

Abstract

Field-aligned currents couple energy between the Earth’s magnetosphere and ionosphere and are responsible for driving both micro and macro motions of plasma and neutral atoms in both regimes. These currents are believed to be a contributing energy source for ion acceleration in the polar ionosphere and may be detected via measurements of magnetic gradients along the track of a polar orbiting spacecraft, usually the north-south gradients of the east-west field component. The detection of such gradients does not require observatory class measurements of the geomagnetic field. The Magnetic Field instrument (MGF) measures the local magnetic field onboard the Enhanced Polar Outflow Probe (e-POP) satellite by using two ring-core fluxgate sensors to characterize and remove the stray spacecraft field. The fluxgate sensors have their heritage in the MAGSAT design, are double wound for reduced mass and cross-field dependence, and are mounted on a modest 0.9 m carbon-fiber boom. The MGF samples the magnetic field 160 times per sec (∼50 meters) to a resolution of 0.0625 nT and outputs data at 1952 bytes per second including temperature measurements. Its power consumption is 2.2 watts, and its noise level is 7 pT per root Hz at 1 Hz.
Aerospace Technology and Astronautics Article Astrophysics and Astroparticles Physics Physics and Astronomy Planetology Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics

Details

Metrics

Logo image