2014
DOI: 10.1007/s11214-014-0105-z
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The CASSIOPE/e-POP Magnetic Field Instrument (MGF)

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… Show more

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Cited by 46 publications
(49 citation statements)
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“…The MGF instrument from the CSA's ePOP payload (Wallis et al, 2006) is the design on which this prototype is based but is not sufficiently radiation tolerant for the OR-BITALS mission.…”
Section: Modern State Of Space Fluxgate Magnetometersmentioning
confidence: 99%
See 1 more Smart Citation
“…The MGF instrument from the CSA's ePOP payload (Wallis et al, 2006) is the design on which this prototype is based but is not sufficiently radiation tolerant for the OR-BITALS mission.…”
Section: Modern State Of Space Fluxgate Magnetometersmentioning
confidence: 99%
“…Narod and Bennest, 1990). The NGL design was previously modified for low-radiation space applications as the magnetic field instrument (MGF) in the CSA's enhanced Polar Outflow Probe (ePOP) payload on the CAScade, Smallsat and IOnospheric Polar Explorer (CAS-SIOPE) satellite (Wallis et al, 2006).…”
Section: Introduction and Applicationmentioning
confidence: 99%
“…In addition to the O + peak, the TOA spectrum in pixel P5 also shows significant ion counts in the NO + TOA range, which may be indicative of the presence of a low flux of NO + ions of 12.2–14.9 eV and/or lower energy N 2 + ions. The observed magnetic field perturbation and electron data [ Wallis et al ., ; Knudsen et al ., ] at this time are indicative of small‐scale structures of field‐aligned current and soft precipitating electrons, respectively, which might suggest auroral ionization of N 2 in the E and/or F region and the subsequent up‐flow and/or charge exchange of the resulting N + and N 2 + ions.…”
Section: Observationmentioning
confidence: 86%
“…The specific materials used in sensor construction are often not provided in instrument publications. However, MACOR is explicitly mentioned or known to be used in the NASA MAGSAT satellite (Acuña et al, 1978); the S100, STE, and PC104 observatory magnetometers developed by Narod Geophysics Ltd. (Narod and Bennest, 1990); both the Canadian CARISMA ground network (Mann et al, 2008) and the US EMScope magnetotelluric network (Schultz, 2009); the Danish Oersted satellite (Nielsen et al, 1995); the miniaturised SMILE instrument (Forslund et al, 2007); the Vector Fluxgate Magnetometer (VMAG) for the Demonstration and Science Experiment program (Moldwin, 2010); a prototype radiation tolerant fluxgate (Miles et al, 2013); and the Canadian Space Agency Cassiope/e-POP satellite (Wallis et al, 2015). Unfortunately, MACOR is expensive, difficult to machine, and brittle.…”
Section: Introductionmentioning
confidence: 99%