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The Search-Coil Magnetometer for MMS

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TLDR
The tri-axial search-coil magnetometer (SCM) belongs to the FIELDS instrumentation suite on the Magnetospheric Multiscale (MMS) mission as discussed by the authors.
Abstract
The tri-axial search-coil magnetometer (SCM) belongs to the FIELDS instrumentation suite on the Magnetospheric Multiscale (MMS) mission (Torbert et al. in Space Sci. Rev. (2014), this issue). It provides the three magnetic components of the waves from 1 Hz to 6 kHz in particular in the key regions of the Earth’s magnetosphere namely the subsolar region and the magnetotail. Magnetospheric plasmas being collisionless, such a measurement is crucial as the electromagnetic waves are thought to provide a way to ensure the conversion from magnetic to thermal and kinetic energies allowing local or global reconfigurations of the Earth’s magnetic field. The analog waveforms provided by the SCM are digitized and processed inside the digital signal processor (DSP), within the Central Electronics Box (CEB), together with the electric field data provided by the spin-plane double probe (SDP) and the axial double probe (ADP). On-board calibration signal provided by DSP allows the verification of the SCM transfer function once per orbit. Magnetic waveforms and on-board spectra computed by DSP are available at different time resolution depending on the selected mode. The SCM design is described in details as well as the different steps of the ground and in-flight calibrations.

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Citations
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Journal ArticleDOI

Magnetospheric Multiscale Overview and Science Objectives

TL;DR: Magnetospheric multiscale (MMS) as mentioned in this paper is a NASA four-spacecraft constellation mission to investigate magnetic reconnection in the boundary regions of the Earth's magnetosphere.
Journal ArticleDOI

The Axial Double Probe and Fields Signal Processing for the MMS Mission

TL;DR: The axial double probe (ADP) instrument on the magnetospheric multiscale (MMS) spacecraft has been used to measure DC electric field with a precision of ∼ 1.1mV/m, a resolution of ∼ 25μV/μ, and a range of ∼±1 V/m in most of the plasma environments MMS will encounter.
Journal ArticleDOI

Nature of Kinetic Scale Turbulence in the Earth's Magnetosheath

TL;DR: In this article, a combined observational and theoretical analysis is presented to investigate the nature of plasma turbulence at kinetic scales in the Earth's magnetosheath, which is similar to that in the upstream solar wind: predominantly anisotropic, lowfrequency and kinetic Alfven in nature.
References
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Journal ArticleDOI

Demagnetizing Factors of the General Ellipsoid

J. A. Osborn
- 01 Jun 1945 - 
TL;DR: In this paper, the demagnetizing factors of ellipsoids of three different axes are presented, along with supplementary formulas which cover a large number of special cases of ellipses.
Journal ArticleDOI

Geospace Environmental Modeling (GEM) magnetic reconnection challenge

TL;DR: In this paper, a simple Harris sheet configuration with a specified set of initial conditions, including a finite amplitude, magnetic island perturbation to trigger the dynamics of magnetic reconnection is studied.
Journal ArticleDOI

Transport of solar wind into Earth's magnetosphere through rolled-up Kelvin–Helmholtz vortices

TL;DR: It is shown that during northward solar-wind magnetic field conditions—in the absence of active reconnection at low latitudes—there is aSolar-wind transport mechanism associated with the nonlinear phase of the Kelvin–Helmholtz instability that can supply plasma sources for various space weather phenomena.
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Current disruption in the Earth's magnetosphere: Observations and models

TL;DR: In this paper, the cross-tail current sheet shows a rapid growth in the current density, a large upsurge in the duskward ion bulk speed to nearly the ion thermal speed, an increase in the plasma pressure and its isotropy, a rise in the ion beta, and a decrease in the thickness of the current sheet to a length scale comparable to the thermal ion gyroradius.
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