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The Magnetospheric Multiscale Magnetometers

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TLDR
To achieve mission objectives, the calibration determined on the ground will be refined in space to ensure all eight magnetometers are precisely inter-calibrated, and the information flow that provides the data on the rapid time scale needed for mission success is described.
Abstract
The success of the Magnetospheric Multiscale mission depends on the accurate measurement of the magnetic field on all four spacecraft. To ensure this success, two independently designed and built fluxgate magnetometers were developed, avoiding single-point failures. The magnetometers were dubbed the digital fluxgate (DFG), which uses an ASIC implementation and was supplied by the Space Research Institute of the Austrian Academy of Sciences and the analogue magnetometer (AFG) with a more traditional circuit board design supplied by the University of California, Los Angeles. A stringent magnetic cleanliness program was executed under the supervision of the Johns Hopkins University’s Applied Physics Laboratory. To achieve mission objectives, the calibration determined on the ground will be refined in space to ensure all eight magnetometers are precisely inter-calibrated. Near real-time data plays a key role in the transmission of high-resolution observations stored on board so rapid processing of the low-resolution data is required. This article describes these instruments, the magnetic cleanliness program, and the instrument pre-launch calibrations, the planned in-flight calibration program, and the information flow that provides the data on the rapid time scale needed for mission success.

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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.
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The ERG Science Center

TL;DR: The Exploration of energization and radiation in Geospace (ERG) Science Center serves as a hub of the ERG project, providing data files in a common format and developing the space physics environment data analysis software and plug-ins for data analysis as mentioned in this paper.
References
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Journal ArticleDOI

Interplanetary Magnetic Field and the Auroral Zones

TL;DR: In this article, it was found that a model with a southward interplanetary magnetic field leads to a natural explanation of the SD currents and speculative aspects of the problem as they appear at this time are discussed.
Journal ArticleDOI

Satellite studies of magnetospheric substorms on August 15, 1968: 9. Phenomenological model for substorms

TL;DR: In this paper, the authors present a phenomenological model of the magnetospheric substorm sequence, which can be divided into three main phases: the growth phase, the expansion phase, and the recovery phase.
Journal Article

Satellite studies of magnetospheric substorms on August 15, 1968. IX - Phenomenological model for substorms.

TL;DR: In this article, observations made during three substorms on August 15, 1968, are shown to be consistent with current theoretical ideas about the cause of substorm, and the phenomenological model described in several preceding papers is further expanded.
Journal ArticleDOI

Plasma acceleration at the earth's magnetopause - Evidence for reconnection

TL;DR: In this paper, high-speed plasma at the magnetopause in agreement with theoretical predictions of magnetic field reconnection is reported, and the observations agree with the predictions of the reconnection model of the dayside magnetopsause, in which the magnetic field is described as a rotational discontinuity, or a large-amplitude Alfven wave.
Journal ArticleDOI

The solar flare phenomenon and the theory of reconnection and annihilation of magnetic fields

TL;DR: In this paper, a systematic study of the theoretical mechanisms for diffusion, reconnection, and annihilation of magnetic fields is presented, and it is shown that there is no reason to expect runaway electrons and no effective instability unless the fields are exactly antiparallel.
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