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Wind Magnetic Field Investigation

ResourceID
spase://SMWG/Instrument/Wind/MFI

Description

The magnetic field experiment on Wind provides data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the mission, and, where appropriate, relate them to the statics and dynamics of the magnetosphere. The basic instrument of the Magnetic Field Investigation (MFI) on the Wind Spacecraft is a boom-mounted dual triaxial fluxgate magnetometer and associated electronics. The dual configuration provides redudancy and also permits accurate removal of the dipolar portion of the spacecraft magnetic field. The instrument provides:

        * (1) near real-time data at nominally one vector per 92 s as key paramter data for broad dissemination,
        * (2) rapid data at 10.9 vectors/s for standard analysis,
        * (3) occasionally, snapshot (SS) memory data and Fast Fourier Transform data (FFT), both based on 44 vectors/s.

        These measurements are precise (0.025%), accurate, ultra-sensitive (0.008 nT/step quantization), and where the sensor noise level is <0.006 nT r.m.s for 0-10 Hz. The digital processing unit utilizes a 12-bit microprocessor controlled analogue-to-digital converter. The instrument features a very wide dynamic range of measurement capability, from 4 nT up to 65 536 nT per axis in eight discrete ranges. (The upper range permits complete testing in the Earth's field.) In the FFT mode power spectral density elements are transmitted to the ground as fast as once every 23 s (high rate), and 2.7 min of SS memory time series data, triggered automatically by pre-set command, requires typically about 5.1 hours for transmission. Standard data products are the following vector field averages: 0.0226 s (detail data from SS), 0.092 s ('detail' in standard mode), 3 s, 1 min, and 1 hour, in both GSE and GSM coordinates, as well as the FFT spectral elements. High instrument reliability is obtained by the use of fully redundant systems and extremely conservative designs.

        The instrument was turned on on 1994-11-12.

        References: Lepping, R. P., et al., The Wind Magnetic Field Investigation, Space Science Reviews, 71, 207-229, 1995.

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Details

Version:2.0.1

Instrument

ResourceID
spase://SMWG/Instrument/Wind/MFI
ResourceHeader
ResourceName
Wind Magnetic Field Investigation
AlternateName
Wind MFI
ReleaseDate
2021-04-08 16:50:08Z
Description

The magnetic field experiment on Wind provides data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the mission, and, where appropriate, relate them to the statics and dynamics of the magnetosphere. The basic instrument of the Magnetic Field Investigation (MFI) on the Wind Spacecraft is a boom-mounted dual triaxial fluxgate magnetometer and associated electronics. The dual configuration provides redudancy and also permits accurate removal of the dipolar portion of the spacecraft magnetic field. The instrument provides:

        * (1) near real-time data at nominally one vector per 92 s as key paramter data for broad dissemination,
        * (2) rapid data at 10.9 vectors/s for standard analysis,
        * (3) occasionally, snapshot (SS) memory data and Fast Fourier Transform data (FFT), both based on 44 vectors/s.

        These measurements are precise (0.025%), accurate, ultra-sensitive (0.008 nT/step quantization), and where the sensor noise level is <0.006 nT r.m.s for 0-10 Hz. The digital processing unit utilizes a 12-bit microprocessor controlled analogue-to-digital converter. The instrument features a very wide dynamic range of measurement capability, from 4 nT up to 65 536 nT per axis in eight discrete ranges. (The upper range permits complete testing in the Earth's field.) In the FFT mode power spectral density elements are transmitted to the ground as fast as once every 23 s (high rate), and 2.7 min of SS memory time series data, triggered automatically by pre-set command, requires typically about 5.1 hours for transmission. Standard data products are the following vector field averages: 0.0226 s (detail data from SS), 0.092 s ('detail' in standard mode), 3 s, 1 min, and 1 hour, in both GSE and GSM coordinates, as well as the FFT spectral elements. High instrument reliability is obtained by the use of fully redundant systems and extremely conservative designs.

        The instrument was turned on on 1994-11-12.

        References: Lepping, R. P., et al., The Wind Magnetic Field Investigation, Space Science Reviews, 71, 207-229, 1995.
Acknowledgement
User will acknowledge the Wind MFI instrument team in any publication resulting from the use of these data.
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Andriy.Koval
InformationURL
Name
Wind Magnetic Field Investigation (MFI) Paper
URL
Description

The Space Science Reviews paper describing Wind Magnetic Field Investigation (MFI).

InformationURL
Name
NSSDC's Master Catalog
URL
Description

Information about the Magnetic Field Investigation (MFI) experiment on the Wind mission.

InstrumentType
Magnetometer
InvestigationName
Magnetic Field Investigation
ObservatoryID