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Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005

Cite as:

Ritter, Patricia (2018): Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005. V. 1.0. GFZ Data Services. http://doi.org/10.5880/GFZ.2.3.2018.007

Status

I   N       R   E   V   I   E   W : Ritter, Patricia (2018): Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005. V. 1.0. GFZ Data Services. http://doi.org/10.5880/GFZ.2.3.2018.007

Abstract

This dataset comprises profiles of Hall ionospheric current densities derived from scalar magnetic field data measured from the CHAMP satellite during six magnetic storms. The Hall currents are intense electric currents that flow horizontally above the earth’s surface in the polar region and perpendicular to the geomagnetic field. They peak at approximately ± 80° of geomagnetic latitude. Together with the field-aligned currents they form part of the ionospheric current system. During enhanced geomagnetic activity the Hall current peak locations are shifted equatorward.

The CHAllenging Minisatellite Payload (CHAMP) spacecraft circled the Earth during the years 2000 – 2010 on a near-polar orbit (inclination 87.3°), each orbit taking 93 minutes at an altitude of initially 455 km. Within 4 months CHAMP covered all local times. The data records used for determining the Hall currents are scalar magnetic field measurements obtained with the Overhauser magnetometer on the satellite boom, with a sample frequency of 1 Hz and a resolution of 0.1 nT.

In order to isolate the magnetic effects of ionospheric currents in the satellite observations, the contributions from all other sources were removed from the scalar field readings. The main, crustal and external magnetic fields were subtracted using the POMME 6 model (Maus et al, 2010, http://www.geomag.us/models/pomme6.html). The Hall current densities were obtained by fitting a line current model to the observed magnetic field residuals. The model consists of a series of 160 horizontal infinite current lines centered at the orbit position closest to the geographic pole, at an altitude of 110 km and separated by 1° in latitude. The magnetic field of the line currents are related to the current strength according to the Biot–Savart law. Assuming a static current, the strength of each current line is derived from an inversion of the observed field residuals applying a least squares fitting approach. This method of Hall current estimation from scalar magnetometer records measured at satellites was proposed initially by Olsen (1996). The reliability of the approach was demonstrated and validated in a statistical study where Hall current density estimates from CHAMP were directly compared with independent determinations from ground observations of the IMAGE magnetometer array (Ritter et al., 2004).

Dataset Contact

  • Ritter, Patricia (Coordinator Dept. 2) ; GFZ German Research Centre for Geosciences, Potsdam, Germany;

Keywords

CHAllenging Minisatellite Payload, CHAMP Satellite, geomagnetic field, ionospheric current system, Hall current, magnetic storm

GCMD Science Keywords

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          • givenName: Patricia
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          • nameIdentifier (nameIdentifierScheme=ORCID): 0000-0002-0926-1771
          • affiliation: GFZ German Research Centre for Geosciences, Potsdam, Germany
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      • publisher: GFZ Data Services
      • publicationYear: 2018
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        • subject: CHAMP Satellite
        • subject: geomagnetic field
        • subject: ionospheric current system
        • subject: Hall current
        • subject: magnetic storm
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          • givenName: Patricia
          • familyName: Ritter
          • nameIdentifier (nameIdentifierScheme=ORCID): 0000-0002-0926-1771
          • affiliation: GFZ German Research Centre for Geosciences, Potsdam, Germany
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      • Entry_Title: Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005
      • Data_Set_Citation
        • Dataset_Creator: Ritter, Patricia
        • Dataset_Title: Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005
        • Dataset_Release_Date: 2018
        • Dataset_Release_Place: Potsdam, Germany
        • Dataset_Publisher: GFZ Data Services
        • Online_Resource: http://dx.doi.org/10.5880/GFZ.2.3.2018.007
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        • Topic: SUN-EARTH INTERACTIONS
        • Term: IONOSPHERE/MAGNETOSPHERE DYNAMICS
        • Variable_Level_1: ELECTRIC FIELDS/ELECTRIC CURRENTS
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        • Topic: SUN-EARTH INTERACTIONS
        • Term: IONOSPHERE/MAGNETOSPHERE DYNAMICS
        • Variable_Level_1: MAGNETIC STORMS
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        • Topic: SOLID EARTH
        • Term: GEOMAGNETISM
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      • Keyword: CHAllenging Minisatellite Payload
      • Keyword: CHAMP Satellite
      • Keyword: geomagnetic field
      • Keyword: ionospheric current system
      • Keyword: Hall current
      • Keyword: magnetic storm
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          • Last_Name: Deutsches GeoForschungsZentrum GFZ
      • Summary
        • Abstract: This dataset comprises profiles of Hall ionospheric current densities derived from scalar magnetic field data measured from the CHAMP satellite during six magnetic storms. The Hall currents are intense electric currents that flow horizontally above the earth’s surface in the polar region and perpendicular to the geomagnetic field. They peak at approximately ± 80° of geomagnetic latitude. Together with the field-aligned currents they form part of the ionospheric current system. During enhanced geomagnetic activity the Hall current peak locations are shifted equatorward. The CHAllenging Minisatellite Payload (CHAMP) spacecraft circled the Earth during the years 2000 – 2010 on a near-polar orbit (inclination 87.3°), each orbit taking 93 minutes at an altitude of initially 455 km. Within 4 months CHAMP covered all local times. The data records used for determining the Hall currents are scalar magnetic field measurements obtained with the Overhauser magnetometer on the satellite boom, with a sample frequency of 1 Hz and a resolution of 0.1 nT. In order to isolate the magnetic effects of ionospheric currents in the satellite observations, the contributions from all other sources were removed from the scalar field readings. The main, crustal and external magnetic fields were subtracted using the POMME 6 model (Maus et al, 2010, http://www.geomag.us/models/pomme6.html). The Hall current densities were obtained by fitting a line current model to the observed magnetic field residuals. The model consists of a series of 160 horizontal infinite current lines centered at the orbit position closest to the geographic pole, at an altitude of 110 km and separated by 1° in latitude. The magnetic field of the line currents are related to the current strength according to the Biot–Savart law. Assuming a static current, the strength of each current line is derived from an inversion of the observed field residuals applying a least squares fitting approach. This method of Hall current estimation from scalar magnetometer records measured at satellites was proposed initially by Olsen (1996). The reliability of the approach was demonstrated and validated in a statistical study where Hall current density estimates from CHAMP were directly compared with independent determinations from ground observations of the IMAGE magnetometer array (Ritter et al., 2004).
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    • resource
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      • creator
        • creatorName: Ritter, Patricia
        • givenName: Patricia
        • familyName: Ritter
        • nameIdentifier (nameIdentifierScheme=ORCID): 0000-0002-0926-1771
        • affiliation: GFZ German Research Centre for Geosciences, Potsdam, Germany

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License: CC BY 4.0

Dataset Description

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