2018-11-17T00:54:04Zhttp://doidb.wdc-terra.org/oaip/oaioai:doidb.wdc-terra.org:65792018-11-02T15:40:19ZDOIDBDOIDB.GFZ
10.5880/GFZ.2.3.2018.007
Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005
Ritter, Patricia
Hall current densities derived from CHAMP scalar magnetic field data during six magnetic storms 2003 and 2005
2018
Potsdam, Germany
GFZ Data Services
http://dx.doi.org/10.5880/GFZ.2.3.2018.007
EARTH SCIENCE
SUN-EARTH INTERACTIONS
IONOSPHERE/MAGNETOSPHERE DYNAMICS
ELECTRIC FIELDS/ELECTRIC CURRENTS
EARTH SCIENCE
SUN-EARTH INTERACTIONS
IONOSPHERE/MAGNETOSPHERE DYNAMICS
MAGNETIC STORMS
EARTH SCIENCE
SOLID EARTH
GEOMAGNETISM
MAGNETIC FIELD
geoscientificInformation
CHAllenging Minisatellite Payload
CHAMP Satellite
geomagnetic field
ionospheric current system
Hall current
magnetic storm
Deutsches GeoForschungsZentrum GFZ
GFZ
DATA CENTER CONTACT
Deutsches GeoForschungsZentrum GFZ
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).
DIF
9.8.2