TERRAPUB Earth, Planets and Space
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Earth Planets Space, Vol. 65 (No. 11), pp. 1271-1283, 2013
doi:10.5047/eps.2013.08.006

Swarm SCARF Dedicated Ionospheric Field Inversion chain

Arnaud Chulliat, Pierre Vigneron, Erwan Thébault, Olivier Sirol, and Gauthier Hulot

Equipe de Géomagnétisme, Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS, F-75005 Paris, France

(Received April 2, 2013; Revised August 25, 2013; Accepted August 26, 2013; Online published November 22, 2013)

Abstract: The geomagnetic daily variation at mid-to-low latitudes, referred to as the geomagnetic Sq field, is generated by electrical currents within the conducting layers of the ionosphere on the dayside of the Earth. It is enhanced in a narrow equatorial band, due to the equatorial electrojet. The upcoming ESA Swarm satellite mission, to be launched end of 2013, will consist of three satellites in low-Earth orbit, providing a dense spatial and temporal coverage of the ionospheric Sq field. A Satellite Constellation Application and Research Facility (SCARF) has been set up by a consortium of research institutions, aiming at producing various level-2 data products during the Swarm mission. The Dedicated Ionospheric Field Inversion (DIFI) chain is a SCARF algorithm calculating global, spherical harmonic models of the Sq field at quiet times. It describes seasonal and solar cycle variations, separates primary and induced magnetic fields based upon advanced 3D-models of the mantle electrical conductivity, and relies on core, lithospheric and magnetospheric field models derived from other SCARF algorithms for removing non-ionospheric fields from the data. The DIFI chain was thoroughly tested on synthetic data during the SCARF preparation phase; it is now ready to be used for deriving models from real Swarm data.
Key words: Swarm, ionosphere, inversion, geomagnetism, space magnetometry.


Corresponding author E-mail: chulliat@ipgp.fr


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