Magnetic signatures of equatorial spread F as observed by the CHAMP satellite

By Claudia Stolle, Hermann Lühr, Martin K. A. Rother, G. Balasis. 2006

235 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e80b62288984b733b095cc01a31a785b350f1e28

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Citations in the corpus

On monthly/seasonal/longitudinal variations of equatorial irregularity occurrences and their relationship with the postsunset vertical drift velocities (2008, background): “Similarly, the s/l distributions of equatorial spread-F events observed by the polar-orbiting CHAMP satellite between 380 and 450 km altitudes from 2001 to 2004 cannot provide fine spatial/temporal resolution as the low-latitude-orbiting ROCSAT does [ Stolle et al., 2006 ].”
The Magnetic Field of the Earth’s Lithosphere (2010, methodology): “Stolle et al. (2006) proposed an automatic procedure to identify the magnetic field contribution generated by post-sunset low-latitude ionospheric plasma instabilities.”
Sq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo Currents (2017, unknown): “The strong eastward equatorial electric field during the pre-reversal enhancement is linked to another phenomena called equatorial spread-F or plasma bubble, which is characterized by a depletion of the equatorial ionospheric plasma density (e.g., Burke et al. 2004; Stolle et al. 2006).”
Third generation of the Potsdam Magnetic Model of the Earth (POMME) (2006, methodology): “[18] Plasma pressure-driven electric currents reduce the magnetic field in the ionospheric F-region by a few nanotesla.”
Resolution of direction of oceanic magnetic lineations by the sixth‐generation lithospheric magnetic field model from CHAMP satellite magnetic measurements (2008, unknown): “We further discarded all tracks which were identified as being contaminated by magnetic signals because of plasma irregularities in the low-latitude ionosphere [Stolle et al., 2006].”