An n = 90 internal potential function of the Martian crustal magnetic field

By J. Cain, B. Ferguson, D. Mozzoni. 2003

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An overview of radar soundings of the martian ionosphere from the Mars Express spacecraft (2008, methodology): “(2004); and for a more detailed description of the Mars express spacecraft, see Chicarro et al. (2004). Prior to the Mars Express mission, most of our knowledge of the Martian ionosphere came from radio occultation studies. This technique involves making accurate measurements of the phase shift prod”
Electron pitch angle distributions as indicators of magnetic field topology near Mars (2007, unknown): “(d) Field magnitude measured by MAG (black) and predicted using the spherical harmonic model of Cain et al. [2003] (dashed red).”
Crustal magnetic field of Mars (2004, methodology): “, 2002] for the Earth, and FSU-90 [Cain et al., 2003] and our converted model for Mars.”
EARLY CRUSTAL EVOLUTION OF MARS 1 (2005, result): “Figure 4b presents a spherical harmonic representation of the data from the model of Purucker et al. (2000); several other workers (Connerney et al. 2001, Cain et al. 2003, Arkani-Hamed 2002) have produced essentially identical results.”
The Magnetic Field of Planet Earth (2010, background): “14 Lowes-Mauersberger power spectra of the field of internal origin for the Earth (after Olsen et al. 2009a and Maus et al. 2008), Mars (after Cain et al. 2003), Jupiter, Mercury (after Connerney 2008) and the Moon (after Purucker 2008) at their respective surface reference radius.”