Fig. 9.From: Evaluation of candidate geomagnetic field models for IGRF-11Lowes-Mauersberger spectra of the vector field differences i, j R n between the IGRF-11 average SV over the interval 2005 to 2010 (IGRF-2010 minus DGRF-2005 divided by 5, referred to as SV-2007.5-G11 in the text) and the SV candidate models considered for IGRF-10 epoch at 2007.5.Back to article page