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In the CASP6 experiment, the assessors reported that knotted models were still being submitted and that such knotted models submitted for comparative modeling targets were rejected out of hand without additional assessment (Tress et al., 2005).
Table 4 summarizes the candidate models submitted for IGRF-2010.
Important details about the team models submitted for SV are collected for reference in Table 6.
Table 4. Summary of IGRF-2010 candidate models submitted for consideration in IGRF-11.
The retrospective MF models submitted for DGRF-2005 were found to largely be in good agreement.
By construction, the IGRF model is defined as a weighted average of candidate models submitted for evaluation by various teams (Finlay et al., 2010).
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For this reason, the evaluators also relied on the companion descriptions of the candidate model submitted for evaluation and finally often on their empirical experience.
We carried out a similar analysis for the candidate models submitted to IGRF for epoch 2015.0 (Table 4).
We describe the candidate models submitted by the British Geological Survey for the 12th generation International Geomagnetic Reference Field.
Overall, 75% of the models submitted were in agreement with others for that gene and passed our quality control checks.
Table 2 Summary of DGRF-2010 candidate models submitted to IGRF-12 DGRF candidate models for main field epoch 2010 Team Model Organization Data Comments (parent model etc).
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