From: Evaluation of candidate geomagnetic field models for IGRF-12
Predictive SV candidate models for epoch 2015-2020 | ||||
---|---|---|---|---|
Team | Model | Organization | Data | Comments (parent model, propagation to 2015) |
A | SV-2015-2020-A | BGS | Ørsted; CHAMP; Swarm A, B, C; | Based on core flow parent model evaluated |
Observatory hourly means | and averaged SV from 2015.0 to 2020.0 | |||
B | SV-2015-2020-B | DTU Space | Ørsted; CHAMP; SAC-C; Swarm A, B, C; | Based on parent CHAOS-5 model |
Observatory monthly means | evaluated from splines at 2014.0 | |||
C | SV-2015-2020-C | ISTerre | Ørsted; SAC-C; CHAMP; Swarm B | Based on parent ensemble COV-OBS.x1 model |
observatory monthly mean | evaluated and averaged SV from 2015.0 to 2020.0 | |||
D | SV-2015-2020-D | IZMIRAN | Swarm A, B, C | Natural orthogonal components (NOCs) |
Nov-2013 to Sep-2014, no data selection | estimated at 2014.7 (sept-2014) | |||
E | SV-2015-2020-E | NGDC-NOAA | Ørsted; Swarm A, B, C | From parent model |
first-order Taylor series with slope at 2015.0 | ||||
F | SV-2015-2020-F | GFZ | Swarm A, B, C; | From parent model |
USTHB/EOST | observatory hourly means | evaluated and averaged SV from 2013.5 to 2014.5 | ||
G | SV-2015-2020-G | NASA | Geodynamo simulation and assimilation from CALS3K.2, | |
UMBC | gufm1, CM4, CHAOS-4+; average SV from 2015.0 to 2020.0 | |||
H | SV-2015-2020-H | IPGP | Swarm A, B, C | Geodynamo simulation and assimilation from Swarm |
LPG Nantes | evaluated and averaged SV from 2015.0 to 2020.0 | |||
I | SV-2015-2020-I | LPG Nantes | Swarm A and C | From parent model |
CNES | Nov-2013 to Sep-2014 | first-order Taylor series with slope at 2014.3 |