Registered Model Settings for GEM-CEDAR Challenge
| Model setting tag | Model setting description |
| 10_CTIPE | CTIPe (including NO Cooling) run driven by Weimer electric potential and SWMF particle precipitation |
| 10_TIE-GCM | TIE-GCM1.95 with Weimer-2005, CCMC RoR settings |
| 31_CTIPE | CTIPe runs driven by high-latitude electric potential and particle precipitation obtained from SWMF |
| 3_JB2008 | JB2008 run by CCMC |
| 3_NRLMSISE-00 | NRLMSISe00 from http://sisko.colorado.edu/sutton/data.html |
| 4_CTIPE | 1_CTIPe run including NO cooling |
| 4_GITM | GITM2.0, CCMC RoR settings |
| 51_CTIPE | CTIPe runs with AMIE electric potential and particle precipitation (run with magnetometers, SuperDARN, and DMSP inputs, provided by ASTRA) |
| 61_CTIPE | 31_CTIPE run including NO cooling |
| 6_CTIPE | 3_CTIPE run including NO cooling |
| 7_TIE-GCM | TIE-GCM 1.94 driven by AMIE (from ASTRA) with dynamic co-latitude |
| 81_CTIPE | 51_CTIPE run including NO cooling |
| 8_CTIPE | 5_CTIPE run including NO cooling |
| 8_TIE-GCM | TIE-GCM 1.94 with SWMF |
| 9_CTIPE | CTIPe (including NO Cooling) run driven by superDARN electric potential (SAM) |
| 9_TIE-GCM | TIEGCM-CMIT |
| 1_BFM92 | Burton (1975) Feldstein (1992) and Murayama (1982) |
| 1_CMIT | CMIT 2.0, George_Millward (28/05/2009, 04/06/2009) |
| 1_CMIT-LTR | CMIT 2.1-1, LFM+MIX, ~163K cells |
| 1_CTIPE | CTIPe 2.0 w/ Weimer2005 |
| 2_CTIPE | CTIPe runs at NOAA/SWPC with Weimer 2005 using 1-minute solar wind and IMF from ACE; particle precipitation from TIROS/NOAA auroral particle measurements; (f10.7+f81)/2; and the (2,2), (2,3), (2,4), (2,5), and (1,1) propagating tidal modes are imposed at 80 km altitude with a prescribed amplitude and phase |
| 3_CTIPE | CTIPe runs driven by high-latitude electric potential obtained from SWMF |
| 5a_CTIPE | CTIPe runs with AMIE (run with magnetometers and SuperDARN inputs, provided by ASTRA) |
| 5b_CTIPE | CTIPe runs with AMIE (run with magnetometers inputs, provided by ASTRA) |
| 5_CTIPE | CTIPe runs with AMIE (run with magnetometers, SuperDARN, and DMSP inputs, provided by ASTRA) |
| 11_CTIPE | CTIPe_3.2 w/ Weimer2005 (ACE IMF and Solar Wind data) |
| 0_GITM | 0_GITM |
| 1_GITM | 1_GITM |
| 3_GITM | 3_GITM |
| 6_GITM | GITM_2.5 w/ Weimer2005 (ACE IMF and Solar Wind data) |
| 1_HWM07 | HWM07 model |
| 1_IRF96 | IRF-96, Robert Weigel, 2010/06/04 Impulse Response Function with 96 lags (ver. 0) |
| 1_IRI | IRI-2007 |
| 2_IRI | IRI-2012 with NeQuick model for topside Ne, MSIS-86 neutral composition |
| 4_IRI | IRI-2016 with URSI foF2 model, NeQuick for topside Ne, NRLMSISE00 neutral composition |
| 1_JB2008 | original JB2008 |
| 2_JB2008 | JB2008 with Weimer temperature correction |
| 1_LFM | Michael_Wiltberger (13/11/2008, 15/05/2009) |
| 1_LFM-MIX | GEM2008_CHALLENGE_061410 runs, CCMC (2010) |
| 1_NARMAX | UOS-NARMAX-HW - NARMAX polynomial derivation from previous estimated Dst and 1-hour OMNI averaged solar wind data. Without ring current effects, Hualiang_Wei_300311 |
| 2_NARMAX | UOS-NARMAX-RJB - NARMAX polynomial derivation from previous estimated Dst and 1-hour OMNI averaged solar wind data. With ring current effects, Richard_Boynton_300311 |
| 1_NRLMSISE-00 | Original NRLMSISE-00 model |
| 2_NRLMSISE-00 | Original NRLMSISE-00 model plus yearly corrections to exospheric temperature and density and composition at 120 km, based on annual average ratio of orbit derived densities to MSIS (Emmert, JGR, A06315, 2009; Emmert et al., GRL, L12102, 2010). This version of NRLMSISE-00 was used in the SAMI3 runs. |
| 1_OPENGGCM | OpenGGCM 3.1, 3 M cells, subtracted GSE_OpenGGCM dipole, added GSE dipole |
| 2a_OPENGGCM | OpenGGCM 3.1, 6.5M cells - model run in SM coordinates |
| 2_OPENGGCM | OpenGGCM 3.1, 6.5M cells, subtracted GSE OpenGGCM dipole, added GSE dipole |
| 3_OPENGGCM | OpenGGCM 3.1, Alexander Vapirev's submission, subtracted GSE_OpenGGCM dipole, added GSE dipole |
| 4_OPENGGCM | OpenGGCM 4.0, ~7 mln cells, with updating dipole |
| 5_OPENGGCM | OpenGGCM 4.0 with CRCM, with updating dipole (planned at CCMC) |
| 6_OPENGGCM | OpenGGCM 4.0 with RCM, with updating dipole (planned at CCMC) |
| 7_OPENGGCM | Grid 518/200/252 (-20.01 600.01)(-40.01 40.01)(-40.01 40.01) |
| 8_OPENGGCM | OpenGGCM 4.0 with CTIM and dipole rotation 6.0M cells |
| 1a_OPENGGCM | OpenGGCM v3.1, 3 M cells, sat in GSE OpenGGCM coordinates, CCMC RoR settings |
| 1_RAMSCB | RAM-SCB stand-alone driven by LANL particle observations Volland-Stern electric field and dipole magnetic field, Dan Welling 310311 |
| 2_RAMSCB | RAM-SCB stand-alone driven by LANL particle observations Weimer 2000 electric field and dipole magnetic field, Dan Welling 310311 |
| 3_RAMSCB | RAM-SCB stand-alone driven by LANL particle observations Weimer 2000 electric field and T89Self Consistent magnetic field, Dan Welling 310311 |
| 4_RAMSCB | RAM-SCB driven by SWMF/BATSRUS and RIMa (Ridley Ionosphere Model), Dan Weling 310311 |
| 5_RAMSCB | RAM-SCB driven by SWMF/BATSRUS, MultiSpecies RIM and PWOM (Polar Wind Outflow Model) |
| 1_RCM | Rice Convection Model, Hilmer and Voigt (1995) magnetic field, Siscoe-Hill polar cap potential drop, Tsyganenko and Mukai (2003) plasma condition on the outer-L boundary |
| 2_RCM | Rice Convection Model, Hilmer and Voigt (1995) magnetic field, Siscoe-Hill polar cap potential drop, Borovsky (1998) plasma condition on the outer-L boundary |
| 3_RCM | Rice Convection Model, Hilmer and Voigt (1995) magnetic field, Siscoe-Hill polar cap potential drop, MSM plasma condition on the outer-L boundary |
| 4_RCM | Rice Convection Model, Hilmer and Voigt (1995) magnetic field, Weimer (2005) polar cap potential drop, Borovsky (1998) plasma condition on the outer-L boundary |
| 1_RDST | RDST (real-time analysis of magnetometer data) version 2.1c, Vince Eccles (04/20/2011) |
| 1_RiceDst | Rice Univ. Dst model - neural network using Boyle 1997 solar wind driver and dyn. pressure, Ramkumar_Bala_31031 |
| 1_SAMI3 | 1_SAMI3_HWM93 |
| 1_SAMI3_HWM07 | 1_SAMI3_HWM07 |
| 1_SAMI3_HWM93 | 1_SAMI3_HWM93 |
| 7_SWMF | SWMF V. 20110215 BATSRUS+CRCM, 1.78M cells, 1/8 RE res., 2.7 times slower than RT on 200 processors on Harpertown nodes of Pleiades, Alex Glocer and Xing Meng |
| 8_SWMF | SWMF V20110111 BATSRUS+RCM2, 1M cells 1/4 Re res. out to 9 Re 3 times faster than RT on 240 processors on Pleiades, InnerBc density0.2cpcp18 /cc RCM ions ration NH/N09/1, Yiqun Yu and Xing Meng |
| 9_SWMF | SWMF.v20110131, ~1 mln cells with RCM, with updating dipole |
| 1_SWMF | BATSRUS v.7.73; 2M cells; CCMC |
| 2_SWMF | BATSRUS v.7.73; 700K cells (real-time setup); CCMC RoR settings |
| 3_SWMF | BATSRUS v.8.01 with RCM; 2M cells; CCMC RoR settings |
| 4_SWMF | BATSRUS v8.01; 3M cells; CCMC ROR settings |
| 5_SWMF | BATSRUS v8.01 with RCM; 3M cells; CCMC ROR settings |
| 6_SWMF | SWMF V.20090403, BATSRUS + RCM2, 900K cells, RT on 64 procs, A. Ridley |
| 1_TIE-GCM | TIE-GCM v.1.93 with Heelis |
| 2_TIE-GCM | TIE-GCM1.94 with Weimer-2005 |
| 3_TIE-GCM | TIE-GCM1.94 with Weimer 2005 high-latitude electric potential in double resolution |
| 4_TIE-GCM | TIE-GCM1.94 with Weimer 2005 and SABER/TIDI lower boundary conditions in double resolution |
| 5_TIE-GCM | TIE-GCM1.94 driven by AMIE with constant critical cross-over latitudes (fixed at 55 and 70 mlat) |
| 6_TIE-GCM | TIE-GCM 1.94 with AMIE (from ASTRA) |
| 11_TIE-GCM | TIE-GCM2.0 w/ Weimer2005 (OMNI IMF and Solar Wind data) |
| 1_T04 | Tsyganenko 2004, CCMC |
| 1_T96 | Tsyganenko 1996, CCMC |
| 1_UAM | Upper Atmosphere Model (UAM), A.A. Namgaladze et al., FAC as external driver |
| 2_UAM | UAM with AMIE electric potentials as external drivers |
| 3_UAM | UAM with Weimer-2005 (and/or Weimer-96) electric potentials |
| 4_UAM | UAM, driver as 5_UAM, but constraint by using MSIS neutral temperature profiles, 2 min resolution |
| 5_UAM | UAM, fully theoretical, FAC as external driver, 30 sec resolution |
| 1_UAM-P | Upper Atmosphere Model (UAM) - Potsdam Version w/ FAC Iijima and Potemra Model (IPM) |
| 1_USU-GAIM | 1_USU-GAIM |
| 1_IFM | 1_USU-IFM |
| 1_USU-IFM | 1_USU-IFM |
| 1_WEIGEL | Robert Weigel's ground perturbation model |
| 3_WEIGEL | R. Weigel's ground perturbation model (issued 2012/03/15) |
| 5_WEIMER | Weimer empirical geomagnetic prediction model (issued 2011/04/19) |
| 1_WEIMER | Weimer 2005 , Daniel_Weimer (12/05/2009) |
| 2_WEIMER | Weimer 2005, GEM08_Daniel_Weimer_030809 , that is still in the development stage. The model is based on input data from over 100 magnetometer stations in the Northern hemisphere, as well as the simultaneous interplaneta ry magnetic field from ACE. The database used for this submission spans a time period fro m 1998 thru 2001. The model calculates the North, East, and Vertical magnetic perturbatio ns in corrected geomagnetic coordinates, and can also derive output values in geographic c oordinates. For this challenge submission, a post-processing step rotates the results int o geomagnetic dipole coordinates and also interpolates the results. |
| 3_WEIMER | New empirical model of geomagnetic perturbation. Finalized in 2011. Input values are from ACE measurements and the F10.7 index. |
| 1_WINDMI | |
| 2_WINDMI | WINDMI-1.0-nominal, Siscoe solar wind driver |
| 3_WINDMI | WINDMI-1.0-nominal, Newell solar wind driver |
Model setting tags uniquely identify individual model settings. Their format is: Number (referring to unique model setting), underscore and a one-word model name (for example, SWMF, OpenGGCM).
