GEM-CEDAR Challenge
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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).

National Aeronautics and Space Administration Air Force Materiel Command Air Force Office of Scientific Research Air Force Research Laboratory Air Force Weather Agency NOAA Space Environment Center National Science Foundation Office of Naval Research

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