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Glocer-RECONX (2016-02-02)

Reconnection site determination tool

Model Description

Post-processing utility to calculate changes of magnetic topology in the day side magnetosphere.

The outputs includes separator surfaces and lines and magnetic nulls, all of which determine where magnetic reconnection can occur.
 
Visualization is done in HTML5 using the Plotly library in Python (Glocer_visualization.py and miniconda environment "separatrix_visualization" developed by Asher Pembroke)

Model Figure(s) :

  • Glocer-RECONX sample output diagram
  • Model Inputs Description

    Three-dimensional magnetosphere solution: 
    SWMF: 3d__var_1_e20150317-010900-000.out, 3d__var_1_e20150317-010900-000.info, 3d__var_1_e20150317-010900-000.tree
    OpenGGCM, LFM, GUMICS (SWMF without  *.tree files): interpolated N, B_x, B_y, and B_z data in dayside magnetosphere/ Tecplot output format.

    Model Outputs Description

    Set of outputs:
    3d__var_1_e20150317-010800-000.out_NegNulls.dat
    3d__var_1_e20150317-010800-000.out_PlusNulls.dat
    3d__var_1_e20150317-010800-000.out_Separator.dat
    3d__var_1_e20150317-010800-000.out_Separator_Plane_Y.dat
    3d__var_1_e20150317-010800-000.out_Surface1.dat
    3d__var_1_e20150317-010800-000.out_Surface2.dat
    Negative nulls, positive nulls (depending on eigenvalues of matrix of derivatives),
    Separator (intersection of surfaces separating different topologies) and Surface lists. (Surfaces between closed and open and open and solar wind/IMF topology).
    
    All output files are ASCII files formatted for TecPlot:
    
    Example file with one position:
    
    [RECONX_Glocer_output]$ cat 3d__var_1_e20150317-010900-000.out_NegNulls.dat
    VARIABLES = "X", "Y", "Z"
    Zone I=  1, J=  1, DATAPACKING=POINT
      1.2500000000E+00 -2.5000000000E-01 -1.1750000000E+01
    

    Model Caveats

    Model calculated topology for 3D output snapshots from another model's run.
    Runs in parallel on 60 processors but may still take hours to process a single magnetosphere configuration.

    Change Log

    2016/03/02: Model was modified to use fewer longitude and latitude positions to determine surfaces in order to limit execution time.

    Model Acknowledgement/Publication Policy (if any)

    
    	
    	
    	

    Model Domains:

    Geospace

    Space Weather Impacts:

    Phenomena :

    Simulation Type(s):

    Post_Processing_Tools

    Temporal Dependence Possible? (whether the code results depend on physical time?)

    false

    Model is available at?

    CCMC

    Source code of the model is publicly available?

    false

    CCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):

    production

    Code Language:

    Fortran and C++

    Regions (this is automatically mapped based on model domain):

    Earth.Magnetosphere

    Contacts :

    Alex.Glocer, ModelDeveloper
    Lutz.Rastaetter, ModelHostContact

    Acknowledgement/Institution :

    Relevant Links :

    Publications :

  • A. Glocer, J. Dorelli, G. Toth, et al., "Separator reconnection at the magnetopause for predominantly northward and southward IMF: Techniques and results", JGR SPACE PHYSICS, 121 (1), 140-156 (2016)
  • C. M. Komar, P. A. Cassak, J.C. Dorelli, et al., "Tracing magnetic separators and their dependence on IMF clock angle in global magnetospheric simulations" JGR SPACE PHYSICS, 118 (8), 4998-5007 (2013)
  • Model Access Information :

    Access URL: https://ccmc.gsfc.nasa.gov/requests/PP/user_registration.php?model=RECONX
    Access URL Name: Runs-on-Request
    Repository ID: spase://CCMC/Repository/NASA/GSFC/CCMC
    Availability: online
    AccessRights: OPEN
    Format: HTML
    Encoding: None

    Linked to Other Spase Resource(s) (example: another SimulationModel) :

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