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Glocer-RECONX (2016-02-02)Reconnection site determination toolModel DescriptionPost-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) :Model Inputs DescriptionThree-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 DescriptionSet 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 CaveatsModel 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 Log2016/03/02: 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:GeospaceSpace Weather Impacts:Phenomena :Simulation Type(s):Post_Processing_ToolsTemporal Dependence Possible? (whether the code results depend on physical time?)falseModel is available at?CCMCSource code of the model is publicly available?falseCCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):productionCode Language:Fortran and C++Regions (this is automatically mapped based on model domain):Earth.MagnetosphereContacts :Alex.Glocer, ModelDeveloperLutz.Rastaetter, ModelHostContact Acknowledgement/Institution :Relevant Links :Publications :Model Access Information :Access URL: https://ccmc.gsfc.nasa.gov/requests/PP/user_registration.php?model=RECONXAccess 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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