Noe Brucy
119 lines
5.7 KiB
YAML
119 lines
5.7 KiB
YAML
plot : # Plot parameters
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put_title : False # Add a title to plot
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# Maps
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ntick : 6 # Number of ticks for maps
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# Overlays
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vel_red : 40 # Take point each vel_red for velocities
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tight_layout : False # Wheter to apply tight_layout
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time_fmt : "{:.3g} {}" # Time format string, 1st field is time and 2nd is unit
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rcParams: # Anything there will be passed to matplotlib's rcParams
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{} # remove and replace by rcParams keys
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disk: # Disk speficic parameters
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enable : False # Enable specific disk analysis
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center : [0.5, 0.5, 0.5] # Position of the center of the disk (in fraction of lbox)
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binning : "log" # Kind of binning (lin : linear, log : logarithmic)
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mass_star : 1. # Mass of the central star
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nb_bin : 100 # Number of bins for averaged quantities
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bin_in : 1e-3 # Outer radius of the inner bin
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bin_out : 0.25 # Inner radius of the outer bin
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rmin_pdf : 0.075 # Inner radius for PDF computation
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rmax_pdf : 0.3 # Outer radius for PDF computation
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pdf: # parameters for probability density functions
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nb_bin : 100 # Number of bins for the PDF
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range : [-1.5, 2.5] # Range of the PDF (log of fluctuation)
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xmin_fit : 0.3 # Lower boundary of the fit (log of fluctuation)
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xmax_fit : 1.5 # Upper boundary of the fit (log of fluctuation)
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fit_cut : 1e-4 # Exclude value that are < fit_cut * maximum
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filaments: # parameters for FilFinder
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datamap : "fluct_coldens"
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verbose : False
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rmin : 0.15 # In fraction of the box (zoom to be taken into account)
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rmax : 0.45 # In fraction of the box (idem)
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size_thresh : 400 # in pixels**2
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skel_thresh : 50 # in pixels
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branch_thresh : 50 # in pixels
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glob_thresh : 1.5 # in datamap unit
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pymses: # Parameters for Pymses reader
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# Source settings
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variables : ["rho","vel","Br","Bl","P", "g", "phi"] # Read these grid variables
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part_variables : ["vel","mass","id","level","epoch"] # Read these particles variables
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check_variables : True # Whether to check if the variables are indeed in the data
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order : '<' # Bit order
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# Processing options
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levelmax : 20 # Maximal AMR level visited when looking levels
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fft : False # Quick and dirty rendering using FFT
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verbose : False # Let pymses write on standart output
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multiprocessing : True # Whether to use multiprocessing
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# Camera settings
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center : [0.5, 0.5, 0.5] # Center of the image
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zoom : 1. # Zoom of the image
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map_size : 1024 # Size of the computed maps in pixel
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# Filter parameters
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filter : False # Enable filtering
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min_coords : [0.35, 0.35, 0.45]
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max_coords : [0.65, 0.65, 0.55]
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input: # Parameters on how to look for input files (= output from Ramses)
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log_prefix : "run.log" # Prefix of the log file
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label_filename : "label.txt" # Name of the label file
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nml_filename : "run.nml" # name of the namelist file
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ramses_ism : True # If ramses-ism is used
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out: # Parameters for post processing
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copy_info : True # Copy logs, nml and info files to the outdir
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tag : "" # Tag for the image
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interactive : False # Interactive mode (keep figures open)
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save : True # Save the plots on the disk
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ext : '.jpeg' # extension for plots
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ext_subfolder : True # Separate production by extension in subfolders
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fmt : "" # Format of the output filename for plots
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# The following keys are accepted
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# {out} : The output directory (where hdf5 files are also stored)
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# {run} : Name of the relevant run
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# {num} : Name of the input file (from Ramses)
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# {ext} : Extension defined above (with the dot)
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# {name} : Name of the rule
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# {subfolder} : replaced by /{ext[1:]}/ if ext_subfolder is true
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# {tag} : Tag defined above
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# {nml[nml_key]} : The value of nml_key in the namelist (ex: {nml[amr_params/levelmin]})
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process: # General setting of the post-processor module
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verbose : True # Give more infos on what is going on
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num_process : 1 # Number of forks
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mpi : False # If available, use mpi4py
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allow_error : False # Catch all errors in rules involving the disk
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save_cells : True # Save cells structure on disk
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save_parts : True # Save particles on disk
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unload_cells : True # Save memory usage
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logfile : "" # Store log in a file
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rules: # Specific rules parameters
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turb_energy_threshold : -1 # Remove invalid data (<0 = no threshold)
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astrophysix: # Parameters for astrophysix and galactica
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generate : False # Whether to generate astrophysix objects
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simu_fmt : "{tag}_{run}" # Format of the name of simulation
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descr_fmt : "{tag}_{run}" # Format of the default description
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# The following keys are accepted
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# {run} : Name of the relevant run
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# {tag} : Tag defined above
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# {nml[nml_key]} : The value of nml_key in the namelist (ex: {nml[amr_params/levelmin]})
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