Planet¶

Planet Diagram

OTSO.planet ¶

planet(
    cutoff_comp: str = "Vertical",
    solar_wind_params: SolarWindParams = {},
    geomagnetic_params: GeomagneticParams = {},
    tsyganenko_params: TsyganenkoParams = {},
    datetime_params: DateTimeParams = {},
    magfield_params: MagFieldParams = {},
    integration_params: IntegrationParams = {},
    rigidity_params: RigidityParams = {},
    coordinate_params: CoordinateParams = {},
    computation_params: ComputationParams = {},
    data_retrieval_params: DataRetrievalParams = {},
    custom_field_params: CustomFieldParams = {},
    particle_params: ParticleParams = {},
    grid_params: GridParams = {},
    asymptotic_params: AsymptoticParams = {},
    transmission_params: TransmissionParams = {},
) -> list

Compute planetary cutoff grid using the OTSO framework.

Generates a global grid of geomagnetic cutoff rigidities across the Earth's surface. Users can also request the computation of asymptotic viewing directions and transmission functions by request. Useful for studying global cosmic ray accessibility patterns.

Parameters:

cutoff_comp (str, default: 'Vertical' ) –

Cutoff computation method ("Vertical", "Apparent", "Custom").
datetime_params (DateTimeParams, default: {} ) –
Date/time parameters.

Available keys:
- year (int, default=2024): Year (e.g., 2023)
- month (int, default=1): Month (1–12)
- day (int, default=1): Day (1–31)
- hour (int, default=12): Hour (0–23)
- minute (int, default=0): Minute (0–59)
- second (int, default=0): Second (0–59)
magfield_params (MagFieldParams, default: {} ) –
Magnetic field models.

Available keys:
- internalmag (str, default="IGRF"): "NONE", "IGRF", "Dipole", "Custom Gauss", "CHAOS"
- externalmag (str, default="TSY89c"): "NONE", "TSY87short", "TSY87long", "TSY89a", "TSY96", "TSY01", "TSY01S", "TSY04", "TSY89c", "TSY15N", "TSY15B", "TA16_RBF", "TSY89_refit", "MHD"
- boberg (bool, default=False): Enable Boberg extension
- bobergtype (str, default="EXTENSION"): "EXTENSION", "CONTINUOUS", "DST_DEPENDENT", "DST_MIDPOINT"
- magnetopause (str, default="Kobel"): "NONE", "Kobel", "Sibeck", "Lin", "Sphere", "aFormisano"
- spheresize (float, default=25): Spherical boundary radius (Re)
- AdaptiveExternalModel (bool, default=False): Auto-select external model
- optimise_tsy (bool, default=False): Use the faster implementation of the selected Tsyganenko model (affects externalmag="TSY01", "TSY01S", "TSY04", or "TSY96"; other models are unaffected by this flag). Both settings give numerically identical results (all known bugs are fixed in both); True is just faster
rigidity_params (RigidityParams, default: {} ) –
Rigidity scanning.

Available keys:
- startrigidity (float, default=20): Initial rigidity (GV)
- endrigidity (float, default=0): Final rigidity (GV)
- rigiditystep (float, default=0.01): Step size (GV)
- rigidityscan (str, default="ADAPTIVE"): Penumbra scanning ("ADAPTIVE"/"ON"/"OFF"). "ADAPTIVE" extends the fine scan until the penumbra is bounded by clean guard bands; "ON" uses a fixed ±0.75 GV window around a 0.25 GV coarse scan; "OFF" scans the full range
asymptotic_params (AsymptoticParams, default: {} ) –
Asymptotic computation parameters.

Available keys:
- unit (str, default="GeV"): level unit ("GeV", "GV")
- asymptotic (str, default="NO"): Enable asymptotic cone computation ("YES"/"NO")
- asymlevels (list, default=[0.1,0.3,0.5,1,2,3,4,5,6,7,8,9,10,15,20,30,50,70,100,300,500,700,1000]): level values for asymptotic computation
transmission_params (TransmissionParams, default: {} ) –
Transmission function computation parameters

Available keys:
- transmission (bool, default=False): Bool to enable or disable transmission computation
- transmissionRstep (float, default=0.001): R ± transmissionRstep defines the transmission rigidity sampling range
- transmissionsamples (int, default=20): the number of sample rigidities to test within the sampling range
solar_wind_params (SolarWindParams, default: {} ) –
Solar wind parameters. Defaults are quiet-time medians (Kp <= 1) of OMNI data, 1996-2025.

Available keys:
- vx (float, default=-359.4): Solar wind velocity x-component (km/s)
- vy (float, default=0): Solar wind velocity y-component (km/s)
- vz (float, default=0): Solar wind velocity z-component (km/s)
- bx (float, default=0.11): IMF x-component (nT)
- by (float, default=-0.16): IMF y-component (nT)
- bz (float, default=0.58): IMF z-component (nT)
- by_avg (float, default=-0.17): Averaged IMF By over last 30mins (nT)
- bz_avg (float, default=0.59): Averaged IMF Bz over last 30mins (nT)
- density (float, default=4.94): Solar wind density (particles/cm³)
- pdyn (float, default=1.31): Solar wind dynamic pressure (nPa); computed from density and velocity when 0, or when density or velocity is given without pdyn
geomagnetic_params (GeomagneticParams, default: {} ) –
Geomagnetic indices. Defaults are quiet-time medians (Kp <= 1) of OMNI data, 1996-2025.

Available keys:
- Dst (float, default=-4): Dst index (nT)
- kp (float, default=0.7): Kp index (0-9)
- n_index (float, default=0.145): Newell coupling function
- b_index (float, default=0.032): Boynton coupling function
- sym_h_corrected (float, default=-18.07): Corrected SYM-H index (nT)
tsyganenko_params (TsyganenkoParams, default: {} ) –
Tsyganenko model coefficients. Defaults are quiet-time medians (Kp <= 1) of OMNI data, 1996-2025.

Available keys:
- G1 (float, default=0.38): Tsyganenko G1 coefficient
- G2 (float, default=0.12): Tsyganenko G2 coefficient
- G3 (float, default=0.47): Tsyganenko G3 coefficient
- W1 (float, default=0.07): Tsyganenko W1 coefficient
- W2 (float, default=0.06): Tsyganenko W2 coefficient
- W3 (float, default=0.13): Tsyganenko W3 coefficient
- W4 (float, default=0.03): Tsyganenko W4 coefficient
- W5 (float, default=0.05): Tsyganenko W5 coefficient
- W6 (float, default=0.08): Tsyganenko W6 coefficient
integration_params (IntegrationParams, default: {} ) –
Integration settings.

Available keys:
- intmodel (str, default="Boris-Buneman"): "4RK", "5RK", "6RK", "Vay", "HC", "Boris-Buneman"
- gyropercent (float, default=1): Step size as a percentage of the gyration period. With adaptivestep=True (default) it caps each step using the local field; with adaptivestep=False the step is fixed for the whole trace at this percentage of the gyration period at the launch point
- minaltitude (float, default=20): Minimum altitude (GDZ = km or other = Re)
- maxdistance (float, default=100): Maximum path length travelled (Re), not distance from Earth; 0 disables this check (use 0 for long trapped-particle runs: a 0.6c proton travels 100 Re in ~4 s)
- maxtime (float, default=0): Maximum flight time in seconds (lab frame); 0 = no limit
- mintrapdist (float, default=0): Minimum trapping distance
- startaltitude (float, default=20): Starting altitude (GDZ = km or other = Re)
- betaerror (float, default=0.001): Maximum allowed beta error for integration steps %
- totalbetacheck (bool, default=False): Enable cumulative beta check during integration
- adaptivestep (bool, default=True): Enable adaptive time steps
- maxsteps (int, default=0): Maximum number of integration steps; 0 = no limit
particle_params (ParticleParams, default: {} ) –
Particle settings.

Available keys:
- Anum (int, default=1): Atomic number (-1=muon, 0=electron, 1=proton, 2=alpha)
- anti (str, default="YES"): YES = anti-particle, NO = particle
- zenith (float, default=0): Zenith angle for Custom cutoff computation
- azimuth (float, default=0): Azimuth angle for Custom cutoff computation
grid_params (GridParams, default: {} ) –
Grid configuration parameters.

Available keys:
- latstep (float, default=-5): Latitude step size for grid
- longstep (float, default=5): Longitude step size for grid
- maxlat (float, default=90): Maximum latitude for grid
- minlat (float, default=-90): Minimum latitude for grid
- maxlong (float, default=360): Maximum longitude for grid
- minlong (float, default=0): Minimum longitude for grid
- array_of_lats_and_longs (list, default=None): Custom grid points
- grid_type (str, default="regular"): "regular" (latstep/longstep grid), "healpix" (equal-area HEALPix points), "healpix_geomag" (HEALPix rings laid out in centred-dipole coordinates for the date; most accurate per point) or "fibonacci" (golden-angle spiral)
- nside (int, default=12): Resolution for the equal-area grid types: 12 * nside**2 points (12 -> 1728 points, ~550 km spacing, like a 5° grid at the equator)
coordinate_params (CoordinateParams, default: {} ) –
Coordinate systems.

Available keys:
- coordsystem (str, default="GEO"): Output coordinate system; "GDZ", "GEO", "GSM", "GSE", "SM", "GEI", "MAG", "SPH", "RLL"
- inputcoord (str, default="GDZ"): Input coordinate system; "GDZ", "GEO", "GSM", "GSE", "SM", "GEI", "MAG", "SPH", "RLL"
computation_params (ComputationParams, default: {} ) –
Computation settings.

Available keys:
- corenum (int, default=None): Number of CPU cores for multicore processing
- threadnum (int, default=None): Number of threads per CPU core for Fortran computations
- Verbose (bool, default=True): Enable verbose output
- delim (str, default=";"): Delimiter for asymptotic output formatting
data_retrieval_params (DataRetrievalParams, default: {} ) –
Data retrieval.

Available keys:
- serverdata (str, default="OFF"): Server data retrieval from OMNI
- livedata (str, default="OFF"): real-time data retrieval from NOAA
custom_field_params (CustomFieldParams, default: {} ) –
Custom fields.

Available keys:
- g (list, default=None): Gauss g coefficients
- h (list, default=None): Gauss h coefficients
- max_degree (int, default=13): Max degree of spherical harmonic expansion
- MHDfile (str, default=None): MHD simulation file
- MHDcoordsys (str, default=None): MHD coordinate system
- MHDgridtype (str, default="auto"): How the MHD grid is looked up - "auto" detects per-axis spacing automatically, "uniform" forces the fast fixed-spacing path (only correct if every axis really is evenly spaced), "stretched" forces the general path needed for a grid whose resolution varies with position (e.g. finer near Earth)
- MHDinterpolation (str, default="trilinear"): How the field is reconstructed between grid points - "trilinear" is the classic fast corner-blend (kinked gradients at cell boundaries), "tricubic" is a smooth C^1 fit that's far more accurate in smooth field regions but can overshoot near sharp gradients/boundaries, "monotonic" is the same tricubic fit with overshoot limiting (recommended for general use), "divfree" returns the curl of an interpolated vector potential so the field is exactly divergence-free (for long quasi-trapped trajectories; less point-wise accurate than "tricubic"; the gridded field must itself be divergence-free, e.g. an external-only field - a warning is issued otherwise)

Returns:

list ( list ) –
[planet_dataframe, asymptotic_dataframe, transmission_dataframe, readme_text]
- planet_dataframe: Global cutoff rigidity grid
- asymptotic_dataframe: Global asymptotic viewing directions for the energy/rigidity levels input.
- transmission_dataframe: Global tranmssion values for set rigidity values.
- readme_text: OTSO computation summary

Examples:

    from OTSO import planet

    if __name__ == '__main__':

        # Basic global grid
        planet_results = planet(
            cutoff_comp="Vertical",
            grid_params={"latstep": -10, "longstep": 15},
            computation_params={"corenum": 8, "threadnum": 1},
            datetime_params={"year": 2000},
            rigidity_params={"rigiditystep": 0.01},
            integration_params={"gyropercent":10}
        )


        # Access the results
        planet_df, asymptotic_df, transmission_df, metadata = planet_result