Skymap¶

OTSO.skymap ¶
skymap(
Stations: Union[str, Sequence[str]],
customlocations: Optional[list] = None,
solar_wind_params: SolarWindParams = {},
geomagnetic_params: GeomagneticParams = {},
tsyganenko_params: TsyganenkoParams = {},
datetime_params: DateTimeParams = {},
magfield_params: MagFieldParams = {},
integration_params: IntegrationParams = {},
particle_params: ParticleParams = {},
rigidity_params: RigidityParams = {},
coordinate_params: CoordinateParams = {},
computation_params: ComputationParams = {},
data_retrieval_params: DataRetrievalParams = {},
custom_field_params: CustomFieldParams = {},
skymap_params: SkymapParams = {},
) -> list
Compute geomagnetic cutoff rigidities over a range of zenith and azimuth combinations for given neutron monitor stations, or user-defined locations. Useful for showing the East-West asymmetry of cosmic-ray arrival.
Upon calling this function, OTSO will perform particle tracing simulations based on the specified parameters, returning the cutoff rigidities as functions of zenith and azimuth, and related metadata.
Parameters:
-
Stations(str | list) –Station name(s) or identifiers used for cutoff calculations.
-
customlocations(list, default:None) –Custom locations as [["NAME", lat, lon]].
-
cutoff_comp(str) –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 extensionbobergtype(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 modeloptimise_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
-
skymap_params(SkymapParams, default:{}) –Sky map zenith and azimuth resolution parameters
Available keys:
zenithstep(float, default=15): Zenith resolutionazimuthstep(float, default=45): Azimuth resolutionmaxzenith(float, default=75): Maximum deviation from the zenithminzenith(float, default=0): Minimum deviation from the zenithmaxazimuth(float, default=360): Maximum azimuth valueminazimuth(float, default=0): Minimum azimuth value
-
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 functionb_index(float, default=0.032): Boynton coupling functionsym_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 coefficientG2(float, default=0.12): Tsyganenko G2 coefficientG3(float, default=0.47): Tsyganenko G3 coefficientW1(float, default=0.07): Tsyganenko W1 coefficientW2(float, default=0.06): Tsyganenko W2 coefficientW3(float, default=0.13): Tsyganenko W3 coefficientW4(float, default=0.03): Tsyganenko W4 coefficientW5(float, default=0.05): Tsyganenko W5 coefficientW6(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 pointminaltitude(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 limitmintrapdist(float, default=0): Minimum trapping distancestartaltitude(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 integrationadaptivestep(bool, default=True): Enable adaptive time stepsmaxsteps(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
-
coordinate_params(CoordinateParams, default:{}) –Coordinate systems.
Available keys:
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 processingthreadnum(int, default=None): Number of threads per CPU core for Fortran computationsVerbose(bool, default=True): Enable verbose output
-
data_retrieval_params(DataRetrievalParams, default:{}) –Data retrieval.
Available keys:
serverdata(str, default="OFF"): Server data retrieval from OMNIlivedata(str, default="OFF"): real-time data retrieval from NOAA
-
custom_field_params(CustomFieldParams, default:{}) –Custom fields.
Available keys:
g(list, default=None): Gauss g coefficientsh(list, default=None): Gauss h coefficientsmax_degree(int, default=13): Max degree of spherical harmonic expansionMHDfile(str, default=None): MHD simulation fileMHDcoordsys(str, default=None): MHD coordinate systemMHDgridtype(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) –[skymap_dataframe, readme_text]
- skymap_dataframe: Cutoff data values per input station and zenith and azimuth combination in a pandas dataframe. (Ru, Rc, Rl, PTF)
- readme_text: OTSO computation summary
Examples:
import OTSO
if __name__ == "__main__":
stations = ["ROME"] # list of neutron monitor stations (using their abbreviations)
# Using parameter groups
skymap_results = skymap(
Stations=stations,
computation_params={"corenum": 1,"threadnum": 8},
datetime_params={"year": 2005,"month": 5,"day": 1,"hour": 0},
integration_params={"gyropercent": 10},
magfield_params={"internalmag": "IGRF","externalmag": "NONE"},
rigidity_params={"rigiditystep": 0.01},
skymap_params={"zenithstep": 5,"azimuthstep": 15}
)
# Access the results
skymap_data, metadata = result