API Reference
Full documentation for all public classes and functions in sparta-solar, generated from the source docstrings.
Atmospheric data sources
MERRA-2 daily reanalysis
MERRA2DailyAtmosphere
Bases: BaseAtmosphere
MERRA-2 daily atmospheric data accessor.
Provides methods to load and interpolate MERRA-2 daily atmospheric data for specific locations or regular grids. Data is automatically cached locally and loaded from Zarr archives organized by year.
The class inherits from BaseAtmosphere and provides two main factory methods: - at_sites(): Extract data at specific point locations - on_regular_grid(): Extract data on a regular lat/lon mesh
Attributes: database_path: Path to local MERRA-2 data storage directory
Available Variables: - pressure: Surface air pressure [Pa] - albedo: Surface albedo [0-1] - pwater: Precipitable water [kg/m²] - ozone: Total column ozone [kg/m²] - beta: Angström turbidity parameter - alpha: Angström wavelength exponent - ssa: Aerosol single scattering albedo
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
at_sites–Load atmospheric data at specific geographic locations.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
-
on_regular_grid–Load atmospheric data on a regular lat/lon grid.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
at_sites
classmethod
at_sites(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float] | float,
longitude: Sequence[float] | float,
site_names: Sequence[str] | None = None,
) -> Self
Load atmospheric data at specific geographic locations.
Extracts and interpolates MERRA-2 data for one or more point locations. Performs bilinear spatial interpolation and quadratic temporal interpolation.
Args: times: Time points for data extraction. Can be numpy datetime64 array or pandas DatetimeIndex. latitude: Latitude coordinate(s) in decimal degrees. Single value or sequence. Range: -90° < lat < 90°. longitude: Longitude coordinate(s) in decimal degrees. Single value or sequence. Range: -180° ≤ lon < 180°. site_names: Optional names for the sites. If provided, added as a coordinate in the output dataset.
Returns: MERRA2DailyAtmosphere: Instance containing interpolated atmospheric data.
Raises: ValueError: If latitude and longitude have different lengths, or if coordinates are out of valid range. NotImplementedError: If required data files are not found locally and downloading is not yet implemented.
Examples: >>> import pandas as pd >>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>> # Single location
>>> times = pd.date_range("2020-01-01", periods=5, freq="D")
>>> atmos = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=40.4168,
... longitude=-3.7038,
... site_names="Madrid"
... )
>>> # Multiple locations
>>> lats = [40.4168, 41.3851, 36.7213] # Madrid, Barcelona, Málaga
>>> lons = [-3.7038, 2.1734, -4.4214]
>>> names = ["Madrid", "Barcelona", "Málaga"]
>>> atmos = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=lats,
... longitude=lons,
... site_names=names
... )
>>> # Access data
>>> pressure = atmos.dataset["pressure"]
>>> print(pressure.dims)
('time', 'site')
Source code in src/spartasolar/atmoslib/merra2_daily.py
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compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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on_regular_grid
classmethod
on_regular_grid(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float] | float,
longitude: Sequence[float] | float,
) -> Self
Load atmospheric data on a regular lat/lon grid.
Extracts and interpolates MERRA-2 data onto a user-specified regular grid. The output has dimensions (time, lat, lon). NaN values in albedo are filled with zeros.
Args: times: Time points for data extraction. latitude: Latitude coordinates for the grid in decimal degrees. Must be a sequence (list, array). longitude: Longitude coordinates for the grid in decimal degrees. Must be a sequence (list, array).
Returns: MERRA2DailyAtmosphere: Instance containing gridded atmospheric data.
Raises: ValueError: If coordinates are out of valid range. NotImplementedError: If required data files are not found locally.
Examples: >>> import pandas as pd >>> import numpy as np >>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>> # Define a regular grid over Iberian Peninsula
>>> times = pd.date_range("2020-06-01", periods=10, freq="D")
>>> lats = np.linspace(36, 44, 9) # 9 latitude points
>>> lons = np.linspace(-10, 4, 15) # 15 longitude points
>>> atmos = MERRA2DailyAtmosphere.on_regular_grid(
... times=times,
... latitude=lats,
... longitude=lons
... )
>>> # Access gridded data
>>> albedo = atmos.dataset["albedo"]
>>> print(albedo.dims)
('time', 'lat', 'lon')
>>> print(albedo.shape)
(10, 9, 15)
Source code in src/spartasolar/atmoslib/merra2_daily.py
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MERRA-2 long-term averages
MERRA2LTAAtmosphere
Bases: BaseAtmosphere
MERRA-2 long-term monthly average atmospheric database.
Provides climatological monthly averages (1999-2018) of atmospheric constituents from NASA MERRA-2 reanalysis. Data is interpolated spatially and temporally to match requested coordinates and times.
See module documentation for examples.
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
at_sites–Retrieve monthly climatology at specific sites.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
-
on_regular_grid–Retrieve monthly climatology on a regular spatial grid.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
at_sites
classmethod
at_sites(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float] | float,
longitude: Sequence[float] | float,
site_names: Sequence[str] | None = None,
) -> Self
Retrieve monthly climatology at specific sites.
Parameters:
-
(timesndarray or DatetimeIndex) –Time stamps for climatology retrieval. Monthly climatology is repeated for each year and interpolated to exact times.
-
(latitudeSequence[float]) –Latitude(s) in degrees North [-90, 90]
-
(longitudeSequence[float]) –Longitude(s) in degrees East [-180, 180]
-
(site_namesSequence[str], default:None) –Names for each site
Returns:
-
MERRA2LTAAtmosphere–Instance with interpolated climatological data
Examples:
>>> times = pd.date_range("2023-01-01", "2023-12-31", freq="D")
>>> atm = MERRA2LTAAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42,
... site_names="Málaga"
... )
Source code in src/spartasolar/atmoslib/merra2_lta.py
compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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on_regular_grid
classmethod
on_regular_grid(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float],
longitude: Sequence[float],
) -> Self
Retrieve monthly climatology on a regular spatial grid.
Parameters:
-
(timesndarray or DatetimeIndex) –Time stamps for climatology retrieval
-
(latitudeSequence[float]) –Latitude grid coordinates in degrees North
-
(longitudeSequence[float]) –Longitude grid coordinates in degrees East
Returns:
-
MERRA2LTAAtmosphere–Instance with gridded climatological data
Examples:
>>> import numpy as np
>>> lats = np.linspace(36.0, 41.0, 20)
>>> lons = np.linspace(-5.0, -3.0, 20)
>>> times = pd.date_range("2023-01-15", periods=12, freq="MS") + pd.Timedelta(14.5, "d")
>>> atm = MERRA2LTAAtmosphere.on_regular_grid(
... times=times,
... latitude=lats,
... longitude=lons
... )
Source code in src/spartasolar/atmoslib/merra2_lta.py
MERRA-2 via Google Earth Engine
MERRA2GEEAtmosphere
Bases: BaseAtmosphere
MERRA-2 atmospheric database via Google Earth Engine.
Provides access to NASA MERRA-2 reanalysis via GEE API. Automatically corrects for GEE's latitude grid offset and time stamp convention.
Requires GEE authentication and active project configuration.
See module documentation for setup instructions and examples.
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
at_site–Retrieve MERRA-2 data from GEE for a specific site.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
-
distill_crude_data–Refine raw GEE MERRA-2 data for clear-sky modeling.
-
get_filename–Generate cache filename for GEE MERRA-2 data.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
at_site
classmethod
at_site(
times: DatetimeIndex,
latitude: float,
longitude: float,
site_name: str | None = None,
) -> Self
Retrieve MERRA-2 data from GEE for a specific site.
Downloads data from GEE if not cached, applies spatial/temporal corrections, then interpolates to requested times.
Parameters:
-
(timesDatetimeIndex) –Time stamps for data retrieval (UTC)
-
(latitudefloat) –Latitude in degrees North [-90, 90]
-
(longitudefloat) –Longitude in degrees East [-180, 180]
-
(site_namestr, default:None) –Name identifier for the site
Returns:
-
MERRA2GEEAtmosphere–Instance with interpolated atmospheric data
Examples:
>>> import pandas as pd
>>> from spartasolar import config
>>> config.set_option('merra2_gee.project', 'my-gee-project')
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2GEEAtmosphere.at_site(
... times=times,
... latitude=36.72,
... longitude=-4.42,
... site_name="Málaga"
... )
>>> result = atm.compute(model="SPARTA")
Notes
- Requires
merra2_gee.projectconfiguration - Automatically corrects GEE's 0.25° latitude offset
- Adjusts time stamps from hour-start to hour-center
- Data is cached locally to minimize API calls
Source code in src/spartasolar/atmoslib/merra2_geeapi.py
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compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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distill_crude_data
staticmethod
Refine raw GEE MERRA-2 data for clear-sky modeling.
Performs post-processing on GEE data: 1. Adjusts time stamps from hour-start to hour-center (NASA convention) 2. Calculates solar zenith angle for albedo masking 3. Computes Ångström turbidity coefficient (beta) from AOD and alpha 4. Calculates aerosol single-scattering albedo (SSA) 5. Converts ozone from DU to kg/m²
Parameters:
-
(dataDataFrame) –Raw data from GEE API with columns: TOTEXTTAU, TOTSCATAU, TOTANGSTR, PS, TO3, TQV, ALBEDO
-
(latfloat) –Site latitude (for solar position calculation)
-
(lonfloat) –Site longitude (for solar position calculation)
Returns:
-
DataFrame–Processed DataFrame with columns: times_utc, albedo, pressure, ozone, pwater, beta, alpha, ssa
Notes
GEE time stamps are at hour start (e.g., 01:00 UTC), but MERRA-2 hourly averages represent the period centered at half-past (e.g., 01:30 UTC). This function adds 30 minutes to correct the convention.
Albedo is masked to 0 for solar zenith angles > 89°.
Source code in src/spartasolar/atmoslib/merra2_geeapi.py
get_filename
classmethod
Generate cache filename for GEE MERRA-2 data.
Constructs a standardized filename for cached data with encoded coordinates and year.
Parameters:
-
(yearint) –Year for the data
-
(latitudefloat) –Latitude in degrees North [-90, 90]
-
(longitudefloat) –Longitude in degrees East [-180, 180]
Returns:
-
Path–Absolute path to the .parquet cache file
Examples:
>>> path = MERRA2GEEAtmosphere.get_filename(2023, 40.4168, -3.7038)
>>> print(path.name)
# "merra2_gee_hourly_404168N_37038W_2023.parquet"
Source code in src/spartasolar/atmoslib/merra2_geeapi.py
Copernicus CRS via SODA API
CRSSODAAtmosphere
Bases: BaseAtmosphere
CRS SODA (Copernicus Radiation Service) atmospheric database.
Provides access to atmospheric constituent data from the SODA McClear service via WPS API. Data is cached locally after first retrieval.
Requires user registration at https://www.soda-pro.com/ and email
configuration via crs_soda.user_email config option.
See module documentation for examples.
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
at_site–Retrieve CRS SODA atmospheric data for a specific site.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
-
distill_crude_data–Refine and enrich raw CRS data for clear-sky modeling.
-
get_filename–Generate the cache filename for CRS SODA data.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
at_site
classmethod
at_site(
times: DatetimeIndex,
latitude: float,
longitude: float,
site_name: str | None = None,
) -> Self
Retrieve CRS SODA atmospheric data for a specific site.
Downloads data from SODA API if not cached, then interpolates to requested times. Data is automatically resampled to hourly resolution.
Parameters:
-
(timesDatetimeIndex) –Time stamps for data retrieval (UTC)
-
(latitudefloat) –Latitude in degrees North [-90, 90]
-
(longitudefloat) –Longitude in degrees East [-180, 180]
-
(site_namestr, default:None) –Name identifier for the site
Returns:
-
CRSSODAAtmosphere–Instance with interpolated atmospheric data
Examples:
>>> import pandas as pd
>>> from spartasolar import config
>>> config.set_option('crs_soda.user_email', 'user@example.com')
>>>
>>> times = pd.date_range("2020-01-01", "2020-01-31", freq="h")
>>> atm = CRSSODAAtmosphere.at_site(
... times=times,
... latitude=36.72,
... longitude=-4.42,
... site_name="Málaga"
... )
>>> result = atm.compute(model="SPARTA")
Notes
- Requires
crs_soda.user_emailconfiguration - Data is cached locally to minimize API calls
- Temporal interpolation uses quadratic splines
Source code in src/spartasolar/atmoslib/crs_sodaapi.py
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compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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distill_crude_data
staticmethod
Refine and enrich raw CRS data for clear-sky modeling.
Performs post-processing on SODA API data: 1. Calculates AOD550 and estimates Ångström exponent ($\alpha$) using weighted average of aerosol mixture optical properties 2. Estimates surface pressure from site altitude using barometric formula 3. Resamples to 1-hour intervals with center-time alignment
Parameters:
-
(dataDataFrame) –Raw data from SODA API
-
(metadatalist[str]) –Metadata lines from API response (contains altitude)
Returns:
-
DataFrame–Processed DataFrame with columns: times_utc, pressure, albedo, pwater, ozone, aod550, beta, alpha
Notes
The $\alpha$ estimation uses typical values for aerosol species from CAMS Reanalysis: - Desert dust (DU): 0.3 (coarse particles) - Sea salt (SS): 0.5 (large hygroscopic particles) - Black carbon (BC): 1.2 (fine combustion particles) - Organic matter (OR): 1.8 (fine particles) - Sulphates (SU): 1.7 (very fine scatterers) - Nitrates (NI), Ammonium (AM): 1.9
References
.. [1] Bozzo et al. (2017). Implementation of a CAMS-based aerosol climatology in the IFS, ECMWF.
Source code in src/spartasolar/atmoslib/crs_sodaapi.py
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get_filename
classmethod
Generate the cache filename for CRS SODA data.
Constructs a standardized filename pattern for cached data including version, encoded coordinates, and year. Coordinates are multiplied by $10^4$ and suffixed with cardinal direction indicators.
Parameters:
-
(yearint) –Year for the data
-
(latitudefloat) –Latitude in degrees North [-90, 90]
-
(longitudefloat) –Longitude in degrees East [-180, 180]
-
(versionstr) –API version string (e.g., "1.0.0")
Returns:
-
Path–Absolute path to the .parquet cache file
Examples:
>>> path = CRSSODAAtmosphere.get_filename(2023, 40.4168, -3.7038, "1.0.0")
>>> print(path.name)
# "crs_soda_mcclear_v1.0.0_404168N_37038W_2023.parquet"
Notes
Coordinate encoding: - Multiplied by $10^4$ and converted to integers - Signs replaced by suffixes: 'N'/'S' for latitude, 'E'/'W' for longitude - Example: latitude -12.34 becomes "123400S"
Source code in src/spartasolar/atmoslib/crs_sodaapi.py
Custom atmosphere
CustomAtmosphere
Bases: BaseAtmosphere
Custom atmospheric data provider.
This class allows users to supply their own atmospheric constituent data from measurements, numerical weather prediction models, or other sources. Data can be provided for specific sites (time series) or regular grids.
See module documentation for examples.
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
at_sites–Create custom atmospheric data for specific sites.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
-
on_regular_grid–Create custom atmospheric data on a regular spatial grid.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
at_sites
classmethod
at_sites(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float] | float,
longitude: Sequence[float] | float,
constituents: dict[
str, ndarray[tuple[int, int], float]
],
site_names: Sequence[str] | None = None,
var_attrs: dict | None = None,
global_attrs: dict | None = None,
) -> Self
Create custom atmospheric data for specific sites.
Parameters:
-
(timesndarray or DatetimeIndex) –Time stamps for the data (length n_times)
-
(latitudefloat or Sequence[float]) –Latitude(s) in degrees North [-90, 90] (length n_sites)
-
(longitudefloat or Sequence[float]) –Longitude(s) in degrees East [-180, 180] (length n_sites)
-
(constituentsdict[str, ndarray]) –Atmospheric variables as 2D arrays with shape (n_times, n_sites). Standard variable names: 'pressure' (Pa), 'pwater' (cm), 'ozone' (atm-cm), 'alpha', 'beta', 'ssa', 'albedo'
-
(site_namesSequence[str], default:None) –Names for each site
-
(var_attrsdict, default:None) –Custom attributes for variables (CF conventions)
-
(global_attrsdict, default:None) –Custom global attributes for the dataset
Returns:
-
CustomAtmosphere–Instance with atmospheric data loaded
Examples:
>>> times = pd.date_range("2020-01-01", periods=24, freq="h")
>>> atm = CustomAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42,
... constituents={
... "pressure": np.full((24, 1), 101325.0),
... "pwater": np.linspace(1.0, 2.0, 24).reshape(24, 1),
... "ozone": np.full((24, 1), 0.3)
... }
... )
Source code in src/spartasolar/atmoslib/custom.py
compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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on_regular_grid
classmethod
on_regular_grid(
times: ndarray[tuple[int], datetime64] | DatetimeIndex,
latitude: Sequence[float],
longitude: Sequence[float],
constituents: dict[
str, ndarray[tuple[int, int, int], float]
],
var_attrs: dict | None = None,
global_attrs: dict | None = None,
) -> Self
Create custom atmospheric data on a regular spatial grid.
Parameters:
-
(timesndarray or DatetimeIndex) –Time stamps for the data (length n_times)
-
(latitudeSequence[float]) –Latitude coordinates in degrees North (length n_lats)
-
(longitudeSequence[float]) –Longitude coordinates in degrees East (length n_lons)
-
(constituentsdict[str, ndarray]) –Atmospheric variables as 3D arrays with shape (n_times, n_lats, n_lons). Standard names: 'pressure', 'pwater', 'ozone', 'alpha', 'beta', 'ssa', 'albedo'
-
(var_attrsdict, default:None) –Custom variable attributes
-
(global_attrsdict, default:None) –Custom global dataset attributes
Returns:
-
CustomAtmosphere–Instance with gridded atmospheric data
Examples:
>>> lats = np.linspace(36.0, 41.0, 20)
>>> lons = np.linspace(-5.0, -3.0, 20)
>>> times = pd.date_range("2020-06-15", periods=5, freq="h")
>>> atm = CustomAtmosphere.on_regular_grid(
... times=times,
... latitude=lats,
... longitude=lons,
... constituents={
... "pressure": np.full((5, 20, 20), 101325.0),
... "pwater": np.random.uniform(1.0, 3.0, (5, 20, 20)),
... }
... )
Source code in src/spartasolar/atmoslib/custom.py
Base class
BaseAtmosphere
Abstract base class for atmospheric database interfaces.
This class defines the common interface that all atmospheric data sources must implement. It provides methods for loading atmospheric constituent data and computing clear-sky solar radiation using various radiative transfer models.
Subclasses must implement methods to retrieve atmospheric data either at specific sites (time series) or on regular grids. The class handles: - Loading and validation of atmospheric datasets - Integration with solar position calculations - Execution of clear-sky radiation models (SPARTA, Bird, etc.) - CF-compliant metadata management
Attributes:
-
database_path(Path or None) –Directory containing the database files (set by subclass)
-
dataset(Dataset) –The loaded atmospheric dataset
Examples:
Subclasses should define database_path and implement data retrieval:
>>> class MyAtmosphere(BaseAtmosphere, database_path="/path/to/data"):
... @classmethod
... def at_sites(cls, times, latitude, longitude, **kwargs):
... # Implementation here
... pass
Notes
This is an abstract base class and cannot be instantiated directly. Use concrete implementations like MERRA2DailyAtmosphere or CustomAtmosphere.
See Also
MERRA2DailyAtmosphere : Most commonly used implementation CustomAtmosphere : For user-provided data
Validates that the database path exists (if specified) and initializes the internal atmosphere dataset to None.
Raises:
-
AttributeError–If database_path is specified but does not exist
Methods:
-
__init_subclass__–Automatically sets the database path for subclasses.
-
compute–Compute clear-sky solar radiation using a radiative transfer model.
Source code in src/spartasolar/atmoslib/_base.py
__init_subclass__
__init_subclass__(database_path: str, **kwargs)
Automatically sets the database path for subclasses.
Parameters:
-
(database_pathstr or None) –The directory path where the specific atmosphere data is stored. Pass
Nonefor sources that do not use a file database (e.g.CustomAtmosphereor API-based retrievers).
Source code in src/spartasolar/atmoslib/_base.py
compute
compute(
model: Model = "SPARTA",
include_atmosphere: bool = False,
model_kwargs: dict | None = None,
) -> Dataset
Compute clear-sky solar radiation using a radiative transfer model.
This method integrates solar position calculations with atmospheric constituent data to compute clear-sky irradiance components (GHI, DNI, DHI, etc.) using the specified radiative transfer model.
Parameters:
-
(modelModel, default:"SPARTA") –Name of the clear-sky model to use. Options: "SPARTA", "Bird"
-
(include_atmospherebool, default:False) –If True, include atmospheric constituents in the output dataset. If False, only radiation components are returned.
-
(model_kwargsdict, default:None) –Additional keyword arguments to pass to the model function
Returns:
-
Dataset–CF-compliant dataset containing computed irradiance components: - ghi: Global Horizontal Irradiance (W/m²) - dni: Direct Normal Irradiance (W/m²) - dhi or dif: Diffuse Horizontal Irradiance (W/m²) - csi: Circumsolar Irradiance (W/m², SPARTA only)
Examples:
>>> import pandas as pd
>>> from spartasolar.atmoslib import MERRA2DailyAtmosphere
>>>
>>> times = pd.date_range("2020-06-15", periods=24, freq="h")
>>> atm = MERRA2DailyAtmosphere.at_sites(
... times=times,
... latitude=36.72,
... longitude=-4.42
... )
>>> result = atm.compute(model="SPARTA")
>>> print(result.ghi.values)
Use different model with custom parameters:
>>> result = atm.compute(
... model="Bird",
... model_kwargs={"scheme": "transmittance_parameterization"}
... )
Notes
The method automatically: - Calculates solar position (zenith angle, Earth-Sun distance) - Converts atmospheric units to model requirements - Handles both gridded and site-based data structures
See Also
spartasolar.modlib.sparta : SPARTA model implementation spartasolar.modlib.bird : Bird clear-sky model
Source code in src/spartasolar/atmoslib/_base.py
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Clear-sky models
SPARTA
SPARTA
SPARTA(
cosz: float | ndarray = 0.5,
pressure: float | ndarray = 1013.25,
albedo: float | ndarray = 0.2,
pwater: float | ndarray = 1.4,
ozone: float | ndarray = 0.3,
beta: float | ndarray = 0.1,
alpha: float | ndarray = 1.3,
ssa: float | ndarray = 0.92,
asy: float | ndarray = 0.65,
ecf: float | ndarray = 1.0,
csi_param: str = "sparta",
csi_hfov: float = 2.5,
transmittance_scheme: str = "interdependent",
) -> dict[str, ndarray]
Compute clear-sky solar irradiance using the SPARTA model.
SPARTA (Solar PArameterization of the Radiative Transfer of the Atmosphere) is a high-accuracy 2-band broadband clear-sky model that computes direct, diffuse, global, and circumsolar irradiance. The model is fully vectorized and handles nighttime masking automatically.
Parameters:
-
(coszfloat or ndarray, default:0.5) –Cosine of the solar zenith angle [0, 1]. Values ≤ cos(90.5°) ≈ 0.00872 are treated as nighttime.
-
(pressurefloat or ndarray, default:1013.25) –Atmospheric surface pressure in hPa (or mb). Typical range: 800-1100 hPa.
-
(albedofloat or ndarray, default:0.2) –Ground surface albedo [0, 1]. Typical values: 0.1-0.3 (vegetation), 0.6-0.9 (snow), 0.05-0.15 (water).
-
(pwaterfloat or ndarray, default:1.4) –Precipitable water vapor in cm. Typical range: 0.5-6.0 cm.
-
(ozonefloat or ndarray, default:0.3) –Total column ozone in atm-cm. Note: 1 atm-cm = 1000 DU (Dobson Units). Typical range: 0.2-0.5 atm-cm (200-500 DU).
-
(betafloat or ndarray, default:0.1) –Ångström turbidity coefficient (aerosol optical depth at 1000 nm). Automatically clipped to [0, 2.2]. Typical range: 0.02-0.5.
-
(alphafloat or ndarray, default:1.3) –Ångström wavelength exponent. Automatically clipped to [0, 2.5]. Typical values: 0.5-1.0 (coarse aerosols), 1.5-2.0 (fine aerosols).
-
(ssafloat or ndarray, default:0.92) –Aerosol single-scattering albedo at ~700 nm [0, 1]. Typical values: 0.85-0.95 (urban), 0.95-0.99 (desert dust).
-
(asyfloat or ndarray, default:0.65) –Aerosol asymmetry parameter at ~700 nm [-1, 1]. Typical range: 0.6-0.8.
-
(ecffloat or ndarray, default:1.0) –Eccentricity correction factor for Sun-Earth distance. Range: ~0.967 (early July) to ~1.034 (early January).
-
(csi_paramstr, default:'sparta') –Circumsolar irradiance parameterization method: - 'none': Neglects circumsolar component - 'sparta': Uses SPARTA native parameterization (recommended)
-
(csi_hfovfloat, default:2.5) –Half field of view angle in degrees for circumsolar evaluation. Typical pyrheliometer values: 2.5° (standard), 2.9° (some instruments).
-
(transmittance_schemestr, default:'interdependent') –Method for computing atmospheric transmittances: - 'independent': Treats each constituent separately (faster, less accurate) - 'interdependent': Accounts for constituent interactions (more accurate)
Returns:
-
dict[str, float or ndarray]–Dictionary with the following irradiance components (all in W/m²):
- 'dni': Direct Normal Irradiance (beam on plane perpendicular to sun)
- 'dhi': Direct Horizontal Irradiance (beam on horizontal plane)
- 'dif': Diffuse Horizontal Irradiance (scattered radiation)
- 'ghi': Global Horizontal Irradiance (total on horizontal plane)
- 'csi': Circumsolar Normal Irradiance (forward-scattered aureole)
Examples:
Single location and time:
>>> from spartasolar.modlib import SPARTA
>>> result = SPARTA(
... cosz=0.866, # 30° solar zenith angle
... pressure=1013.25,
... pwater=2.0,
... ozone=0.3,
... beta=0.1,
... alpha=1.3
... )
>>> print(f"DNI: {result['dni']:.1f} W/m²")
>>> print(f"GHI: {result['ghi']:.1f} W/m²")
Vectorized computation for time series:
>>> import numpy as np
>>> # Simulate conditions at different solar elevations
>>> zenith_angles = np.linspace(0, 85, 20) # degrees
>>> cosz_values = np.cos(np.radians(zenith_angles))
>>>
>>> result = SPARTA(
... cosz=cosz_values,
... pressure=1013.25,
... pwater=np.linspace(1.0, 3.0, 20), # varying water vapor
... ozone=0.3,
... beta=0.08,
... alpha=1.4
... )
>>> print(result['ghi'].shape) # (20,)
High aerosol loading scenario:
>>> result = SPARTA(
... cosz=0.7,
... beta=0.5, # high turbidity
... alpha=0.8, # coarse particles
... ssa=0.88, # slightly absorbing
... csi_param='sparta'
... )
>>> csi_fraction = result['csi'] / result['dni']
>>> print(f"CSI fraction: {csi_fraction:.2%}")
Disable circumsolar correction:
Notes
- Solar constant used: 1361.1 W/m²
- Nighttime threshold: cosz ≤ cos(90.5°) ≈ 0.00872
- All input arrays are automatically broadcast to compatible shapes
- Invalid/missing values (-999, NaN) are handled gracefully
- The 'interdependent' scheme is recommended for highest accuracy
The model has been validated against radiative transfer simulations and ground measurements, showing typical errors < 2% for GHI and DNI under most atmospheric conditions.
See Also
spartasolar.modlib.bird : Alternative Bird clear-sky model
References
.. [1] Ruiz-Arias, J. A. (2023). SPARTA: Solar parameterization for the radiative transfer of the cloudless atmosphere. Renewable and Sustainable Energy Reviews*, 188, 113833. https://doi.org/10.1016/j.rser.2023.113833
Source code in src/spartasolar/modlib/sparta.py
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Bird & Hulstrom
BIRD
BIRD(
cosz: float | ndarray = 0.5,
pressure: float | ndarray = 1013.25,
albedo: float | ndarray = 0.2,
pwater: float | ndarray = 1.4,
ozone: float | ndarray = 0.3,
beta: float | ndarray = 0.1,
alpha: float | ndarray = 1.3,
ssa: float | ndarray = 0.92,
asy: float | ndarray = 0.65,
ecf: float | ndarray = 1.0,
) -> dict[str, ndarray]
Calculates solar irradiance using the Bird & Hulstrom model.
The model estimates solar radiation through individual transmittance processes for Rayleigh scattering, ozone absorption, uniformly mixed gases, water vapor, and aerosol extinction. It also accounts for multiple reflections between the ground and the sky.
Args: cosz: Cosine of the solar zenith angle. pressure: Atmospheric surface pressure in hPa. albedo: Ground surface albedo (0 to 1). pwater: Precipitable water in cm. ozone: Ozone vertical pathlength in atm-cm (1 atm-cm = 1000 DU). beta: Ångström's turbidity coefficient (AOD at 1000 nm). alpha: Ångström's wavelength exponent. ssa: Aerosol single-scattering albedo at ~700 nm. asy: Aerosol asymmetry parameter. ecf: Eccentricity correction factor for the Sun-Earth orbit.
Returns:
dict[str, np.ndarray]: A dictionary containing:
- dni: Direct normal irradiance [W/m²].
- dhi: Direct horizontal irradiance [W/m²].
- dif: Diffuse horizontal irradiance [W/m²].
- ghi: Global horizontal irradiance [W/m²].
Notes: - The model uses a fixed solar constant ((G_{sc})) of 1353 W/m². - Nighttime values are automatically masked (set to 0) for zenith angles greater than 90.5°. - The algorithm includes a 0.9662 correction factor for the direct normal component as per the original publication.
References: - Bird, R. E., & Hulstrom, R. L. (1981). A simplified clear sky model for direct and diffuse insolation on horizontal surfaces. Solar Energy Research Institute (SERI).
Source code in src/spartasolar/modlib/bird.py
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Configuration
config
Configuration Management for SPARTA-Solar.
This module handles the persistent storage and retrieval of user settings using a TOML configuration file located in the standard user configuration directory.
The configuration system manages: - API credentials (e.g., SODA's user email) - Local storage paths for cached data - Algorithm preferences (e.g., solar position algorithm) - Service-specific settings
Configuration Flow: 1. On first import, checks if config file exists 2. If not found, creates it with default template 3. Loads configuration into memory (_GLOBAL_CONFIG) 4. Changes via set_option() are session-only 5. Persistent changes require manual editing of config.toml
Configuration File Location:
- Linux: ~/.config/spartasolar/config.toml
- macOS: ~/Library/Application Support/spartasolar/config.toml
- Windows: C:\Users\
Examples: >>> from spartasolar.config import get_config_path, get_option, set_option
>>> # Get configuration file path
>>> config_path = get_config_path()
>>> print(config_path)
PosixPath('/home/user/.config/spartasolar/config.toml')
>>> # Retrieve an option
>>> email = get_option('crs_soda.user_email')
>>> # Set option for current session only
>>> set_option('sunwhere.algorithm', 'spa')
>>> # Get data directory (returns Path object)
>>> data_dir = get_option('merra2_daily.data_dir')
See Also: - get_config_path(): Get path to configuration file - get_option(): Retrieve configuration value - set_option(): Modify configuration (session only) - show_config(): Display all current settings
Functions:
-
get_config_path–Get the path to the user's configuration file.
-
get_option–Retrieve the value of a specific configuration option.
-
set_option–Temporarily update a global option for the current session.
-
show_config–Print all current global options to the console.
get_config_path
get_config_path() -> Path
Get the path to the user's configuration file.
Returns:
Path: The absolute path to config.toml within the standard
system-specific user configuration directory.
Source code in src/spartasolar/config.py
get_option
Retrieve the value of a specific configuration option.
Options are organized in tables (sections) within the TOML file. This function uses dot notation to access nested values.
Args:
name: The name of the option to retrieve using the format
<table-name>.<option-name> (e.g., 'crs_soda.user_email').
default: Value to return if the option is not found. Defaults to None.
Returns:
Any: The value of the option. Returns default if the option
is missing. Special case: options named 'data_dir' are
automatically converted to Path objects.
Examples: >>> from spartasolar.config import get_option
>>> # Get solar position algorithm
>>> algorithm = get_option('sunwhere.algorithm')
>>> print(algorithm)
'psa'
>>> # Get with default value
>>> email = get_option('crs_soda.user_email', default='user@example.com')
>>> # Data directories return Path objects
>>> from pathlib import Path
>>> data_dir = get_option('merra2_daily.data_dir')
>>> isinstance(data_dir, (Path, type(None)))
True
Source code in src/spartasolar/config.py
set_option
Temporarily update a global option for the current session.
Modifies configuration values in memory only. Changes are lost when the Python session ends. To make persistent changes, edit the config.toml file directly.
Args:
name: The name of the option to update in format <table>.<option>.
value: The new value to assign. Path objects for 'data_dir' options
are automatically converted to strings.
Returns: None
Warning: Session-only changes are NOT saved to the config file. Restart the Python session to revert to file values.
Examples: >>> from spartasolar.config import set_option, get_option
>>> # Change solar position algorithm
>>> set_option('sunwhere.algorithm', 'spa')
>>> get_option('sunwhere.algorithm')
'spa'
>>> # Set data directory with Path object
>>> from pathlib import Path
>>> set_option('merra2_daily.data_dir', Path('/custom/path'))
Note: To persist changes, manually edit the configuration file at the path returned by get_config_path().
Source code in src/spartasolar/config.py
show_config
Print all current global options to the console.
Note:
This function uses pprint for a formatted output of the
global configuration state.