solarwindpy.fitfunctions.power_laws.PowerLawPlusC
- class PowerLawPlusC(xobs, yobs, **kwargs)[source]
Bases:
FitFunctionAssuming that you don’t want special formatting, call order is:
fit_function = FitFunction(function, TeX_string) fit_function.make_fit()
Instances are callable. If the fit fails, calling the instance will return an array of NaNs the same shape as the x-values.
- __init__(xobs, yobs, **kwargs)[source]
Initialize a power law with constant offset.
- Parameters:
xobs (array-like) – Observed values to fit.
yobs (array-like) – Observed values to fit.
yobs – Observed y values (dependent variable). Shape must match xobs.
**kwargs (dict) – Forwarded to
FitFunction.
Notes
The fitting procedure uses scipy.optimize.least_squares with robust loss functions (Huber by default) to handle outliers. The initial parameter guess is provided by the p0 property, which must be implemented by subclasses.
All subclasses inherit this documentation automatically through the docstring-inheritance metaclass.
Examples
>>> import numpy as np >>> from solarwindpy.fitfunctions import Gaussian >>> x = np.linspace(-5, 5, 100) >>> y = 3 * np.exp(-0.5 * x**2) + np.random.normal(0, 0.1, 100) >>> fit = Gaussian(x, y, xmin=-3, xmax=3) >>> fit.make_fit() >>> print(f"Fitted mu: {fit.popt['mu']:.3f}")
- property function
Get the function that`curve_fit` fits.
The function is set at instantiation. It doesn’t make sense to change it unless you redefine the entire FitFunction, so there is no new kwarg.
- property p0
Return initial guesses
[A, b, c]for the fit.
- property TeX_function
Function written in LaTeX.
- property TeX_info
- property argnames
The names of the actual function arguments pulled by getfullargspec.
- build_TeX_info()
- build_plotter()
- property chisq_dof
Chisq per degree of freedom \(\chi^2_\nu\).
If None, not calculated by make_fit_old. If np.nan, fit failed.
- property combined_popt_psigma
Return optimized parameters and uncertainties as a DataFrame.
- Returns:
DataFrame with columns ‘popt’ and ‘psigma’, indexed by parameter names. Relative uncertainty can be computed as: df[‘psigma’] / df[‘popt’]
- Return type:
pd.DataFrame
- property dof
Degrees of freedom in the fit.
- property fit_bounds
Bounds used when running the fit.
- property fit_result
- property initial_guess_info
- property logger
- make_fit(return_exception=False, **kwargs)
Fit the function with the independent xobs and dependent yobs.
Uses least_squares and returns the OptimizeResult object, but treats weights as in curve_fit.
- Parameters:
return_exception (bool) – If True, return exceptions from fitting routine, instead of raising. This is useful when looping through many fits and wanting to identify failed fits after the fact.
**kwargs – The description is missing.
- property nobs
The total number of observations used in the fit.
- property observations
- property pcov
Returns a copy so that the matrix isn’t accidentally edited.
- property plotter
- property popt
Optimized fit parameters.
- property psigma
- residuals(pct=False, use_all=False)
Calculate fit residuals.
- Parameters:
- Returns:
Residuals as observed - fitted.
- Return type:
Examples
>>> # Create FitFunction with constraints >>> ff = Gaussian(x, y, xmin=3, xmax=7) >>> ff.make_fit() >>> >>> # Residuals for fitted region only >>> r_fit = ff.residuals() >>> >>> # Residuals for all original data >>> r_all = ff.residuals(use_all=True) >>> >>> # Percentage residuals >>> r_pct = ff.residuals(pct=True)
Notes
Addresses TODO: “calculate with all values…including those excluded by set_extrema” (though set_extrema doesn’t exist - constraints are passed in __init__).
- property rsq
Coefficient of determination.
Source: <en.wikipedia.org/wiki/Coefficient_of_determination#Definitions>
- set_fit_obs(xobs_raw, yobs_raw, weights_raw, xmin=None, xmax=None, xoutside=None, ymin=None, ymax=None, youtside=None, wmin=None, wmax=None, logx=False, logy=False)
Set the observed values we’ll actually use in the fit.
By applying limits to xobs_raw and yobs_raw and checking for finite values.
All boundaries are inclusive <= or >=.
If logy, then make selection of wmin and wmax based on \(w/(y \ln(10))\).
- Parameters:
xobs_raw – The description is missing.
yobs_raw – The description is missing.
weights_raw – The description is missing.
xmin – The description is missing.
xmax – The description is missing.
xoutside – The description is missing.
ymin – The description is missing.
ymax – The description is missing.
youtside – The description is missing.
wmin – The description is missing.
wmax – The description is missing.
logx – The description is missing.
logy – The description is missing.
- property sufficient_data
Ensure that we can fit the data before doing any computations.