Source code for pygmt.src.filter1d

"""
filter1d - Time domain filtering of 1-D data tables
"""

from typing import Literal

import numpy as np
import pandas as pd
from pygmt.clib import Session
from pygmt.exceptions import GMTInvalidInput
from pygmt.helpers import (
    build_arg_list,
    fmt_docstring,
    use_alias,
    validate_output_table_type,
)


[docs] @fmt_docstring @use_alias( E="end", F="filter_type", N="time_col", ) def filter1d( data, output_type: Literal["pandas", "numpy", "file"] = "pandas", outfile: str | None = None, **kwargs, ) -> pd.DataFrame | np.ndarray | None: r""" Time domain filtering of 1-D data tables. A general time domain filter for multiple column time series data. The user specifies which column is the time (i.e., the independent variable) via ``time_col``. The fastest operation occurs when the input time series are equally spaced and have no gaps or outliers and the special options are not needed. Read a table and output as a :class:`numpy.ndarray`, :class:`pandas.DataFrame`, or ASCII file. Full option list at :gmt-docs:`filter1d.html` {aliases} Parameters ---------- {output_type} {outfile} filter_type : str **type**\ *width*\ [**+h**]. Set the filter **type**. Choose among convolution and non-convolution filters. Append the filter code followed by the full filter *width* in same units as time column. By default, this performs a low-pass filtering; append **+h** to select high-pass filtering. Some filters allow for optional arguments and a modifier. Available convolution filter types are: - **b**: boxcar. All weights are equal. - **c**: cosine arch. Weights follow a cosine arch curve. - **g**: Gaussian. Weights are given by the Gaussian function. - **f**: custom. Instead of *width* give name of a one-column file with your own weight coefficients. Non-convolution filter types are: - **m**: median. Returns median value. - **p**: maximum likelihood probability (a mode estimator). Return modal value. If more than one mode is found we return their average value. Append **+l** or **+u** if you rather want to return the lowermost or uppermost of the modal values. - **l**: lower (absolute). Return the minimum of all values. - **L**: lower. Return minimum of all positive values only. - **u**: upper (absolute). Return maximum of all values. - **U**: upper. Return maximum of all negative values only. Upper case type **B**, **C**, **G**, **M**, **P**, **F** will use robust filter versions: i.e., replace outliers (2.5 L1 scale off median, using 1.4826 \* median absolute deviation [MAD]) with median during filtering. In the case of **L**\|\ **U** it is possible that no data passes the initial sign test; in that case the filter will return 0.0. Apart from custom coefficients (**f**), the other filters may accept variable filter widths by passing *width* as a two-column time-series file with filter widths in the second column. The filter-width file does not need to be co-registered with the data as we obtain the required filter width at each output location via interpolation. For multi-segment data files the filter file must either have the same number of segments or just a single segment to be used for all data segments. end : bool Include ends of time series in output. The default [False] loses half the filter-width of data at each end. time_col : int Indicate which column contains the independent variable (time). The left-most column is 0, while the right-most is (*n_cols* - 1) [Default is ``0``]. Returns ------- ret Return type depends on ``outfile`` and ``output_type``: - None if ``outfile`` is set (output will be stored in file set by ``outfile``) - :class:`pandas.DataFrame` or :class:`numpy.ndarray` if ``outfile`` is not set (depends on ``output_type``) """ if kwargs.get("F") is None: raise GMTInvalidInput("Pass a required argument to 'filter_type'.") output_type = validate_output_table_type(output_type, outfile=outfile) with Session() as lib: with ( lib.virtualfile_in(check_kind="vector", data=data) as vintbl, lib.virtualfile_out(kind="dataset", fname=outfile) as vouttbl, ): lib.call_module( module="filter1d", args=build_arg_list(kwargs, infile=vintbl, outfile=vouttbl), ) return lib.virtualfile_to_dataset(vfname=vouttbl, output_type=output_type)