Source code for pyrfu.pyrf.dec_par_perp

#!/usr/bin/env python
# -*- coding: utf-8 -*-


from typing import Tuple

# 3rd party imports
import numpy as np
import xarray as xr
from xarray.core.dataarray import DataArray

# Local imports
from pyrfu.pyrf.resample import resample
from pyrfu.pyrf.ts_scalar import ts_scalar
from pyrfu.pyrf.ts_vec_xyz import ts_vec_xyz

__author__ = "Louis Richard"
__email__ = "louisr@irfu.se"
__copyright__ = "Copyright 2020-2024"
__license__ = "MIT"
__version__ = "2.4.2"
__status__ = "Prototype"


[docs]def dec_par_perp( inp: DataArray, b_bgd: DataArray, flag_spin_plane: bool = False ) -> Tuple[DataArray, DataArray, DataArray]: r"""Decomposes a vector into par/perp to B components. If flagspinplane decomposes components to the projection of ``b0`` into the XY plane. ``alpha`` gives the angle between ``b0`` and the XY. plane. Parameters ---------- inp : xarray.DataArray Time series of the field to decompose. b_bgd : xarray.DataArray Time series of the background magnetic field. flag_spin_plane : bool, Optional Flag if True gives the projection in XY plane. Returns ------- a_para : xarray.DataArray Time series of the input field parallel to the background magnetic field. a_perp : xarray.DataArray Time series of the input field perpendicular to the background magnetic field. alpha : xarray.DataArray Time series of the angle between the background magnetic field and the XY plane. Examples -------- >>> from pyrfu import mms, pyrf Time interval >>> tint = ["2019-09-14T07:54:00.000", "2019-09-14T08:11:00.000"] Spacecraft index >>> mms_id = 1 Load magnetic field (FGM) and electric field (EDP) >>> b_xyz = mms.get_data("B_gse_fgm_brst_l2", tint, mms_id) >>> e_xyz = mms.get_data("E_gse_edp_brst_l2", tint, mms_id) Decompose e_xyz into parallel and perpendicular to b_xyz components >>> e_para, e_perp, _ = pyrf.dec_par_perp(e_xyz, b_xyz) """ # Check arguments types assert isinstance(inp, xr.DataArray), "inp must be an xarray.DataArray" assert isinstance(b_bgd, xr.DataArray), "b_bgd must be an xarray.DataArray" assert isinstance(flag_spin_plane, bool), "flag_spin_plane must be boolean" # Check inp and b_bgd shapes assert inp.ndim == 2 and inp.shape[1], "inp must be a vector" assert b_bgd.ndim == 2 and b_bgd.shape[1], "b_bgd must be a vector" # Resample background magnetic field to input b_bgd = resample(b_bgd, inp) # Get times and data inp_time = inp.time.data inp_data = inp.data b_bgd_data = b_bgd.data if not flag_spin_plane: b_mag = np.linalg.norm(b_bgd_data, axis=1, keepdims=True) indices = np.where(b_mag < 1e-3)[0] if indices.size > 0: b_mag[indices] = 1e-3 * np.ones((len(indices), 1)) b_hat = b_bgd_data / b_mag a_para_arr = np.sum(b_hat * inp_data, axis=-1) a_para = ts_scalar(inp_time, a_para_arr) a_perp_arr = inp_data - ( b_hat * np.tile(a_para_arr[:, np.newaxis], (1, inp_data.shape[1])) ) a_perp = ts_vec_xyz(inp_time, a_perp_arr) alpha_arr = np.zeros_like(a_para_arr) alpha = ts_scalar(inp_time, alpha_arr) else: b_tot = np.sqrt(b_bgd_data[:, 0] ** 2 + b_bgd_data[:, 1] ** 2) b_hat = b_bgd_data / b_tot[:, np.newaxis] a_para_arr = inp_data[:, 0] * b_hat[:, 0] + inp_data[:, 1] * b_hat[:, 1] a_para = ts_scalar(inp_time, a_para_arr) a_perp_arr = inp_data[:, 0] * b_hat[:, 1] - inp_data[:, 1] * b_hat[:, 0] a_perp = ts_scalar(inp_time, a_perp_arr) alpha_arr = np.arctan2(b_bgd_data[:, 2], b_tot) alpha = ts_scalar(inp_time, alpha_arr) return a_para, a_perp, alpha