Source code for pyrfu.pyrf.calc_agyro

#!/usr/bin/env python

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

# Local imports
from pyrfu.pyrf.ts_scalar import ts_scalar

__author__ = "Louis Richard"
__email__ = "louisr@irfu.se"
__copyright__ = "Copyright 2020-2024"
__license__ = "MIT"
__version__ = "2.4.13"
__status__ = "Prototype"


[docs]def calc_agyro(p_xyz: DataArray) -> DataArray: r"""Compute agyrotropy coefficient as .. math:: A\Phi = \frac{|P_{\perp 1} - P_{\perp 2}|}{P_{\perp 1} + P_{\perp 2}} Parameters ---------- p_xyz : DataArray Time series of the pressure tensor Returns ------- DataArray Time series of the agyrotropy coefficient of the specie. Raises ------ TypeError If input is not a xarray.DataArray. ValueError If input is not a time series of a tensor (n_time, 3, 3). Examples -------- >>> from pyrfu import mms, pyrf Time interval >>> tint = ["2019-09-14T07:54:00.000","2019-09-14T08:11:00.000"] Spacecraft index >>> ic = 1 Load magnetic field and electron pressure tensor >>> b_xyz = mms.get_data("b_gse_fgm_srvy_l2", tint, 1) >>> p_xyz_e = mms.get_data("pe_gse_fpi_fast_l2", tint, 1) Rotate electron pressure tensor to field aligned coordinates >>> p_fac_e_qq = mms.rotate_tensor(p_xyz_e, "fac", b_xyz, "qq") Compute agyrotropy coefficient >>> agyro_e = pyrf.calc_agyro(p_fac_e_qq) """ # Check input type if not isinstance(p_xyz, xr.DataArray): raise TypeError("p_xyz must be a xarray.DataArray") # Check input shape if p_xyz.data.ndim != 3 or p_xyz.shape[1] != 3 or p_xyz.shape[2] != 3: raise ValueError("p_xyz must be a time series of a tensor") # Parallel and perpendicular components p_perp_1, p_perp_2 = [p_xyz.data[:, 1, 1], p_xyz.data[:, 2, 2]] agyrotropy = np.abs(p_perp_1 - p_perp_2) / (p_perp_1 + p_perp_2) agyrotropy = ts_scalar(p_xyz.time.data, agyrotropy) return agyrotropy