Source code for pyrfu.pyrf.calc_sqrtq

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

# 3rd party imports
import numpy as np
import xarray as xr

# Local imports
from .ts_scalar import ts_scalar

__author__ = "Louis Richard"
__email__ = "louisr@irfu.se"
__copyright__ = "Copyright 2020-2023"
__license__ = "MIT"
__version__ = "2.4.2"
__status__ = "Prototype"


[docs]def calc_sqrtq(p_xyz): r"""Computes agyrotropy coefficient as in [1]_ .. math:: Q = \frac{P_{12}^2 + P_{13}^2 + P_{23}^2} {P_\perp^2 + 2 P_\perp P_\parallel} Parameters ---------- p_xyz : xarray.DataArray Time series of the pressure tensor Returns ------- sqrt_q : xarray.DataArray Time series of the agyrotropy coefficient of the specie References ---------- .. [1] Swisdak, M. (2016), Quantifying gyrotropy in magnetic reconnection, Geophys. Res.Lett., 43, 43–49, doi: https://doi.org/10.1002/2015GL066980. 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_pp = mms.rotate_tensor(p_xyz_e, "fac", b_xyz, "pp") Compute agyrotropy coefficient >>> sqrt_q_e = pyrf.calc_sqrtq(p_fac_e_pp) """ # Check input type assert isinstance(p_xyz, xr.DataArray), "p_xyz must be a xarray.DataArray" # Check import shape message = "p_xyz must be a time series of a tensor" assert p_xyz.data.ndim == 3 and p_xyz.shape[1] == 3 and p_xyz.shape[2] == 3, message # Parallel and perpendicular components p_para = p_xyz.data[:, 0, 0] p_perp = (p_xyz.data[:, 1, 1] + p_xyz.data[:, 2, 2]) / 2 # Off-diagonal terms p_12, p_13, p_23 = [p_xyz.data[:, 0, 1], p_xyz.data[:, 0, 2], p_xyz.data[:, 1, 2]] sqrt_q = np.sqrt(p_12**2 + p_13**2 + p_23**2) sqrt_q /= np.sqrt(p_perp**2 + 2 * p_perp * p_para) sqrt_q = ts_scalar(p_xyz.time.data, sqrt_q) return sqrt_q