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# -*- coding: utf-8 -*- |
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# Copyright (c) 2022 Stefan Bender |
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# |
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# This module is part of pyspaceweather. |
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# pyspaceweather is free software: you can redistribute it or modify |
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# it under the terms of the GNU General Public License as published |
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# by the Free Software Foundation, version 2. |
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# See accompanying COPYING.GPLv2 file or http://www.gnu.org/licenses/gpl-2.0.html. |
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"""Python interface for OMNI space weather data |
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Omni2 [#]_ space weather data interface for python. |
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.. [#] https://omniweb.gsfc.nasa.gov/ow.html |
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""" |
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import os |
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from pkg_resources import resource_filename |
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import logging |
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from warnings import warn |
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import numpy as np |
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import pandas as pd |
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from .core import _assert_file_exists, _dl_file |
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__all__ = [ |
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"cache_omnie", |
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"omnie_hourly", |
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"omnie_mask_missing", |
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"read_omnie", |
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] |
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OMNI_URL_BASE = "https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/extended" |
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OMNI_PREFIX, OMNI_EXT = "omni2", "dat" |
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OMNI_SUBDIR = "omni_extended" |
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LOCAL_PATH = resource_filename(__name__, os.path.join("data", OMNI_SUBDIR)) |
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_OMNI_MISSING = { |
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"year": None, |
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"doy": None, |
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"hour": None, |
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"bsrn": 9999, |
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"id_imf": 99, |
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"id_sw": 99, |
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"n_imf": 999, |
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"n_plasma": 999, |
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"B_mag_avg": 999.9, |
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"B_mag": 999.9, |
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"theta_B": 999.9, |
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"phi_B": 999.9, |
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"B_x": 999.9, |
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"B_y_GSE": 999.9, |
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"B_z_GSE": 999.9, |
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"B_y_GSM": 999.9, |
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"B_z_GSM": 999.9, |
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"sigma_B_mag_avg": 999.9, |
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"sigma_B_mag": 999.9, |
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"sigma_B_x_GSE": 999.9, |
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"sigma_B_y_GSE": 999.9, |
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"sigma_B_z_GSE": 999.9, |
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"T_p": 9999999.0, |
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"n_p": 999.9, |
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"v_plasma": 9999.0, |
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"phi_v": 999.9, |
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"theta_v": 999.9, |
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"n_alpha_n_p": 9.999, |
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"p_flow": 99.99, |
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"sigma_T": 9999999.0, |
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"sigma_n": 999.9, |
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"sigma_v": 9999.0, |
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"sigma_phi_v": 999.9, |
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"sigma_theta_v": 999.9, |
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"sigma_na_np": 9.999, |
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"E": 999.99, |
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"beta_plasma": 999.99, |
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"mach": 999.9, |
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"Kp": 9.9, |
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"R": 999, |
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"Dst": 99999, |
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"AE": 9999, |
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"p_01MeV": 999999.99, |
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"p_02MeV": 99999.99, |
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"p_04MeV": 99999.99, |
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"p_10MeV": 99999.99, |
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"p_30MeV": 99999.99, |
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"p_60MeV": 99999.99, |
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"flag": 0, |
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"Ap": 999, |
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"f107_adj": 999.9, |
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"PC": 999.9, |
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"AL": 99999, |
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"AU": 99999, |
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"mach_mag": 99.9, |
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"Lya": 0.999999, |
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"QI_p": 9.9999 |
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} |
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def cache_omnie( |
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year, |
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prefix=None, |
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ext=None, |
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local_path=None, |
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url_base=None, |
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): |
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"""Download OMNI2 data to local cache |
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Downloads the OMNI2 (extended) data file from [#]_ to the local location. |
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.. [#] https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/extended/ |
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Parameters |
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---------- |
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year: int |
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Year of the data. |
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prefix: str, optional |
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File prefix for constructing the file name as <prefix>_year.<ext>. |
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Defaults to 'omni2'. |
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ext: str, optional |
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File extension for constructing the file name as <prefix>_year.<ext>. |
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Defaults to 'dat'. |
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local_path: str, optional |
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Path to the locally stored data yearly files, defaults to the |
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data location within the package. |
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url_base: str, optional |
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URL for the directory that contains the yearly files. |
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Returns |
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------- |
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Nothing. |
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""" |
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prefix = prefix or OMNI_PREFIX |
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ext = ext or OMNI_EXT |
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local_path = local_path or LOCAL_PATH |
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url_base = url_base or OMNI_URL_BASE |
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basename = "{0}_{1:04d}.{2}".format(prefix, year, ext) |
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if not os.path.exists(local_path): |
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os.makedirs(local_path) |
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omnie_file = os.path.join(local_path, basename) |
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if not os.path.exists(omnie_file): |
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url = os.path.join(url_base, basename) |
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logging.info("%s not found, downloading from %s.", omnie_file, url) |
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_dl_file(omnie_file, url) |
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def omnie_mask_missing(df): |
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"""Mask missing values with NaN |
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Marks missing values in the OMNI2 data set by NaN. |
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The missing value indicating numbers are taken from the file format description |
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https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/extended/aareadme_extended |
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Parameters |
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---------- |
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df: pandas.DataFrame |
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The OMNI2 data set, e.g. from ``omnie_hourly()`` or ``read_omnie()``. |
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Returns |
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------- |
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df: pandas.DataFrame |
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The same dataframe with the missing values masked with numpy.nan. |
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Note |
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---- |
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This function returns a copy of the dataframe, and all the integer columns |
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will be converted to float to support NaN. |
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""" |
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res = df.copy() |
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for _c in df.columns: |
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_m = _OMNI_MISSING.get(_c, None) |
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if _m is None: |
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continue |
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_mask = df[_c] != _m |
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res[_c] = df[_c].where(_mask) |
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return res |
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def read_omnie(omnie_file): |
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"""Read and parse OMNI2 extended files [#]_ |
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Parses the Omni2 extended data files, available at [#]_, |
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into a :class:`pandas.DataFrame`. |
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.. [#] https://omniweb.gsfc.nasa.gov/ow.html |
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.. [#] https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/extended/ |
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Parameters |
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---------- |
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omnie_file: str |
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File to parse, absolute path or relative to the current dir. |
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Returns |
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------- |
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sw_df: pandas.DataFrame |
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The parsed OMNI2 space weather data (hourly values). |
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Details in |
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https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/extended/aareadme_extended |
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Raises an ``IOError`` if the file is not found. |
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The dataframe contains the following columns: |
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year: |
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The observation year |
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doy: |
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Day of the year |
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hour: |
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Hour of the day |
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bsrn: |
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Bartels Solar Rotation Number. |
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id_imf: |
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ID for IMF spacecraft |
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id_sw: |
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ID for SW plasma spacecraft |
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n_imf: |
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Number of points in IMF averages |
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n_plasma: |
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Numberof points in plasma averages |
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B_mag_avg: |
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Magnetic field magnitude average B |
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B_mag: |
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Magnetic field vector magnitude |
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theta_B: |
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Latitude angle of the magnetic field vector |
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phi_B: |
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Longitude angle of the magnetic field vector |
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B_x: |
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B_x GSE, GSM |
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B_y_GSE: |
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B_y GSE |
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B_z_GSE: |
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B_z GSE |
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B_y_GSM: |
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B_y GSM |
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B_z_GSM: |
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B_z GSM |
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sigma_B_mag_avg: |
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RMS standard deviation of B_mag_avg |
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sigma_B_mag: |
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RMS standard deviation of B_mag |
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sigma_B_x_GSE: |
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RMS standard deviation of B_x_GSE |
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sigma_B_y_GSE: |
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RMS standard deviation of B_y_GSE |
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sigma_B_z_GSE: |
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RMS standard deviation of B_z_GSE |
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T_p: |
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Proton temperature |
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n_p: |
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Proton density |
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v_plasma: |
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Plasma flow speed |
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phi_v: |
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Plasma flow longitude angle |
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theta_v: |
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Plasma flow latitude angle |
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n_alpha_n_p: |
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Alpha/Proton ratio |
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p_flow: |
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Flow pressure |
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sigma_T: |
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Standard deviation of T_p |
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sigma_n: |
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Standard deviation of n_p |
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sigma_v: |
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Standard deviation of v_plasma |
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sigma_phi_v: |
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Standard deviation of phi_v |
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sigma_theta_v: |
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Standard deviation of theta_v |
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sigma_na_np: |
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Standard deviation of n_alpha_n_p |
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E: |
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Electric field magnitude |
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beta_plasma: |
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Plasma beta |
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mach: |
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Alfvén Mach number |
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Kp: |
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Kp index value |
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R: |
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Sunspot number |
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Dst: |
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Dst index value |
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AE: |
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AE index value |
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p_01MeV, p_02MeV, p_04MeV, p_10MeV, p_30MeV, p_60MeV: |
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Proton fluxes >1 MeV, >2 MeV, >4 MeV, >10 MeV, >30 MeV, > 60 MeV |
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flag: |
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Flag (-1, ..., 6) |
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Ap: |
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Ap index value |
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f107_adj: |
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F10.7 radio flux at 1 AU |
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PC: |
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PC index value |
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AL, AU: |
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AL and AU index values |
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mach_mag: |
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Magnetosonic Mach number |
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The extended dataset contains the addional columns: |
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Lya: |
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Solar Lyman-alpha irradiance |
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QI_p: |
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Proton QI |
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""" |
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_assert_file_exists(omnie_file) |
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# FORMAT( |
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# 2I4,I3,I5,2I3,2I4,14F6.1,F9.0,F6.1,F6.0,2F6.1,F6.3,F6.2, |
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# F9.0,F6.1,F6.0,2F6.1,F6.3,2F7.2,F6.1,I3,I4,I6,I5,F10.2, |
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# 5F9.2,I3,I4,2F6.1,2I6,F5.1,F9.6,F7.4 |
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# ) |
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sw = np.genfromtxt( |
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omnie_file, |
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skip_header=0, |
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delimiter=[ |
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# 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 |
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322
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|
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# yy dd hr br i1 i2 n1 n2 B B' tB fB Bx By Bz By Bz sB sB sB |
|
323
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|
|
4, 4, 3, 5, 3, 3, 4, 4, 6, 6, 6, 6, 6, 6, 6, 6, 6, 6, 6, 6, |
|
324
|
|
|
# 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 |
|
325
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|
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# sB sB Tp np v fv tv nr p sT sn sv sf st sr E bp M Kp R |
|
326
|
|
|
6, 6, 9, 6, 6, 6, 6, 6, 6, 9, 6, 6, 6, 6, 6, 7, 7, 6, 3, 4, |
|
327
|
|
|
# 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 |
|
328
|
|
|
# Ds AE p1 p2 p4p10p30p60 fl Apf10 PC AL AU Mm La QI |
|
329
|
|
|
6, 5,10, 9, 9, 9, 9, 9, 3, 4, 6, 6, 6, 6, 5, 9, 7, |
|
330
|
|
|
], |
|
331
|
|
|
dtype=( |
|
332
|
|
|
"i4,i4,i4,i4,i4,i4,i4,i4,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8," |
|
333
|
|
|
"f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,f8,i4,i4," |
|
334
|
|
|
"i4,i4,f8,f8,f8,f8,f8,f8,i4,i4,f8,f8,i4,i4,f8,f8,f8" |
|
335
|
|
|
), |
|
336
|
|
|
names=[ |
|
337
|
|
|
"year", "doy", "hour", "bsrn", "id_imf", "id_sw", "n_imf", "n_plasma", |
|
338
|
|
|
"B_mag_avg", "B_mag", "theta_B", "phi_B", |
|
339
|
|
|
"B_x", "B_y_GSE", "B_z_GSE", "B_y_GSM", "B_z_GSM", |
|
340
|
|
|
"sigma_B_mag_avg", "sigma_B_mag", |
|
341
|
|
|
"sigma_B_x_GSE", "sigma_B_y_GSE", "sigma_B_z_GSE", |
|
342
|
|
|
"T_p", "n_p", "v_plasma", "phi_v", "theta_v", "n_alpha_n_p", "p_flow", |
|
343
|
|
|
"sigma_T", "sigma_n", "sigma_v", |
|
344
|
|
|
"sigma_phi_v", "sigma_theta_v", "sigma_na_np", |
|
345
|
|
|
"E", "beta_plasma", "mach", "Kp", "R", "Dst", "AE", |
|
346
|
|
|
"p_01MeV", "p_02MeV", "p_04MeV", "p_10MeV", "p_30MeV", "p_60MeV", |
|
347
|
|
|
"flag", "Ap", "f107_adj", "PC", "AL", "AU", "mach_mag", "Lya", "QI_p", |
|
348
|
|
|
] |
|
349
|
|
|
) |
|
350
|
|
|
sw = sw[sw["year"] != -1] |
|
351
|
|
|
ts = pd.to_datetime( |
|
352
|
|
|
[ |
|
353
|
|
|
"{0:04d}.{1:03d} {2:02d}".format(yy, dd, hh) |
|
354
|
|
|
for yy, dd, hh in sw[["year", "doy", "hour"]] |
|
355
|
|
|
], |
|
356
|
|
|
format="%Y.%j %H", |
|
357
|
|
|
) |
|
358
|
|
|
sw_df = pd.DataFrame(sw, index=ts) |
|
359
|
|
|
# Adjust Kp to 0...9 |
|
360
|
|
|
sw_df["Kp"] = 0.1 * sw_df["Kp"] |
|
361
|
|
|
return sw_df |
|
362
|
|
|
|
|
363
|
|
|
|
|
364
|
|
|
def omnie_hourly( |
|
365
|
|
|
year, |
|
366
|
|
|
prefix=None, |
|
367
|
|
|
ext=None, |
|
368
|
|
|
local_path=None, |
|
369
|
|
|
url_base=None, |
|
370
|
|
|
cache=False, |
|
371
|
|
|
): |
|
372
|
|
|
"""OMNI hourly data for year `year` |
|
373
|
|
|
|
|
374
|
|
|
Loads the OMNI hourly data for the given year, |
|
375
|
|
|
from the locally cached data. |
|
376
|
|
|
Use `local_path` to set a custom location if you |
|
377
|
|
|
have the omni data already available. |
|
378
|
|
|
|
|
379
|
|
|
Parameters |
|
380
|
|
|
---------- |
|
381
|
|
|
year: int |
|
382
|
|
|
Year of the data. |
|
383
|
|
|
prefix: str, optional, default 'omni2' |
|
384
|
|
|
File prefix for constructing the file name as <prefix>_year.<ext>. |
|
385
|
|
|
ext: str, optional, default 'dat' |
|
386
|
|
|
File extension for constructing the file name as <prefix>_year.<ext>. |
|
387
|
|
|
local_path: str, optional |
|
388
|
|
|
Path to the locally stored data yearly files, defaults to the |
|
389
|
|
|
data location within the package. |
|
390
|
|
|
url_base: str, optional |
|
391
|
|
|
URL for the directory that contains the yearly files. |
|
392
|
|
|
cache: boolean, optional, default False |
|
393
|
|
|
Download files locally if they are not already available. |
|
394
|
|
|
|
|
395
|
|
|
Returns |
|
396
|
|
|
------- |
|
397
|
|
|
sw_df: pandas.DataFrame |
|
398
|
|
|
The parsed space weather data (hourly values). |
|
399
|
|
|
|
|
400
|
|
|
Raises an ``IOError`` if the file is not available. |
|
401
|
|
|
|
|
402
|
|
|
See Also |
|
403
|
|
|
-------- |
|
404
|
|
|
read_omnie |
|
405
|
|
|
""" |
|
406
|
|
|
prefix = prefix or OMNI_PREFIX |
|
407
|
|
|
ext = ext or OMNI_EXT |
|
408
|
|
|
local_path = local_path or LOCAL_PATH |
|
409
|
|
|
url_base = url_base or OMNI_URL_BASE |
|
410
|
|
|
|
|
411
|
|
|
basename = "{0}_{1:04d}.{2}".format(prefix, year, ext) |
|
412
|
|
|
omnie_file = os.path.join(local_path, basename) |
|
413
|
|
|
|
|
414
|
|
|
# ensure that the file exists |
|
415
|
|
|
if not os.path.exists(omnie_file): |
|
416
|
|
|
warn("Could not find OMNI2 data {0}.".format(omnie_file)) |
|
417
|
|
|
if cache: |
|
418
|
|
|
cache_omnie( |
|
419
|
|
|
year, |
|
420
|
|
|
prefix=prefix, ext=ext, |
|
421
|
|
|
local_path=local_path, url_base=url_base, |
|
422
|
|
|
) |
|
423
|
|
|
else: |
|
424
|
|
|
warn( |
|
425
|
|
|
"Local data files not found, pass `cache=True` " |
|
426
|
|
|
"or run `sw.cache_omnie()` to download the file." |
|
427
|
|
|
) |
|
428
|
|
|
|
|
429
|
|
|
return read_omnie(omnie_file) |
|
430
|
|
|
|