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Data loader (and downloader) for Solar Orbiter/EPD energetic charged particle sensors EPT, HET, and STEP. Supports level 2 and low latency data provided by ESA's Solar Orbiter Archive.

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ARCHIVED

⚠️ This repository is archived, please visit https://github.com/jgieseler/solo-epd-loader for the current version of this package! ⚠️

solo-loader

Data loader for SolO/EPD EPT, HET, and STEP level 2 (l2) and low latency (ll) data provided by CDF files from http://soar.esac.esa.int/soar.

Requirements

Installation

Install all the requirements, download epd_loader.py, and place it in your working directory. Then access it as described in the Usage section.

Usage

The standard usecase is to utilize the epd_load function, which returns Pandas dataframe(s) of the EPD measurements and a dictionary containing information on the energy channels.

from epd_loader import *

df_1, df_2, energies = \
    epd_load(sensor, viewing, level, startdate, enddate, path, autodownload)

Input

  • sensor: ept, het, or step (string)
  • viewing: sun, asun, north, or south (string); not needed for sensor = step
  • level: ll or l2 (string)
  • startdate, enddate: YYYYMMDD, e.g., 20210415 (integer) (if no enddate is provided, enddate = startdate will be used)
  • path: directory in which Solar Orbiter data is/should be organized; e.g. /home/gieseler/uni/solo/data/ (string)
  • autodownload: if True will try to download missing data files from SOAR (bolean)

Return

  • For sensor = ept or het:

    1. Pandas dataframe with proton fluxes and errors (for EPT also alpha particles) in 'particles / (s cm^2 sr MeV)'
    2. Pandas dataframe with electron fluxes and errors in 'particles / (s cm^2 sr MeV)'
    3. Dictionary with energy information for all particles:
      • String with energy channel info
      • Value of lower energy bin edge in MeV
      • Value of energy bin width in MeV
  • For sensor = step:

    1. Pandas dataframe with fluxes and errors in 'particles / (s cm^2 sr MeV)'
    2. Dictionary with energy information for all particles:
      • String with energy channel info
      • Value of lower energy bin edge in MeV
      • Value of energy bin width in MeV

Data folder structure

The path variable provided to the module should be the base directory where the corresponding cdf data files should be placed in subdirectories. First subfolder defines the data product level (l2 or low_latency at the moment), the next one the instrument (so far only epd), and finally the sensor (ept or het for now).

For example, the folder structure could look like this: /home/userxyz/solo/data/l2/epd/het. In this case, you should call the loader with path=/home/userxyz/solo/data; i.e., the base directory for the data.

Hint: You can use the (automatic) download function described in one of the following sections to let the subfolders be created initially automatically. (NB: It might be that you need to run the code with sudo/admin privileges in order to be able to create new folders on your system.)

Data download within Python

Data files can be downloaded from http://soar.esac.esa.int/soar directly from within python. They are saved in the folder provided by the path argument.

Automatic download

While using epd_load() to obtain the data, one can choose to automatically download missing data files. For that, just add autodownload=True to the function call:

from epd_loader import *

df_protons, df_electrons, energies = \
    epd_load(sensor='het', viewing='sun', level='l2', 
             startdate=20200820, enddate=20200821, \
             path='/home/userxyz/solo/data/', autodownload=True)

# plot protons and alphas
ax = df_protons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

# plot electrons
ax = df_electrons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

Note: The code will always download the latest version of the file available at SOAR. So in case a file V01.cdf is already locally present, V02.cdf will be downloaded nonetheless.

Manual download

Level 2 data can be manually downloaded using epd_l2_download(). But because this is usually only done internally, the path variable is defined a bit different here; it needs to be the full path to where the cdf files should be stored (instead of the base directory). Following example downloads EPT NORTH telescope data for Aug 20 2020 to the dir /home/userxyz/solo/data/. Right now rudimentary working with one download (1 file/day) per call.

from epd_loader import *

epd_l2_download(20200820, '/home/userxyz/solo/data/l2/epd/ept/', 'ept', 'north')

epd_ll_download() provides the same functionality for low latency data:

from epd_loader import *

epd_ll_download(20200820, '/home/userxyz/solo/data/low_latency/epd/ept/', 'ept', 'north')

Example 1 - low latency data

Example code that loads low latency (ll) electron and proton (+alphas) fluxes (and errors) for EPT NORTH telescope from Apr 15 2021 to Apr 16 2021 into two Pandas dataframes (one for protons & alphas, one for electrons). In general available are 'sun', 'asun', 'north', and 'south' viewing directions for 'ept' and 'het' telescopes of SolO/EPD.

from epd_loader import *

df_protons, df_electrons, energies = \
    epd_load(sensor='ept', viewing='north', level='ll', 
             startdate=20210415, enddate=20210416, \
             path='/home/userxyz/solo/data/')

# plot protons and alphas
ax = df_protons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

# plot electrons
ax = df_electrons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

Example 2 - level 2 data

Example code that loads level 2 (l2) electron and proton (+alphas) fluxes (and errors) for HET SUN telescope from Aug 20 2020 to Aug 20 2020 into two Pandas dataframes (one for protons & alphas, one for electrons).

from epd_loader import *

df_protons, df_electrons, energies = \
    epd_load(sensor='het', viewing='sun', level='l2', 
             startdate=20200820, enddate=20200821, \
             path='/home/userxyz/solo/data/')

# plot protons and alphas
ax = df_protons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

# plot electrons
ax = df_electrons.plot(logy=True, subplots=True, figsize=(20,60))
plt.show()

Example 3 - reproducing EPT data from Fig. 2 in Gómez-Herrero et al. 20211

from epd_loader import *

# set your local path here
lpath = '/home/userxyz/solo/data'

# load data
df_protons, df_electrons, energies = \
    epd_load(sensor='ept', viewing='sun', level='l2', startdate=20200708, 
             enddate=20200724, path=lpath, autodownload=True)

# change time resolution to get smoother curve (resample with mean)
resample = '60min'

fig, axs = plt.subplots(2, sharex=True)
fig.suptitle('EPT Sun')

# plot selection of channels
for channel in [0, 8, 16, 26]:
    df_electrons['Electron_Flux'][f'Electron_Flux_{channel}']\
        .resample(resample).mean().plot(ax = axs[0], logy=True,
        label=energies["Electron_Bins_Text"][channel][0])
for channel in [6, 22, 32, 48]:
    df_protons['Ion_Flux'][f'Ion_Flux_{channel}']\
        .resample(resample).mean().plot(ax = axs[1], logy=True,
        label=energies["Ion_Bins_Text"][channel][0])

axs[0].set_ylim([0.3, 4e6])
axs[1].set_ylim([0.01, 5e8])

axs[0].set_ylabel("Electron flux\n"+r"(cm$^2$ sr s MeV)$^{-1}$")
axs[1].set_ylabel("Ion flux\n"+r"(cm$^2$ sr s MeV)$^{-1}$")
axs[0].legend()
axs[1].legend()
plt.subplots_adjust(hspace=0)
plt.show()

NB: This is just an approximate reproduction with different energy channels (smaller, not combined) and different time resolution! Figure

Example 4 - reproducing EPT data from Fig. 2 in Wimmer-Schweingruber et al. 20212

from epd_loader import *

# set your local path here
lpath = '/home/userxyz/solo/data'

# load data
df_protons_sun, df_electrons_sun, energies = \
    epd_load(sensor='ept', viewing='sun', level='l2', 
             startdate=20201210, enddate=20201211,
             path=lpath, autodownload=True)
df_protons_asun, df_electrons_asun, energies = \
    epd_load(sensor='ept', viewing='asun', level='l2', 
             startdate=20201210, enddate=20201211,
             path=lpath, autodownload=True)
df_protons_south, df_electrons_south, energies = \
    epd_load(sensor='ept', viewing='south', level='l2', 
             startdate=20201210, enddate=20201211,
             path=lpath, autodownload=True)
df_protons_north, df_electrons_north, energies = \
    epd_load(sensor='ept', viewing='north', level='l2', 
             startdate=20201210, enddate=20201211,
             path=lpath, autodownload=True)

# plot mean intensities of two energy channels; 'channel' defines the lower one
channel = 6
ax = pd.concat([df_electrons_sun['Electron_Flux'][f'Electron_Flux_{channel}'],
                df_electrons_sun['Electron_Flux'][f'Electron_Flux_{channel+1}']],
                axis=1).mean(axis=1).plot(logy=True, label='sun', color='#d62728')
ax = pd.concat([df_electrons_asun['Electron_Flux'][f'Electron_Flux_{channel}'],
                df_electrons_asun['Electron_Flux'][f'Electron_Flux_{channel+1}']],
                axis=1).mean(axis=1).plot(logy=True, label='asun', color='#ff7f0e')
ax = pd.concat([df_electrons_north['Electron_Flux'][f'Electron_Flux_{channel}'],
                df_electrons_north['Electron_Flux'][f'Electron_Flux_{channel+1}']],
                axis=1).mean(axis=1).plot(logy=True, label='north', color='#1f77b4')
ax = pd.concat([df_electrons_south['Electron_Flux'][f'Electron_Flux_{channel}'],
                df_electrons_south['Electron_Flux'][f'Electron_Flux_{channel+1}']],
                axis=1).mean(axis=1).plot(logy=True, label='south', color='#2ca02c')

plt.xlim([datetime.datetime(2020, 12, 10, 23, 0), 
          datetime.datetime(2020, 12, 11, 12, 0)])

ax.set_ylabel("Electron flux\n"+r"(cm$^2$ sr s MeV)$^{-1}$")
plt.title('EPT electrons ('+str(energies['Electron_Bins_Low_Energy'][channel])
          + '-' + str(energies['Electron_Bins_Low_Energy'][channel+2])+' MeV)')
plt.legend()
plt.show()

NB: This is just an approximate reproduction; e.g., the channel combination is a over-simplified approximation! Figure

References

1: Gómez-Herrero et al. 2021, First near-relativistic solar electron events observed by EPD onboard Solar Orbiter, A&A, https://doi.org/10.1051/0004-6361/202039883.

2: Wimmer-Schweingruber et al. 2021, The first year of energetic particle measurements in the inner heliosphere with Solar Orbiter’s Energetic Particle Detector, submitted to A&A.

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Data loader (and downloader) for Solar Orbiter/EPD energetic charged particle sensors EPT, HET, and STEP. Supports level 2 and low latency data provided by ESA's Solar Orbiter Archive.

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