The e-Callisto Validation project aims to evaluate the performance of the actual e-Callisto product. The project consists of two independent validation campaigns. The first campaign is focused on assessing the data quality, while the second is focused on each station's availability and cross-comparison level. The e-Callisto network, which consists of multiple CALLISTO spectrometers deployed worldwide, can continuously observe the solar radio spectrum 24/7. The e-Callisto provides radio spectrograms, which are time series of radio flux measurements at a relatively high number of radio frequencies, and the purpose of the validation campaign is to determine the intended cross-comparison within the e-Callisto network and test cases. The project aims to validate the e-Callisto product's ability to observe different types of solar radio bursts, such as type II, type III, or type IV, and to classify bursts and perform long-term trend analyses. The two main use cases for the validation of the product are the determination of the speed of accelerated electron beams, as they appear in Type III bursts, and the provision of spectrograms as complementary information for analysis of events observed by instruments on spacecraft that look at the same events, but in different wavelengths.
- The entire Data: Here
This is a quick overview of the folder structure:
- Calibrarion_with_Orfees:
- eca_files
- orfees_files
- Orfees_read.py
- calibration.ipynb
- cross_correlation.ipynb
- docs
- radiospectra2:
- validation:
- Bursts:
- sync.py
- up_to_date.py
- upload_to_ecallisto.py
- rating_system:
- config.py
- daily_observation.py
- rating.py
- rating_pro_file.ipynb
- test_data.ipynb
- testing.ipynb
- source:
- validation.py
- update.py
- save_to_sql.py
- hist_test.py
- test_validation.ipynb
- Bursts:
- README.ipynb
- requirements.txt
Here is a brief description for each file:
- eca_files: Contains the eCallisto files for tests
- orfees_files: Contains the Orfees files for tests
- Orfees_read.py
- calibration.ipynb
- cross_correlation.ipynb
Contains the documentation of the project. eCallistoValidation Dokumentation
- radiospectra2: submodule of i4ds radiospectra project (https://github.com/i4Ds/radiospectra).
-
rating_stars: Contains the scripts for the Rating system.
-
source: Contains all files we need for validation.
-
requirements.txt: Contains all the modules we need to install.
This class reads data from Orfees spectrograms and allows the user to manipulate the data in various ways.
To read data from an Orfees spectrogram, use the read_orfees() method. The method takes a filename as a parameter and returns a dictionary containing the spectrogram data, as well as various other metadata. For example:
from Calibrarion_with_Orfees.Orfees_read import *
orfees = OrfeesSpectrogram('path to orfees files')To resize the spectrogram, use the resize() method. The method takes a target shape (in the form of a tuple) as a parameter and returns the resized spectrogram. For example:
orfees = OrfeesSpectrogram('path to orfees files')
spec=CallistoSpectrogram.from_url('http://soleil.i4ds.ch/solarradio/data/200220yy_Callisto/2017/09/06/GREENLAND_20170906_115514_62.fit.gz')
resized_spec = orfees_2.resize((spec.shape[1],spec.shape[0]))
plt.imshow(data,vmin=100, vmax=1000, aspect="auto")
plt.show()To select a time range from the spectrogram, use the time_range() method. The method takes a start time and an end time (in the format HH:MM:SS) as parameters and returns the subset of the spectrogram that falls within the specified time range. For example:
orfees = OrfeesSpectrogram('path to orfees files')
subset_spec = orfees.time_range(start_time, end_time)To plot the spectrogram, use the peek() method. The method takes a start time and an end time (in the format HH:MM:SS) as optional parameters and plots the spectrogram for the specified time range. If no time range is specified, the entire spectrogram is plotted. For example:
orfees = OrfeesSpectrogram('path to orfees files')
spec = CallistoSpectrogram.from_url('http://soleil.i4ds.ch/solarradio/data/2002-20yy_Callisto/2015/11/04/BIR_20151104_120000_03.fit.gz')
# plot without parameters:
orfees.peek()
# plot with the frequency range of ecallisto frequency:
orfees.plot_range_freq(spec)The Rating System provides a way to rate stations based on the signal-to-noise ratio (SNR) and standard deviation (std) of their data. The class uses a quantile normalization method to sort the data into different bins, with each bin representing a certain rating between 1 and 5 stars. The class takes in a start and end time and returns a pandas DataFrame containing the station name, SNR, SNR rating, std, std rating, and
How to use it? To use the Rating system, you first need to import it into your Python script:
install the requirements for rating System:
pip3 install -r rating_requirements.txtExample:
from eCallistoValidation/validation/rating_system/rating import Rating
# create an instance of the Rating class and call its rate_stations method, passing in a start and end time as arguments. For example:
# 1) Run the rating.py script.
# 2) Enter the start time and end time as following:
start_time = input( "Enter start time (YYYY-MM-DD HH:MM:SS): " )
end_time = input( "Enter end time (YYYY-MM-DD HH:MM:SS): " )
rating = Rating( start_time, end_time )
df = rating.rate_stations()
print(df)This function generates a PDF report containing 4 spectrogram plots for each input row. Each row is expected to contain the path of a spectrogram file and some metadata, which is used to calculate and display the standard deviation, signal-to-noise ratio, and maximum mean values of the spectrogram.
To use this function, provide a list of rows where each row is a list containing the spectrogram file path and the corresponding metadata. The PDF report will be saved in the same directory as the script with the name 'bg_sub_images.pdf'.
def get_plot(rows):
with PdfPages('bg_sub_images.pdf') as pdf:
for row in rows:
try:
file_path = row[1]
file_name = row[1].split("/")[4]
spec = CallistoSpectrogram.read(test_config.DATA_PATH + file_path)
fig1, axs1 = plt.subplots(1, 4, figsize=(27, 6))
ax1 = spec.plot()
ax1.title.set_text("Original Data")
plt.close()
# Second column, Constbacksub + elimwrongchannels
spec2 = spec.subtract_bg("constbacksub", "elimwrongchannels")
fig2 = plt.subplots(1, 4, figsize=(27, 6))
ax2 = spec2.plot()
ax2.title.set_text("Background subtracted")
plt.close()
# Third column, subtract_bg_sliding_window
spec3 = spec.subtract_bg("subtract_bg_sliding_window", window_width=800, affected_width=1,
amount=0.05, change_points=True)
fig3 = plt.figure(figsize=(27, 6))
ax3 = spec3.plot()
ax3.title.set_text(
"Gliding background subtracted (window=800)")
plt.close()
# Fourth column, Histograms
fig4, ax4 = plt.subplots(figsize=(27, 6))
# Fourth column, Histograms
data_absolute3 = get_abs_data(spec2)
data_absolute4 = get_abs_data(spec3)
n, bins, patches = ax4.hist([data_absolute3, data_absolute4], histtype='step', bins=25, log = True,
label=['Background subtracted', 'Gliding background subtracted'])
# Calculate the standard deviation and signal-to-noise => rounded them to have 3 digits.
std_data = round(row[6], 3)
snr_data = round(row[7], 3)
max_mean = round(row[8], 3)
# Set title for the histograms and show the std/snr values.
ax4.title.set_text(
f"Histograms, std = {std_data}, snr = {snr_data}, max_mean = {max_mean}")
plt.legend()
plt.close()
# Plot final plot by moving axes to the figure
fig_target, (axA, axB, axC, axD) = plt.subplots(
1, 4, figsize=(30, 9))
plt.suptitle(fig1._suptitle.get_text())
move_axes(fig_target, ax1, axA)
move_axes(fig_target, ax2, axB)
move_axes(fig_target, ax3, axC)
move_axes(fig_target, ax4, axD)
for ax in (ax1, ax2, ax3):
ax.set_xlabel('Time[UT]')
ax.set_ylabel('Frequency[MHz]')
ax4.set_xlabel('Pixel values')
ax4.set_ylabel('Number of pixels')
pdf.savefig(fig_target)
plt.close()
except Exception as err:
print(f"The Error message is: {err} and the file name is {file_name}")