SciQLop (SCIentific Qt application for Learning from Observations of Plasmas) is a powerful and user-friendly tool designed for the visualization and analysis of in-situ space plasma data.
Using SciQLop will let you:
- have a super easy access to tens of thousands of products from the top main data archives in the world,
- explore multivariate time series effortlessly, with lightning-fast and transparent downloads as you scroll, zoom in, and zoom out,
- visualize custom products with simple python code executed on-the-fly,
- easily label time intervals and make or edit catalog of events graphically and rapidely,
- analyze your data in jupyter notebooks,
Heliophysicists now benefit from decades of space exploration through many spacecraft missions. Exploring this massive amount of data to find events of interest, build catalogs, and conduct statistical multi-mission data analysis can be a daunting task if not having the right tool.
SciQLop aims at being this tool! A simple lightweight yet powerful graphical interface coupled to the limitless options brought by the Jupyter Notebook integration, that focuses on providing users with the easiest possible way to explore, label and analyze huge amounts of data. SciQLop is also the right tool for teaching space physics and in situ spacecraft data handling to students effortlessly.
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Interactive and responsive: SciQLop can handle millions of data points without compromising on interactivity. Users can scroll, zoom, move, and export plots with ease.
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User-friendly: Accessing data in SciQLop is as simple as a drag and drop from the tens of thousands of products readily available. Custom user products defined in Python behave exactly the same way and bring infinite possibilities.
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Jupyter notebook integration: SciQLop can be used as a backend for Jupyter notebooks, allowing users to create and manipulate plots from within their notebooks, define new products and much more.
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Catalogs: SciQLop provides a catalog system that allows users to easily label events in their data or visualize existing catalogs of events.
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Evolving and growing list of examples: SciQLop comes with a growing list of examples that demonstrate how to perform common tasks such as loading data, creating plots, and using the catalog system.
- community-driven plugins repository: SciQLop will soon have a plugin system that will allow users to extend the software's capabilities by installing community-driven plugins.
- catalogs coediting: SciQLop will allow users to coedit catalogs, making it easier to collaborate on event labeling and visualization, thereby also improving reproducibility of space physics studies.
Since SciQLop 0.7.1 we produce a Mac App Bundle that you can download from the latest release page just pick the right architecture for your Mac (ARM64 for Apple M1/2/3 chips and x86_64 for intel ones).
If you are using a Linux distribution, you may not need to install anything, you can just download the AppImage from the latest release and run it (after making it executable).
Warning: Due to this issue you should not use any * Python* version higher than 3.10.x.
Since SciQLop depends on specific versions of PySide6 you should use a dedicated virtualenv for SciQLop to avoid any conflict with any other Python package already installed in your system.
- Using releases from PyPi
python -m pip install sciqlop- Using the latest code from GitHub
python -m pip install git+https://github.com/SciQLop/SciQLopOnce installed the sciqlop launcher should be in your PATH and you should be able to start SciQLop from your terminal.
sciqlopor
python -m SciQLop.appThe following API examples are for early adopters and will likely change a bit in the future!
- Creating plot panels:
from SciQLop.backend import TimeRange
from datetime import datetime
# all plots are stacked
p = main_window.new_plot_panel()
p.time_range = TimeRange(datetime(2015, 10, 22, 6, 4, 30).timestamp(), datetime(2015, 10, 22, 6, 6, 0).timestamp())
p.plot("speasy/cda/MMS/MMS1/FGM/MMS1_FGM_BRST_L2/mms1_fgm_b_gsm_brst_l2")
p.plot("speasy/cda/MMS/MMS1/DIS/MMS1_FPI_BRST_L2_DIS_MOMS/mms1_dis_bulkv_gse_brst")
p.plot("speasy/cda/MMS/MMS1/DIS/MMS1_FPI_BRST_L2_DIS_MOMS/mms1_dis_energyspectr_omni_brst")
# tha_peif_sc_pot and tha_peif_en_eflux will share the same plot
p2 = main_window.new_plot_panel()
p2.plot("speasy/cda/THEMIS/THA/L2/THA_L2_ESA/tha_peif_en_eflux")
p2.plots[0].plot("speasy/cda/THEMIS/THA/L2/THA_L2_ESA/tha_peif_sc_pot")
p2.plot("speasy/cda/THEMIS/THA/L2/THA_L2_ESA/tha_peif_velocity_dsl")NOTE: An easy way to get product paths, is to drag a product from Products Tree to any text zone or even your Python terminal.
- Custom products:
from datetime import datetime
import numpy as np
from SciQLop.backend.pipelines_model.easy_provider import EasyVector, EasyScalar
# The following functions can do anything from loading data from a file to any complex computation, they should not
# block the GUI since they will be run in background.
def my_vect(start: datetime, stop: datetime) -> (np.ndarray, np.ndarray):
x = np.arange(start.timestamp(), stop.timestamp(), 0.1) * 1.
y = np.empty((len(x), 3))
y[:, 0] = np.cos(x / 100.) * 10.
y[:, 1] = np.cos((x + 100) / 100.) * 10.
y[:, 2] = np.cos((x + 200) / 100.) * 10.
return x, y
def my_scalar(start: datetime, stop: datetime) -> (np.ndarray, np.ndarray):
x = np.arange(start.timestamp(), stop.timestamp(), 0.1) * 1.
y = np.empty((len(x), 1))
y[:, 0] = np.cos(x / 100.) * 10.
return x, y
my_vector_provider = EasyVector(path='some_root_folder/my_hello_world_vector', get_data_callback=my_vect,
components_names=["x", "y", "z"], metadata={})
my_scalar_provider = EasyScalar(path='some_other_root_folder/my_hello_world_scalar', get_data_callback=my_scalar,
component_name="x", metadata={})More examples can be found in the examples folder, they are also available from the welcome screen.
Just fork the repository, make your changes and submit a pull request. We will be happy to review and merge your changes. Reports of bugs and feature requests are also welcome.
The development of SciQLop is supported by the CDPP.
We acknowledge support from the federation Plas@Par
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