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Data Driven Thermospheric Density Modeling with Machine Learning

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Karman: Data Driven Thermospheric Density Modeling
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Karman is a machine learning (ML) Python package for thermospheric density modelling. It was developed as a collaboration between the Heliophysics Division of NASA and Trillium Technologies under a NASA-funded Sole Source project. Its main goal is to improve our understanding and modeling of thermospheric density variations due to the Sun's influence. Furthermore, it also has the objective to provide a shared framework where people can design, train and benchmark their own thermospheric density models.

Goals

  • Release of ML models to predict thermospheric density changes from solar and geomagnetic data, trained on precise orbit determination (POD)-derived thremospheric density measurements.
  • A framework to support ingestion of solar irradiance, geomagnetic and thermospheric density data from different sources.
  • Benchmarking framework to enable comparison between ML and empirical models at different geomagnetic storm conditions, altitude, times, etc.

Supported Data

Currently, the Karman software supports several input data from different sources:

  • High frequency (i.e., every 30 or 10 seconds) POD-derived thermospheric density data from five space missions (CHAMP, GOCE, GRACE, SWARM-A, SWARM-B), from TU Delft thermosphere data.
  • NRLMSISE-00 and JB-08 thermospheric density empirical models inputs (and corresponding predicted density).
  • Geomagnetic input data from NASA's OMNIWeb high resolution data.
  • EUV Stan Bands from FISM2 empirical model (both daily and flare).
  • Solar irradiance proxies commonly used in empirical thermospheric density models (i.e., F10.7, S10.7, M10.7, Y10.7).

Karman Schematic Illustration

Installation, documentation, and examples

https://karman-project.readthedocs.io/en/latest/

Authors:

The project originated after the initial work of the NASA-FDL 2021 Solar Drag team, funded by the Heliophysics Division of NASA.

Solar Drag team members: Researchers: Stefano Bonasera, Edward Brown, Jorge A. Pérez-Hernández, Bernard Benson; Faculty: Giacomo Acciarini, Atılım Güneş Baydin, Chris Bridges; Advisors: Eric Sutton, Moriba K. Jah.

More info and how to cite:

If you would like to learn more about or cite the techniques Karman uses, please see the following papers:

@article{acciarini2024improving,
  title={Improving Thermospheric Density Predictions in Low-Earth Orbit With Machine Learning},
  author={Acciarini, Giacomo and Brown, Edward and Berger, Tom and Guhathakurta, Madhulika and Parr, James and Bridges, Christopher and Baydin, At{\i}l{\i}m G{\"u}ne{\c{s}}},
  journal={Space Weather},
  volume={22},
  number={2},
  pages={e2023SW003652},
  year={2024},
  publisher={Wiley Online Library}
}
@inproceedings{karman-amos-acciarini,
  author    = {Giacomo Acciarini and Edward Brown and Christopher Bridges and Atılım Güneş Baydin and Thomas E. Berger and Madhulika Guhathakurta},
  title     = {Karman - a Machine Learning Software Package for Benchmarking Thermospheric Density Models},
  booktitle = {Proceedings of the Advanced Maui Optical and Space Surveillance Technologies Conference (AMOS)},
  year      = {2023},
  month     = {September},
  day       = {19},
}

Acknowledgements:

The authors would like to ackowledge the support and precious feedback of several people: Dr. Madhulika Guhathakurta, Tom Berger, and all the NASA-FDL 2021 reviewers.

Contact:

  • giacomo.acciarini@gmail.com