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Updated: Sep 24, 2025

Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface
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Uncertainty quantification techniques for data-driven space weather modeling: thermospheric density application.

Richard J Licata1, Piyush M Mehta2

  • 1Department of Mechanical and Aerospace Engineering, West Virginia University, Morgantown, WV, 26506, USA. rjlicata@mix.wvu.edu.

Scientific Reports
|May 4, 2022
PubMed
Summary
This summary is machine-generated.

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Machine learning models now predict thermospheric density with reliable uncertainty estimates. This improves space weather forecasting and satellite collision risk assessment for low Earth orbit operations.

Area of Science:

  • Space Physics and Aeronomy
  • Machine Learning Applications
  • Atmospheric Science

Background:

  • Space weather, driven by solar activity, significantly impacts Earth's upper atmosphere (thermosphere).
  • Accurate forecasting of thermospheric neutral mass density is crucial for satellite drag prediction and collision avoidance in low Earth orbit (LEO).
  • Current models often lack reliable uncertainty estimates, hindering operational decision-making.

Purpose of the Study:

  • To develop nonlinear machine learning (ML) regression models for predicting thermospheric density.
  • To provide robust and reliable uncertainty estimates alongside density predictions.
  • To evaluate the performance of ML models using both local and global datasets.

Main Methods:

  • Implemented two ML techniques: Monte Carlo (MC) dropout and direct probability distribution prediction.

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Last Updated: Sep 24, 2025

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  • Utilized the negative logarithm of predictive density (NLPD) loss function for model training.
  • Trained and tested models on both local (CHAllenging Minisatellite Payload - CHAMP) and global (High Accuracy Satellite Drag Model - HASDM) density datasets.
  • Main Results:

    • Both ML techniques, using NLPD loss, yielded accurate thermospheric density predictions with well-calibrated uncertainty estimates.
    • The direct probability distribution prediction method demonstrated a significantly lower computational cost.
    • Global models achieved ~11% error on independent test data, while CHAMP models showed ~13% error, with excellent calibration across prediction intervals.

    Conclusions:

    • Proposed ML models offer a promising approach for accurate thermospheric density forecasting with crucial uncertainty quantification.
    • These advancements can enhance space situational awareness and improve the safety of space operations in LEO.
    • The developed models provide a valuable tool for global density predictions and their associated uncertainties.