2022
Stevenson, Emma; Rodriguez-Fernandez, Victor; Minisci, Edmondo; Camacho, David
A deep learning approach to solar radio flux forecasting Journal Article
In: Acta Astronautica, vol. 193, pp. 595-606, 2022, ISSN: 0094-5765.
Abstract | Links | BibTeX | Tags: Deep Learning, Ensemble, Solar Radio Flux, Space, Time Series
@article{STEVENSON2022595,
title = {A deep learning approach to solar radio flux forecasting},
author = {Emma Stevenson and Victor Rodriguez-Fernandez and Edmondo Minisci and David Camacho},
url = {https://www.sciencedirect.com/science/article/pii/S009457652100415X},
doi = {https://doi.org/10.1016/j.actaastro.2021.08.004},
issn = {0094-5765},
year = {2022},
date = {2022-01-01},
journal = {Acta Astronautica},
volume = {193},
pages = {595-606},
abstract = {The effect of atmospheric drag on spacecraft dynamics is considered one of the predominant sources of uncertainty in Low Earth Orbit. These effects are characterised in part by the atmospheric density, a quantity highly correlated to space weather. Current atmosphere models typically account for this through proxy indices such as the F10.7, but with variations in solar radio flux forecasts leading to significant orbit differences over just a few days, prediction of these quantities is a limiting factor in the accurate estimation of future drag conditions, and consequently orbital prediction. In this work, a novel deep residual architecture for univariate time series forecasting, N-BEATS, is employed for the prediction of the F10.7 solar proxy on the days-ahead timescales relevant to space operations. This untailored, pure deep learning approach has recently achieved state-of-the-art performance in time series forecasting competitions, outperforming well-established statistical, as well as statistical hybrid models, across a range of domains. The approach was found to be effective in single point forecasting up to 27-days ahead, and was additionally extended to produce forecast uncertainty estimates using deep ensembles. These forecasts were then compared to a persistence baseline and two operationally available forecasts: one statistical (provided by BGS, ESA), and one multi-flux neural network (by CLS, CNES). It was found that the N-BEATS model systematically outperformed the baseline and statistical approaches, and achieved an improved or similar performance to the multi-flux neural network approach despite only learning from a single variable.},
keywords = {Deep Learning, Ensemble, Solar Radio Flux, Space, Time Series},
pubstate = {published},
tppubtype = {article}
}
The effect of atmospheric drag on spacecraft dynamics is considered one of the predominant sources of uncertainty in Low Earth Orbit. These effects are characterised in part by the atmospheric density, a quantity highly correlated to space weather. Current atmosphere models typically account for this through proxy indices such as the F10.7, but with variations in solar radio flux forecasts leading to significant orbit differences over just a few days, prediction of these quantities is a limiting factor in the accurate estimation of future drag conditions, and consequently orbital prediction. In this work, a novel deep residual architecture for univariate time series forecasting, N-BEATS, is employed for the prediction of the F10.7 solar proxy on the days-ahead timescales relevant to space operations. This untailored, pure deep learning approach has recently achieved state-of-the-art performance in time series forecasting competitions, outperforming well-established statistical, as well as statistical hybrid models, across a range of domains. The approach was found to be effective in single point forecasting up to 27-days ahead, and was additionally extended to produce forecast uncertainty estimates using deep ensembles. These forecasts were then compared to a persistence baseline and two operationally available forecasts: one statistical (provided by BGS, ESA), and one multi-flux neural network (by CLS, CNES). It was found that the N-BEATS model systematically outperformed the baseline and statistical approaches, and achieved an improved or similar performance to the multi-flux neural network approach despite only learning from a single variable.
2019
Hernández, Alfonso; Panizo-LLedot, Ángel; Camacho, David
An ensemble algorithm based on deep learning for tuberculosis classification Inproceedings
In: International conference on intelligent data engineering and automated learning, pp. 145–154, Springer 2019.
Links | BibTeX | Tags: Convolutional Neural Networks, Deep Learning, Ensemble, Health, Image Classification
@inproceedings{hernandez2019ensemble,
title = {An ensemble algorithm based on deep learning for tuberculosis classification},
author = {Alfonso Hernández and Ángel Panizo-LLedot and David Camacho},
doi = {10.1007/978-3-030-33607-3_17},
year = {2019},
date = {2019-01-01},
urldate = {2019-01-01},
booktitle = {International conference on intelligent data engineering and automated learning},
pages = {145--154},
organization = {Springer},
keywords = {Convolutional Neural Networks, Deep Learning, Ensemble, Health, Image Classification},
pubstate = {published},
tppubtype = {inproceedings}
}