TY - JOUR
T1 - Prediction Interval of Interface Regions
T2 - Machine Learning Nowcasting Approach
AU - Alielden, Khaled
AU - Camporeale, Enrico
AU - Korsós, Marianna B.
AU - Taroyan, Youra
N1 - Publisher Copyright:
© 2023. The Authors.
PY - 2023/3/16
Y1 - 2023/3/16
N2 - Stream interaction region (SIR) is one of the space weather phenomena that accelerates the upstream particles of the interface region in interplanetary space and causes geomagnetic storms. SIRs are large-scale structures that vary temporally and spatially, both in latitudinal and radial directions. Predicting the arrival times of interface regions (IRs) is crucial to protect our navigation and communication systems. In this work, a 1D ensemble system comprised of a Long-short-term memory (LSTM) model and a Convolution Neural Network (CNN) model—LCNN is introduced to classify the observed IR time series and give the prediction interval nowcast of its transit time to the observer. The outcomes of the two models are combined in a way to boost the accuracy of the predictor and prevent error propagation between them. The implemented technique is time series classification on datasets from STEREO A and B spacecrafts. The LCNN prediction system of IRs provides advanced Notice Time (NT) interval between [20, 160] minutes with sensitivity around 93% and geometric mean score gmean of 91.7%, and the skills decrease with increasing the prediction time. The LCNN demonstrates an enhancement in the prediction with respect to using only either the CNN or LSTM models. The predicted probabilities are recalibrated so that the predicted frequency of IRs becomes on average consistent with the observed frequency. Application of the method is useful to provide a classification of IRs by inputting a time series and estimating the likelihood of occurrence of an IR and its arrival time on the observer.
AB - Stream interaction region (SIR) is one of the space weather phenomena that accelerates the upstream particles of the interface region in interplanetary space and causes geomagnetic storms. SIRs are large-scale structures that vary temporally and spatially, both in latitudinal and radial directions. Predicting the arrival times of interface regions (IRs) is crucial to protect our navigation and communication systems. In this work, a 1D ensemble system comprised of a Long-short-term memory (LSTM) model and a Convolution Neural Network (CNN) model—LCNN is introduced to classify the observed IR time series and give the prediction interval nowcast of its transit time to the observer. The outcomes of the two models are combined in a way to boost the accuracy of the predictor and prevent error propagation between them. The implemented technique is time series classification on datasets from STEREO A and B spacecrafts. The LCNN prediction system of IRs provides advanced Notice Time (NT) interval between [20, 160] minutes with sensitivity around 93% and geometric mean score gmean of 91.7%, and the skills decrease with increasing the prediction time. The LCNN demonstrates an enhancement in the prediction with respect to using only either the CNN or LSTM models. The predicted probabilities are recalibrated so that the predicted frequency of IRs becomes on average consistent with the observed frequency. Application of the method is useful to provide a classification of IRs by inputting a time series and estimating the likelihood of occurrence of an IR and its arrival time on the observer.
KW - Machine Learning in Heliophysics
KW - COMPUTATIONAL GEOPHYSICS
KW - Neural networks, fuzzy logic, machine learning
KW - EXPLORATION GEOPHYSICS
KW - Gravity methods
KW - GEODESY AND GRAVITY
KW - Transient deformation
KW - Tectonic deformation
KW - Time variable gravity
KW - Gravity anomalies and Earth structure
KW - Satellite geodesy: results
KW - Seismic cycle related deformations
KW - HYDROLOGY
KW - Estimation and forecasting
KW - Extreme events
KW - Time series analysis
KW - INFORMATICS
KW - Forecasting
KW - Machine learning
KW - Temporal analysis and representation
KW - INTERPLANETARY PHYSICS
KW - Solar wind plasma
KW - IONOSPHERE
KW - MAGNETOSPHERIC PHYSICS
KW - MATHEMATICAL GEOPHYSICS
KW - Prediction
KW - Probabilistic forecasting
KW - Persistence, memory, correlations, clustering
KW - Stochastic processes
KW - OCEANOGRAPHY: GENERAL
KW - Ocean predictability and prediction
KW - Time series experiments
KW - NATURAL HAZARDS
KW - Monitoring, forecasting, prediction
KW - NONLINEAR GEOPHYSICS
KW - Probability distributions, heavy and fat‐tailed
KW - Scaling: spatial and temporal
KW - POLICY SCIENCES
KW - RADIO SCIENCE
KW - Interferometry
KW - Ionospheric physics
KW - SEISMOLOGY
KW - Continental crust
KW - Earthquake dynamics
KW - Earthquake source observations
KW - Earthquake interaction, forecasting, and prediction
KW - Seismicity and tectonics
KW - Subduction zones
KW - SPACE PLASMA PHYSICS
KW - Stochastic phenomena
KW - SPACE WEATHER
KW - Policy
KW - Research Article
UR - https://www.scopus.com/pages/publications/85152545180
U2 - 10.1029/2022sw003326
DO - 10.1029/2022sw003326
M3 - Article
SN - 1542-7390
VL - 21
JO - Space Weather
JF - Space Weather
IS - 3
M1 - e2022SW003326
ER -