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Exploring the Capabilities of a Machine Learning Algorithm to Detect Space Weather-Significant Emerging Active RegionsActive regions are a source of various phenomena responsible for Space Weather disturbances; therefore, developing a technology for early warning about upcoming magnetic activity is crucial to mitigate its impact. However, observational limitations and the high nonlinearity of processes associated with the accumulation of magnetic flux and its interaction with the surrounding plasma during the emergence through the convection zone make early activity detection a challenging problem.

To address these challenges, we developed a physics-driven machine learning model that allows us to detect active regions (ARs) before they become visible on the solar surface by analyzing the power spectra of acoustic oscillations observed by the SDO/HMI instrument. This study is based on a time series of Doppler shift maps of 31x31-degree areas tracked with the Carrington rotation rate for four days before and after the emergence. The Doppler shift time series are processed into the oscillation power maps for four frequency ranges and accompanied by line-of-sight magnetograms and the continuum intensity maps from SDO/HMI.

The resulting data are converted into a 1D time series representing the mean temporal variations of these quantities. The redacted time series are used as input to predict AR emergence using the Long Short Term Memory (LSTM) method. The training of the LSTM model is based on 40 ARs, which includes an independent analysis for each sub region that exhibits AR emergence or remains quiet. The emergence of magnetic flux (defined as a decrease of the continuum intensity) was detected with the developed LSTM algorithm from 5 to 48 hours before the reported time by NOAA. The developed model is capable of pointing to the time and location of active region formation. In this presentation, we discuss reasons that impact how early in advance the model can identify the upcoming activity and the possibility of improving the current predictive skills and steps to transition to the operational forecast.
Document ID
20240016051
Acquisition Source
Ames Research Center
Document Type
Poster
Authors
Irina N Kitiashvili
(Ames Research Center Mountain View, United States)
Spiridon Kasapis
(Oak Ridge Associated Universities Oak Ridge, United States)
Alexander G Kosovichev
(New Jersey Institute of Technology Newark, United States)
Date Acquired
December 13, 2024
Subject Category
Solar Physics
Aeronautics (General)
Meeting Information
Meeting: American Geophysical Union (AGU 2024)
Location: Washington, D.C.
Country: US
Start Date: December 9, 2024
End Date: December 13, 2024
Sponsors: American Geophysical Union ( AGU)
Funding Number(s)
CONTRACT_GRANT: 80NSSC22M0162
CONTRACT_GRANT: 80NSSC20K1870
CONTRACT_GRANT: 80NSSC19K0268
CONTRACT_GRANT: 80NSSC19K0630
WBS: 791926.02.11.01.08
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Peer Committee
Keywords
Heliophysics
SMD
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