TY - JOUR
T1 - The ap Prediction Tool Implemented by the A.Ne.Mo.S./NKUA Group
AU - Mavromichalaki, Helen
AU - Livada, Maria
AU - Stassinakis, Argyris
AU - Gerontidou, Maria
AU - Papailiou, Maria-Christina
AU - Drube, Line
AU - Karmi, Aikaterini
N1 - Publisher Copyright:
© 2024 by the authors.
PY - 2024
Y1 - 2024
N2 - A novel tool utilizing machine learning techniques was designed to forecast ap index values for the next three consecutive days (24 values). The tool employs time series data from the 3 h ap index of solar cycles 23 and 24 to train the Long Short-Term Memory (LSTM) model, predicting ap index values for the next 72 h at three-hour intervals. During periods of quiet geomagnetic activity, the LSTM model’s performance is sufficient to yield favorable outcomes. Nevertheless, during geomagnetically disturbed conditions, such as geomagnetic storms of different levels, the model needs to be adapted in order to provide accurate ap index results. In particular, when coronal mass ejections occur, the ap Prediction tool is modulated by inserting predominant features of coronal mass ejections such as the date of the event, the estimated time of arrival and the linear speed. In the present work, this tool is described thoroughly; moreover, results for G2 and G3 geomagnetic storms are presented.
AB - A novel tool utilizing machine learning techniques was designed to forecast ap index values for the next three consecutive days (24 values). The tool employs time series data from the 3 h ap index of solar cycles 23 and 24 to train the Long Short-Term Memory (LSTM) model, predicting ap index values for the next 72 h at three-hour intervals. During periods of quiet geomagnetic activity, the LSTM model’s performance is sufficient to yield favorable outcomes. Nevertheless, during geomagnetically disturbed conditions, such as geomagnetic storms of different levels, the model needs to be adapted in order to provide accurate ap index results. In particular, when coronal mass ejections occur, the ap Prediction tool is modulated by inserting predominant features of coronal mass ejections such as the date of the event, the estimated time of arrival and the linear speed. In the present work, this tool is described thoroughly; moreover, results for G2 and G3 geomagnetic storms are presented.
KW - Ap geomagnetic index
KW - Coronal mass ejections
KW - Cosmic rays
KW - Geomagnetic activity
U2 - 10.3390/atmos15091073
DO - 10.3390/atmos15091073
M3 - Journal article
AN - SCOPUS:85205062351
SN - 2073-4433
VL - 15
JO - Atmosphere
JF - Atmosphere
IS - 9
M1 - 1073
ER -