Improving Multiday Solar Wind Speed Forecasts

We analyze the residual errors for the Wang-Sheeley-Arge (WSA) solar wind speed forecasts as a function of the photospheric magnetic field expansion factor (fp) and the minimum separation angle (d) in the photosphere between the footpoints of open field lines and the nearest coronal hole boundary. W...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Space Weather 2022-09, Vol.20 (9), p.n/a
Hauptverfasser:	Elliot, H A, Arge, C N, Henney, C J, Dayeh, M A, Livadiotis, G, Jahn, J.-M, DeForest, C E
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Analysis Charged particles Corona Coronal hole boundaries Density Error correction Field strength forecast geoeffective Interplanetary magnetic field Lead time Magnetic fields Magnetosphere Mathematical models Meteorology and Climatology Photosphere Photospheric magnetic fields Solar magnetic field Solar wind Solar wind density Solar wind speed Space weather speed Weather Weather forecasting Wind speed
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!