On the Differences in the Ambient Solar Wind Speed Forecasting Caused by Using Synoptic Maps from Different Observatories

We consider the problem of forecasting the solar wind speed using not only well-known magnetic field data sets, such as the Wilcox Solar Observatory (WSO) and the Global Oscillations Network Group (GONG) but others, such as the Infrared Magnetograph (IRmag) at the National Astronomical Observatory o...

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Veröffentlicht in:	Solar physics 2023-10, Vol.298 (10), p.120, Article 120
Hauptverfasser:	Demidov, M. L., Hanaoka, Y., Wang, X. F., Kirichkov, P. N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics and Astroparticles Atmospheric Sciences Celestial bodies Charged particles Coronal hole boundaries Coronal holes Coronal magnetic fields Datasets Empirical equations Field strength Forecasting Infrared astronomy Magnetic fields Mathematical models Observatories Photosphere Physics Physics and Astronomy Potential fields Solar magnetic field Solar observatories Solar physics Solar rotation Solar wind Solar wind speed Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Wind speed Wind speed forecasting
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