Latitude–temporal evolution of coronal holes in cycles 21–23

The latitude–temporal evolution of coronal holes (CHs) and time variations in CH areas were studied based on a version of several CHs (Tlatov et al., 2014) from 1975 to 2012. It was shown that two systems of magnetic fields (MFs) play the main role in the 11-year cycle evolution: high-latitude large...

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Veröffentlicht in:	Geomagnetism and Aeronomy 2015-12, Vol.55 (7), p.877-883
Hauptverfasser:	Ikhsanov, R. N., Tavastsherna, K. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aeronomy Anomalies Coronal holes Earth and Environmental Science Earth Sciences Evolution Geomagnetism Geophysics/Geodesy Latitude Magnetic fields Solar cycle Solar cycles Solar physics Studies
Online-Zugang:	Volltext
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