Centennial evolution of monthly solar wind speeds:fastest monthly solar wind speeds from long‐duration coronal holes
Abstract High‐speed solar wind streams (HSSs) are very efficient drivers of geomagnetic activity at high latitudes. In this paper we use a recently developed ΔH parameter of geomagnetic activity, calculated from the nightside hourly magnetic field measurements of the Sodankylä observatory, as a prox...
Main Authors: | , , |
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Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
American Geophysical Union
2017
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Subjects: | |
Online Access: | http://urn.fi/urn:nbn:fi-fe201903057167 |