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...

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Bibliographic Details
Main Authors: Lukianova, R. (Renata), Holappa, L. (Lauri), Mursula, K. (Kalevi)
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union 2017
Subjects:
Online Access:http://urn.fi/urn:nbn:fi-fe201903057167