activity
20032026
most citedA Millennium Scale Sunspot Number Reconstruction: Evidence For an Unusually Active Sun Since the 1940's

242 citations · 1.7k across the 39 of their papers we have counts for

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physics.space-ph2019★ 12 cited

Structure and evolution of the photospheric magnetic field in 2010 - 2017: comparison of SOLIS/VSM vector field and potential field

Ilpo I. Virtanen, Alexei A. Pevtsov, Kalevi Mursula

The line-of-sight (LOS) component of the large-scale photospheric magnetic field has been observed since the 1950s, but the daily full-disk observations of the full vector magnetic…

physics.space-ph2019★ 7 cited

Explicit IMF -effect maximizes at subauroral latitudes (Dedicated to the memory of Eigil Friis-Christensen)

Lauri Holappa, Nat Gopalswamy, Kalevi Mursula

The most important parameter in the coupling between solar wind and geomagnetic activity is the -component of the interplanetary magnetic field (IMF). However, recent studies…

physics.space-ph2017★ 37 cited

Automated identification of coronal holes from synoptic EUV maps

Amr Hamada, Timo Asikainen, Ilpo Virtanen +1

Coronal holes (CH) are regions of open magnetic field lines in the solar corona and the source of fast solar wind. Understanding the evolution of coronal holes is critical for sola…

physics.space-ph2017

Principal component analysis of geomagnetic activity: New information on solar wind

Kalevi Mursula, Lauri Holappa

We use the principal component analysis (PCA) to study geomagnetic activity at annual resolution using a network of 26 magnetic stations in 1966-2015, and an extended network of 40…

physics.space-ph2017★ 11 cited

Centennial evolution of monthly solar wind speeds: Fastest monthly solar wind speeds from long-duration coronal holes

Renata Lukianova, Lauri Holappa, Kalevi Mursula

High speed solar wind streams (HSSs) are very efficient drivers of geomagnetic activity at high latitudes. In this paper we use a recently developed parameter of geomagnetic…

physics.space-ph2016★ 27 cited

Seasonal solar wind speeds for the last 100 years: Unique coronal hole structures during the peak and demise of the Grand Modern Maximum

Kalevi Mursula, Lauri Holappa, Renata Lukianova

Solar coronal holes are sources of high-speed solar wind streams, which cause persistent geomagnetic activity especially at high latitudes. Here we estimate seasonal solar wind spe…