Cassini plasma spectrometer investigation DT Young, JJ Berthelier, M Blanc, JL Burch, AJ Coates, R Goldstein, ... The Cassini-Huygens Mission: Orbiter In Situ Investigations Volume 2, 1-112, 2004 | 576 | 2004 |
Heliospheric modulation of cosmic rays: Monthly reconstruction for 1951–2004 IG Usoskin, K Alanko‐Huotari, GA Kovaltsov, K Mursula Journal of Geophysical Research: Space Physics 110 (A12), 2005 | 511 | 2005 |
First results of electric field and density observations by Cluster EFW based on initial months of operation G Gustafsson, M André, T Carozzi, AI Eriksson, CG Fälthammar, R Grard, ... Annales Geophysicae 19 (10/12), 1219-1240, 2001 | 371 | 2001 |
Millennium-Scale Sunspot Number Reconstruction:<? format?> Evidence for an Unusually Active Sun since the 1940s IG Usoskin, SK Solanki, M Schüssler, K Mursula, K Alanko Physical Review Letters 91 (21), 211101, 2003 | 340 | 2003 |
Composition and dynamics of plasma in Saturn's magnetosphere DT Young, JJ Berthelier, M Blanc, JL Burch, S Bolton, AJ Coates, FJ Crary, ... Science 307 (5713), 1262-1266, 2005 | 320 | 2005 |
Testing the isotropic boundary algorithm method to evaluate the magnetic field configuration in the tail VA Sergeev, M Malkov, K Mursula Journal of Geophysical Research: Space Physics 98 (A5), 7609-7620, 1993 | 243 | 1993 |
The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets IG Usoskin, R Arlt, E Asvestari, E Hawkins, M Käpylä, GA Kovaltsov, ... Astronomy & Astrophysics 581, A95, 2015 | 216 | 2015 |
The 13.5‐day periodicity in the Sun, solar wind, and geomagnetic activity: The last three solar cycles K Mursula, B Zieger Journal of Geophysical Research: Space Physics 101 (A12), 27077-27090, 1996 | 193 | 1996 |
Current sheet thickness in the near‐Earth plasma sheet during substorm growth phase VA Sergeev, P Tanskanen, K Mursula, A Korth, RC Elphic Journal of Geophysical Research: Space Physics 95 (A4), 3819-3828, 1990 | 191 | 1990 |
Long-term solar cycle evolution: review of recent developments IG Usoskin, K Mursula Solar Physics 218, 319-343, 2003 | 184 | 2003 |
A physical reconstruction of cosmic ray intensity since 1610 IG Usoskin, K Mursula, SK Solanki, M Schüssler, GA Kovaltsov Journal of Geophysical Research: Space Physics 107 (A11), SSH 13-1-SSH 13-6, 2002 | 176 | 2002 |
First results from the RAPID imaging energetic particle spectrometer on board Cluster B Wilken, PW Daly, U Mall, K Aarsnes, DN Baker, RD Belian, JB Blake, ... Annales Geophysicae 19 (10/12), 1355-1366, 2001 | 170 | 2001 |
The mass-hierarchy and CP-violation discovery reach of the LBNO long-baseline neutrino experiment L Collaboration, S Agarwalla, L Agostino, M Aittola, A Alekou, B Andrieu, ... JOURNAL OF HIGH ENERGY PHYSICS 2014 (5), 2013 | 166 | 2013 |
RAPID: The imaging energetic particle spectrometer on Cluster B Wilken, WI Axford, I Daglis, P Daly, W Güttler, WH Ip, A Korth, G Kremser, ... The Cluster and Phoenix Missions, 399-473, 1997 | 165 | 1997 |
Reconstruction of solar activity for the last millennium using Be data IG Usoskin, K Mursula, S Solanki, M Schüssler, K Alanko Astronomy & Astrophysics 413 (2), 745-751, 2004 | 151 | 2004 |
Analysis of leptonic charged weak interactions K Mursula, F Scheck Nuclear Physics B 253, 189-204, 1985 | 141 | 1985 |
Observations in the vicinity of substorm onset: Implications for the substorm process RD Elphinstone, DJ Hearn, LL Cogger, JS Murphree, H Singer, ... Journal of Geophysical Research: Space Physics 100 (A5), 7937-7969, 1995 | 135 | 1995 |
A new calibrated sunspot group series since 1749: statistics of active day fractions IG Usoskin, GA Kovaltsov, M Lockwood, K Mursula, M Owens, SK Solanki Solar Physics 291 (9), 2685-2708, 2016 | 130 | 2016 |
Correlative study of solar activity and cosmic ray intensity IG Usoskin, H Kananen, K Mursula, P Tanskanen, GA Kovaltsov Journal of Geophysical Research: Space Physics 103 (A5), 9567-9574, 1998 | 129 | 1998 |
Limits to the Number of Neutrinos: A Comment on the Z 0 Discovery F Halzen, K Mursula Physical Review Letters 51 (10), 857, 1983 | 127 | 1983 |