University of Oulu

Space Research GroupIlya Usoskin


My hobby
Position Professor, Head of Oulu Cosmic Ray station
Vice-Director of ReSoLVE Center of Excellence
Address: Sodankyla Geophysical Observatory (Oulu unit) and Dept. of Physics
P.O.Box 3000, FIN-90014 University of Oulu
FINLAND
Telephone: 0503441247
e-mail:
Room: PSOAS-314
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Recent publications:
NEW -> Sturevik-Storm, A., A. Aldahan, G. Possnert, A.-M. Berggren, R. Muscheler, D. Dahl-Jensen, B.M. Vinther, I. Usoskin, 10Be climate fingerprints during the Eemian in the NEEM ice core, Greenland, Sci. Rep., 4, 6408, 2014.

  • Usoskin, I.G., G. Hulot, Y. Gallet, R. Roth, A. Licht, F. Joos, G. A. Kovaltsov, E. Thebault and A. Khokhlov, Evidence for distinct modes of solar activity, Astron. Astrophys., 562, L10, 2014.
  • Kocharov, L., T. Laitinen, I. Usoskin and R. Vainio, Transmission and emission of solar energetic particles in semi-transparent shocks, Astrophys. J. Lett., 787, L21, 2014.
  • Soon, W., V.M. Velasco Herrera, K. Selvaraj, R. Traversi, I. Usoskin, Ch.-T. Chen, J.-Y. Lou, Sh.-J. Kao, R.M. Carter, V. Pipin, M. Severi, S. Becagli, A review of Holocene solar-linked climatic variation on centennial to millennial timescales: Physical processes, interpretative frameworks and a new multiple cross-wavelet transform algorithm, Earth Sci. Rev., 134, 1-15, 2014.
  • Mishev, A.V, L.G. Kocharov and I.G. Usoskin, Analysis of the ground level enhancement on 17 May 2012 using data from the global neutron monitor network, J. Geophys. Res., 119, 670-679, 2014.
  • Poluianov, S., I.G. Usoskin, Critical Analysis of a Hypothesis of the Planetary Tidal Influence on Solar Activity, Solar Phys., 289, 2333-2342, 2014.
  • Mironova, I.A., I.G. Usoskin, Possible effect of strong solar energetic particle events on polar stratospheric aerosol: a summary of observational results, Environ. Res. Lett., 9, 015002, 2014.
  • Kovaltsov, G.A., I.G.Usoskin, Occurrence Probability of Large Solar Energetic Particle Events: Assessment from Data on Cosmogenic Radionuclides in Lunar Rocks, Solar Phys., 289, 211-220, 2014.

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