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authFullName_s : P. K. Smolarkiewicz

Direct numerical simulation of fully saturated flow in natural porous media at the pore scale: a comparison of three computational systems

M. Siena , J. D. Hyman , M. Riva , A. Guadagnini , C. L. Winter , et al.
Computational Geosciences, 2015, 19 (2), pp.423-437. ⟨10.1007/s10596-015-9486-7⟩
Journal articles hal-01174152v1

What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?

G. Guerrero , B. Zaire , P. K. Smolarkiewicz , E. M. de Gouveia Dal Pino , A. G. Kosovichev , et al.
The Astrophysical Journal, 2019, 880, ⟨10.3847/1538-4357/ab224a⟩
Journal articles insu-03674431v1