GeoDinamo- Glatzmaier
Amtc_presentation
AMT&C
AMT&C presentation
Katalog produk-kikusui-dc-power-supply-pbzseries-tridinamika
How much helicity is needed to drive large-scale dynamos?
“Making Galaxies Red and Dead Without Feedback” T.Naab, P. Johansson, K. Nagamine, G.Efstathiou, RY Cen and J.P.O. Cambridge, 8 May 2008 “Making Normal.
Laser Magnetized Plasma Interactions for the Creation of Solid Density Warm (~200 eV) Matter M.S. Bakeman @, R. Presura, Y. Sentoku, A. Kemp, C. Plechaty,
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
Influence of turbulence on the dynamo threshold B. Dubrulle, GIT/SPEC N. Leprovost, R. Dolganov, P. Blaineau J-P. Laval and F. Daviaud.
Magnetic Activity Astronomy 315 Professor Lee Carkner Lecture 11.
Turbulent Dynamos and Small-Scale Activity in the Sun and Stars George H. Fisher Dave Bercik Chris Johns-Krull Lauren Alsberg Bill Abbett.
