'Solar wind turbulence' presentation slideshows

Interstellar Turbulence and the Plasma Environment of the Heliosphere

Interstellar Turbulence and the Plasma Environment of the Heliosphere. Steven R. Spangler University of Iowa. The sky as imaged by the Wisconsin H Alpha Mapper (WHAM; Haffner et al 2003, ApJS 149, 405). The Warm Ionized Medium (WIM): where do stellar structures end and turbulence begin?.

491 views • 25 slides

Interplanetary Scintillations and the Acceleration of the Solar Wind

297 views • 17 slides

Spectral Properties of high frequency fluctuations of solar wind plasma

Meeting on Solar Wind Turbulence, Kennebunkport, June 4-7, 2013. Spectral Properties of high frequency fluctuations of solar wind plasma parameters: SPECTR-R data M. Riazantseva 1,2 , G. Zastenker 1 , J. Safrankova 4 , Z. Nemecek 4 , L. Prech 4

187 views • 9 slides

Correlation Length as a Function of B-V Angle

Global Quantities in Solar Wind Turbulence: Effect of B-V Angle and Averaging Interval. Jeffrey Tessein, Joshua Isaacs, and William Matthaeus University of Delaware, Newark, DE. Session: The dissipation of solar wind turbulence. Correlation Length as a Function of B-V Angle.

111 views • 1 slides