'Solar wind flow' presentation slideshows

Mike Lockwood STFC/Rutherford Appleton Laboratory & Southampton University

How the Sun Influences Modern Life. Mike Lockwood STFC/Rutherford Appleton Laboratory & Southampton University Our life-giving star: the flow of energy from the Sun to the Earth BA Festival of Science, York, Monday 10 th September 2007. How the Sun Influences Modern Life.

598 views • 42 slides

The Solar Wind

The Solar Wind. J. T. Gosling LASP, University of Colorado. June 12, 2007. The solar wind is a plasma, i.e., an ionized gas, that fills the solar system. It results from the supersonic expansion of the solar corona.

517 views • 28 slides

A Global Hybrid Simulation Study of the Solar Wind Interaction with the Moon

421 views • 25 slides

Solar wind turbulence from radio occultation data

Solar wind turbulence from radio occultation data. Chashei, I.V. Lebedev Physical Institute, Moscow, Russia Efimov, A.I., Institute of Radio Engineering & Electronics, Moscow, Russia Bird, M.K. Radio Astronomical Institute, Univ. Bonn, Bonn, Germany. TURBULENCE.

317 views • 19 slides

Texture of the Solar-Wind Plasma

Texture of the Solar-Wind Plasma. Turbulence is confined to flux tubes. Median diameter is ~5x10 5 km. Plasma in each flux tube differs. Field-line wandering is confined to inside a flux tube. Flux tubes move independently in the macroscale flow of the solar wind.

245 views • 9 slides

To Kinetic Modeling of Solar Wind over Magnetoactive Regions and Beyond

To Kinetic Modeling of Solar Wind over Magnetoactive Regions and Beyond V.Gubchenko (1), V. Zaitsev(1), H.Biernat (2), M. Khodachenko (2), and H. Rucker(2)

115 views • 1 slides