'Fast solar wind' presentation slideshows

Plasma Unbound: Coronal Heating and

Plasma Unbound: Coronal Heating and. New Insights into. Solar / Stellar Winds. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Outline: Overview and brief historical background Heating the coronal base (reconnection & turbulence)

730 views • 60 slides

Plasma Unbound: New Insights into Heating the Solar Corona and Accelerating the Solar Wind

789 views • 58 slides

Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind

Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind. Outline:

793 views • 58 slides

Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind

Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind. Outline:

583 views • 58 slides

Coronal expansion and solar wind

Coronal expansion and solar wind. The large solar corona Coronal and interplanetary temperatures Coronal expansion and solar wind The heliosphere Origin of solar wind in magnetic network Multi-fluid models of the solar wind. The visible solar corona. Eclipse 11.8.1999.

830 views • 52 slides

Sun-Earth Connection and Space Weather

417 views • 32 slides

Solar and Space Physics

363 views • 23 slides

Uncovering the Global Slow Solar Wind

Uncovering the Global Slow Solar Wind. Liang Zhao and Thomas H. Zurbuchen Department of Atmospheric, Oceanic and Space Sciences, University of Michigan. Motivation. The heliosphere consists of three types of solar wind:. Fast wind (Solar wind from coronal holes).

393 views • 23 slides

SLIDE SHOW 6. SOLAR WIND

ionized tail. dust tail. SLIDE SHOW 6. SOLAR WIND. Observations of comets suggested solar outflow (Biermann). Parker (1958) proposed supersonic expansion. Confirmed in 1960s by spacecraft measurements (Mariner 2, 1962). Slow wind (300 km/s) + Fast solar wind (700 km/s).

319 views • 12 slides

Group E: Non-radial magnetic field expansion

182 views • 8 slides