'Solar wind acceleration region' presentation slideshows

Solar Wind Origin & Heating 1

Solar Wind Origin & Heating 1. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Logistics. Part 1: Observations. Part 2: Theory. 1. Photosphere: tip of the iceberg of the convection zone 2. Chromosphere: waves start to propagate and bump into the magnetic field

593 views • 46 slides

Solar Wind Origin & Heating 1

Solar Wind Origin & Heating 1. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Logistics. Part 1: Observations. Part 2: Theory. 1. Photosphere: tip of the iceberg of the convection zone 2. Chromosphere: waves start to propagate and bump into the magnetic field

474 views • 46 slides

Turbulence and Wave Dissipation in the Chromosphere, Corona, and Solar Wind

Turbulence and Wave Dissipation in the Chromosphere, Corona, and Solar Wind. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Outline: 1. Background: basic ideas about heating & acceleration 2. Corona and solar wind: 3. Chromosphere: acoustic waves & discrete sources?.

621 views • 36 slides

Turbulence and Waves as Sources for the Solar Wind

517 views • 35 slides