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Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds

Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds

Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Outline: Turbulence as a driver of coronal heating & wind acceleration Kinetic partitioning to protons, electrons, and ions.

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841 views • 63 slides
Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds

Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds

Applications of MHD Turbulence to Modeling Solar (and Stellar) Coronal Heating and Winds. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Outline: Turbulence as a driver of coronal heating & wind acceleration Kinetic partitioning to protons, electrons, and ions.

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640 views • 63 slides
Solar Wind Origin & Heating 2

Solar Wind Origin & Heating 2

Solar Wind Origin & Heating 2. 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

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475 views • 47 slides
Ion Heating in the Solar Corona

Ion Heating in the Solar Corona

Ion Heating in the Solar Corona. Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics. Ion Heating in the Solar Corona. Outline: 1. Remote-sensing (UV coronagraph spectroscopy) 2. Follow the ion cyclotron trail to. . . 3. Anisotropic MHD turbulence, and . . .

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718 views • 45 slides
Turbulence and Wave Dissipation in the Chromosphere, Corona, and Solar Wind

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?.

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512 views • 36 slides
S. R. Cranmer 1 , B. D. G. Chandran 2 , and A. A. van Ballegooijen 1

S. R. Cranmer 1 , B. D. G. Chandran 2 , and A. A. van Ballegooijen 1

Tools for Predicting the Rates of Turbulent Heating for Protons, Electrons, & Heavy Ions in the Solar Wind. S. R. Cranmer 1 , B. D. G. Chandran 2 , and A. A. van Ballegooijen 1 (1) Harvard-Smithsonian CfA , (2) UNH. The Sun- heliosphere plasma system. The Sun- heliosphere plasma system.

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366 views • 26 slides

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