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Browse: Keyword: Magnetohydrodynamics

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2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Density and Magnetic Field

(Complete Item Description)

Abstract:: This series of animations shows a two-dimensional unstructured mesh particle-magneto-hydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earths magnetosphere.

Subject:: Science and Technology
Grade Level:: Secondary, Post-secondary
Collection:: NASA GSFC Scientific Visualization Studio

No Strings Attached

2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Magnetic Potential

(Complete Item Description)

Abstract:: This series of animations shows a two-dimensional unstructured mesh particle-magneto-hydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earths magnetosphere.

Subject:: Science and Technology
Grade Level:: Secondary, Post-secondary
Collection:: NASA GSFC Scientific Visualization Studio

No Strings Attached

Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field

(Complete Item Description)

Abstract:: This series of animations compares a two-dimensional global hybrid simulation with an magnetohydrodynamic model of the interaction of the solar wind with the Earths magnetosphere.

Subject:: Science and Technology
Grade Level:: Secondary, Post-secondary
Collection:: NASA GSFC Scientific Visualization Studio

No Strings Attached

Global Hybrid Versus MHD Modeling of the Magnetosphere: Magnetic Potential

(Complete Item Description)

Abstract:: This series of animations compares a two-dimensional global hybrid simulation with an magneto-hydrodynamic model of the interaction of the solar wind with the Earths magnetosphere.

Subject:: Science and Technology
Grade Level:: Secondary, Post-secondary
Collection:: NASA GSFC Scientific Visualization Studio

MHD Theory of Fusion Systems, Spring 2007

(Complete Item Description)

Abstract:: Derivation of the basic MHD model from the Boltzmann equation. Discussion of MHD equilibria in cylindrical, toroidal, and noncircular tokamaks. Use of MHD equilibrium theory in poloidal field design. MHD stability theory including the Energy Principle, interchange instability, ballooning modes, second region of stability, and external kink modes. Emphasis on discovering configurations capable of achieving good confinement at high beta.

Subject:: Science and Technology
Grade Level:: Post-secondary
Collection:: MIT OpenCourseWare

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Model of the Heliosphere Over the Solar Cycle

(Complete Item Description)

Abstract:: This magnetohydrodynamical (MHD) model shows how the heliosphere of the Sun might interact with the local interstellar medium (ISM) over the course of a single 11 year solar cycle. The sun (and the orbit of the Earth) is located in the tiny blue region in the center. The ISM is moving from left to right. The solar wind varies from 400 km-s up to 566 km-s and back down to 400 km-s over the cycle in this particular model. The colors are logarithmically scaled to represent temperature, with blue around 10,000 Kelvins (in the undisturbed ISM and the region immediately around the Sun) and red over 1,000,000 Kelvins (corresponding to the bow shocked region in the plasma). The green region around the Sun has a radius that varies between 100-200 Astronomical Units.

Subject:: Science and Technology
Grade Level:: Secondary, Post-secondary
Collection:: NASA GSFC Scientific Visualization Studio

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