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Turbulence and Magnetic Fields in Astrophysics

Overview of attention for book
Cover of 'Turbulence and Magnetic Fields in Astrophysics'

Table of Contents

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    Book Overview
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    Chapter 1 The Evolving Phenomenological View on Magnetohydrodynamic Turbulence
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    Chapter 2 Coronal Heating and Reduced MHD
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    Chapter 3 MHD Turbulence: Scaling Laws and Astrophysical Implications
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    Chapter 4 Numerical Simulations of Magnetic Fields in Astrophysical Turbulence
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    Chapter 5 Adaptive Mesh Refinement in MHD Modeling. Realization, Tests and Application
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    Chapter 6 Observations of Interstellar Magnetic Fields
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    Chapter 7 MHD Turbulence in Star-Forming Regions and the Interstellar Medium
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    Chapter 8 Thermal Instability and Magnetic Pressure in the Turbulent Interstellar Medium
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    Chapter 9 Developing Diagnostics of Molecular Clouds Using Numerical MHD Simulations
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    Chapter 10 Star Formation and the Initial Mass Function
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    Chapter 11 The Structure and Dynamics of Filamentary Molecular Clouds
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    Chapter 12 Numerical Simulations of MHD Turbulence in Accretion Disks
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    Chapter 13 Recent Developments in Collisionless Reconnection Theory: Applications to Laboratory and Astrophysical Plasmas
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    Chapter 14 Problems and Progress in Astrophysical Dynamos
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    Chapter 15 The Helicity Issue in Large Scale Dynamos
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    Chapter 16 Recent Developments in Magnetic Dynamo Theory
Attention for Chapter 2: Coronal Heating and Reduced MHD
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Citations

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Chapter title
Coronal Heating and Reduced MHD
Chapter number 2
Book title
Turbulence and Magnetic Fields in Astrophysics
Published by
Springer, Berlin, Heidelberg, January 2003
DOI 10.1007/3-540-36238-x_2
Book ISBNs
978-3-54-000274-1, 978-3-54-036238-8
Authors

Sean Oughton, Pablo Dmitruk, William H. Matthaeus, Oughton, Sean, Dmitruk, Pablo, Matthaeus, William H.

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Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 2 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 2 100%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 1 50%
Researcher 1 50%
Readers by discipline Count As %
Physics and Astronomy 2 100%

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