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Challenges to Theories of the Structure of Moderate-Mass Stars

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Table of Contents

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    Book Overview
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    Chapter 46 Program at ITP: Helioseismology — Probing the interior of a star
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    Chapter 47 Solar oscillations and the physics of the solar interior
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    Chapter 48 Helium gravitational settling below the solar convection zone
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    Chapter 49 Influence of the upper layers of the sun on the p-mode frequencies
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    Chapter 50 Accuracy tests for the computation of solar models
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    Chapter 51 Comparison of solar models with Los Alamos and Livermore opacities
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    Chapter 52 Helioseismic inversion
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    Chapter 53 An inversion for the rotation rate in the solar interior
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    Chapter 54 The role of f modes in the inversion of high-ℓ rotational splittings
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    Chapter 55 On the 2-dimensional rotational inversion problem
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    Chapter 56 Implication of the l dependence and the frequency dependence of long-term frequency variation
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    Chapter 57 A new inversion for the hydrostatic stratification of the sun
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    Chapter 58 Absorption of p-mode waves by magnetic fields
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    Chapter 59 Prospects of solar Quantum Chaos
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    Chapter 60 Granulation: Non-adiabatic patterns and shocks
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    Chapter 61 Large eddy simulations of compressible convection
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    Chapter 62 Theoretical spectrum of solar convection
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    Chapter 63 The supergranulation spectrum
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    Chapter 64 Vertically coherent compressible convective flows in a layer with a high density contrast
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    Chapter 65 High wavenumber thermal convection enhanced in regions of partial ionization
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    Chapter 66 The organization of turbulent convection
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    Chapter 67 Convection and its influence on oscillations
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    Chapter 68 Interaction of acoustic oscillations with time-dependent compressible convection
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    Chapter 69 The vibrational stability of the sun
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    Chapter 70 Convective penetration into stellar radiation zones
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    Chapter 71 The effects of magnetic stretching in the convective overshoot region
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    Chapter 72 Towards a theory of wave transport
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    Chapter 73 Transport in oscillatory flows
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    Chapter 74 Simulation of the effect of active regions on intermediate-degree solar oscillations
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    Chapter 75 Effects of spatial filtering on high- ℓ power spectra and rotational splitting inversions
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    Chapter 76 On the analysis of physical wave trains
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    Chapter 77 Solar oscillation ring diagrams from Mt. Wilson full-disk magneto-optical Dopplergrams
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    Chapter 78 Measurements of intermediate- and high-degree (20 < l <600) p-mode solar oscillation power and energy
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    Chapter 79 Further evidence for radial variations in the solar equatorial angular velocity profile
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    Chapter 80 Remarks on the evolution of low-mass stars: More or less opaque?
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    Chapter 81 Applications of stellar seismology to intermediate mass stars: On the main sequence and beyond
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    Chapter 82 Surface chemical composition, nuclear processing, and deep mixing: Main sequence to first dredge-up
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    Chapter 83 Main-sequence mass-loss: Lithium dilution in the hyades and the sun
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    Chapter 84 Comparing Victoria and Yale evolutionary tracks
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    Chapter 85 Wimp-like stellar models and the subgiant branch
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    Chapter 86 Problems for the WIMP Hypothesis?
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    Chapter 87 What has happened to arcturs?
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    Chapter 88 Pulsations of Arcturus
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    Chapter 89 Nonadiabatic nonradial pulsations of RCrB stars
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    Chapter 90 Challenges to theories of the structure of moderate mass stars
Attention for Chapter 61: Large eddy simulations of compressible convection
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Chapter title
Large eddy simulations of compressible convection
Chapter number 61
Book title
Challenges to Theories of the Structure of Moderate-Mass Stars
Published in
ADS, January 1991
DOI 10.1007/3-540-54420-8_61
Book ISBNs
978-3-54-054420-3, 978-3-54-038355-0
Authors

Xin Xie, Juri Toomre

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The data shown below were compiled from readership statistics for 1 Mendeley reader of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 1 100%

Demographic breakdown

Readers by professional status Count As %
Researcher 1 100%
Readers by discipline Count As %
Physics and Astronomy 1 100%