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Challenges to Theories of the Structure of Moderate-Mass Stars

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Cover of 'Challenges to Theories of the Structure of Moderate-Mass Stars'

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
Overall attention for this book and its chapters
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Mentioned by

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1 tweeter

Citations

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Readers on

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3 Mendeley
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Title
Challenges to Theories of the Structure of Moderate-Mass Stars
Published by
ADS, January 1991
DOI 10.1007/3-540-54420-8
ISBNs
978-3-54-038355-0, 978-3-54-054420-3
Editors

Gough, Douglas, Toomre, Juri

Twitter Demographics

The data shown below were collected from the profile of 1 tweeter who shared this research output. Click here to find out more about how the information was compiled.

Mendeley readers

The data shown below were compiled from readership statistics for 3 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 3 100%

Demographic breakdown

Readers by professional status Count As %
Researcher 2 67%
Student > Master 1 33%
Readers by discipline Count As %
Physics and Astronomy 2 67%
Nursing and Health Professions 1 33%

Attention Score in Context

This research output has an Altmetric Attention Score of 1. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 30 January 2020.
All research outputs
#9,893,931
of 15,542,315 outputs
Outputs from ADS
#21,254
of 29,456 outputs
Outputs of similar age
#157,509
of 271,451 outputs
Outputs of similar age from ADS
#105
of 211 outputs
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So far Altmetric has tracked 29,456 research outputs from this source. They receive a mean Attention Score of 4.3. This one is in the 19th percentile – i.e., 19% of its peers scored the same or lower than it.
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