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020 _a9783540383550
_9978-3-540-38355-0
024 7 _a10.1007/3-540-54420-8
_2doi
050 4 _aQC1-75
072 7 _aPH
_2bicssc
072 7 _aSCI055000
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072 7 _aPH
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082 0 4 _a530
_223
245 1 0 _aChallenges to Theories of the Structure of Moderate-Mass Stars
_h[electronic resource] :
_bProceedings of a Conference Held at the Institute for Theoretical Physics University of California, Santa Barbara, CA, USA 19–22 June 1990 /
_cedited by Douglas Gough, Juri Toomre.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c1991.
300 _aVII, 414 p.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aLecture Notes in Physics,
_x0075-8450 ;
_v388
505 0 _aProgram at ITP: Helioseismology — Probing the interior of a star -- Solar oscillations and the physics of the solar interior -- Helium gravitational settling below the solar convection zone -- Influence of the upper layers of the sun on the p-mode frequencies -- Accuracy tests for the computation of solar models -- Comparison of solar models with Los Alamos and Livermore opacities -- Helioseismic inversion -- An inversion for the rotation rate in the solar interior -- The role of f modes in the inversion of high-? rotational splittings -- On the 2-dimensional rotational inversion problem -- Implication of the l dependence and the frequency dependence of long-term frequency variation -- A new inversion for the hydrostatic stratification of the sun -- Absorption of p-mode waves by magnetic fields -- Prospects of solar Quantum Chaos -- Granulation: Non-adiabatic patterns and shocks -- Large eddy simulations of compressible convection -- Theoretical spectrum of solar convection -- The supergranulation spectrum -- Vertically coherent compressible convective flows in a layer with a high density contrast -- High wavenumber thermal convection enhanced in regions of partial ionization -- The organization of turbulent convection -- Convection and its influence on oscillations -- Interaction of acoustic oscillations with time-dependent compressible convection -- The vibrational stability of the sun -- Convective penetration into stellar radiation zones -- The effects of magnetic stretching in the convective overshoot region -- Towards a theory of wave transport -- Transport in oscillatory flows -- Simulation of the effect of active regions on intermediate-degree solar oscillations -- Effects of spatial filtering on high-? power spectra and rotational splitting inversions -- On the analysis of physical wave trains -- Solar oscillation ring diagrams from Mt. Wilson full-disk magneto-optical Dopplergrams -- Measurements of intermediate- and high-degree (20 l.
520 _aThis book summarizes the latest advances in helioseismology, including the measurement of the internal stratification of the sun, the assessment of thesensitivity of oscillations to uncertainties in fundamental physics, and thestudy of the angular velocity and the dynamics of the convection zone. Of particular interest is the structure of the solar core and its relevance to the neutrino problem. The understanding so gained permits one to look ahead confidently to problems concerning the evolution of sun-like starsthat might be addressed by seismological techniques.
650 0 _aPhysics.
650 1 4 _aPhysics, general.
_0http://scigraph.springernature.com/things/product-market-codes/P00002
700 1 _aGough, Douglas.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
700 1 _aToomre, Juri.
_eeditor.
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710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783662138212
776 0 8 _iPrinted edition:
_z9783540544203
776 0 8 _iPrinted edition:
_z9783662138205
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v388
856 4 0 _uhttps://doi.org/10.1007/3-540-54420-8
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