Perspectives in Global Helioseismology, and the Road Ahead
arXiv:0801.4213 · doi:10.1007/s11207-008-9136-5
Abstract
We review the impact of global helioseismology on key questions concerning the internal structure and dynamics of the Sun, and consider the exciting challenges the field faces as it enters a fourth decade of science exploitation. We do so with an eye on the past, looking at the perspectives global helioseismology offered in its earlier phases, in particular the mid-to-late 1970s and the 1980s. We look at how modern, higher-quality, longer datasets coupled with new developments in analysis, have altered, refined, and changed some of those perspectives, and opened others that were not previously available for study. We finish by discussing outstanding challenges and questions for the field.
arXiv commentInvited review; to appear in Solar Physics (24 pages, 6 figures)
References in corpus (56)
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- The 'Forbidden' Abundance of Oxygen in the Sun
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- Line formation in solar granulation: IV. [O I], OI and OH lines and the photospheric O abundance
- A Reappraisal of the Solar Photospheric C/O Ratio
- Up-dated opacities from the Opacity Project
- Influence of gravity waves on the internal rotation and Li abundance of solar-type stars
- Helioseismological Implications of Recent Solar Abundance Determinations
- Constraining solar abundances using helioseismology
- Line formation in solar granulation VI. [C I], C I, CH and C2 lines and the photospheric C abundance
- Solar differential rotation and meridional flow: The role of a subadiabatic tachocline for the Taylor-Proudman balance
- Deeply penetrating banded zonal flows in the solar convection zone
- Are Standard Solar Models Reliable?
- Stellar Evolution with Rotation and Magnetic Fields IV: The Solar Rotation Profile
- Changes in Solar Dynamics from 1995 to 2002
- Surprising Sun
- Helioseismic determination of the solar gravitational quadrupole moment
- Origin of the torsional oscillation pattern of solar rotation
- Excitation of solar-like oscillations across the HR diagram
- Magnetic confinement of the solar tachocline
- Solar Carbon Monoxide, Thermal Profiling, and the Abundances of C, O, and their Isotopes
- What Is The Neon Abundance Of The Sun?
- The Rotation Of The Deep Solar Layers
- The discrepancy between solar abundances and helioseismology
- Temporal variations of the rotation rate in the solar interior
- Can Enhanced Diffusion Improve Helioseismic Agreement for Solar Models with Revised Abundances?
- The subsurface radial gradient of solar angular velocity from MDI f-mode observations
- Sources of oscillation frequency increase with rising solar activity
- Determining solar abundances using helioseismology
- Solar abundances and helioseismology: fine structure spacings and separation ratios of low-degree p modes
- Temporal variations of solar rotation rate at high latitudes
- Line formation in solar granulation VII. CO lines and the solar C and O isotopic abundances
- The Ne/O abundance ratio in the quiet Sun
- On The Determination of MDI High-Degree Mode Frequencies
- Observational Tests and Predictive Stellar Evolution II: Non-standard Models
- Neon Lights Up a Controversy: the Solar Ne/O Abundance
- Solar heavy element abundance: constraints from frequency separation ratios of low-degree p modes
- Changes in the subsurface stratification of the Sun with the 11-year activity cycle
- Spectrum and amplitudes of internal gravity waves excited by penetrative convection in solar-type stars
- Numerical 3D constraints on convective eddy time-correlations : consequences for stochastic excitation of solar p modes
- Low abundances of heavy elements in the solar outer layers: comparisons of solar models with helioseismic inversions
- Observational Searches for Solar g-modes: Some Theoretical Considerations
- Origin of solar torsional oscillations
- Dynamo models and differential rotation in late-type rapidly rotating stars
- Helioseismic test of non-homologous solar radius changes with the 11-year activity cycle
- Does solar structure vary with solar magnetic activity?
- Amplitudes of stochastically excited oscillations in main-sequence stars
- solarFLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data
- Seismic study of the chemical composition of the solar convection zone
- The Non-Homologous Nature of Solar Diameter Variations
- A closure model with plumes I. The solar convection
- A closure model with plumes II. Application to the stochastic excitation of stellar p modes
- Angular momentum conservation and torsional oscillations in the Sun and solar-like stars
- Solar Oscillation Frequency Changes on Time Scales of Nine Days
- Solar Cycle Variations of p-Mode Frequencies
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- Asteroseismology of solar-type stars
- WIYN Open Cluster Study. LXXV. Testing the Metallicity Dependence of Stellar Lithium Depletion Using Hyades-Aged Clusters. 1. Hyades & Praesepe
- Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods
- Global asteroseismic properties of solar-like oscillations observed by Kepler : A comparison of complementary analysis methods
- The solar photospheric abundance of carbon.Analysis of atomic carbon lines with the CO5BOLD solar model
- Solar-like oscillations in KIC11395018 and KIC11234888 from 8 months of Kepler data
- Magnetohydrodynamic waves driven by p-modes
- Alfvénic motions arising from asymmetric acoustic wave drivers in solar magnetic structures
- Asteroseismology of Pulsating Stars
- Seismology of the Sun : Inference of Thermal, Dynamic and Magnetic Field Structures of the Interior