Titlebook: Helioseismology, Asteroseismology, and MHD Connections; Laurent Gizon,Paul Cally,John Leibacher Book 2008 Springer-Verlag New York 2008 GO

金盤是高原

,Angular Momentum Transport in the Sun’s Radiative Zone by Gravito-Inertial Waves,n zones under conditions that are given. We present the modified transport equations and their numerical evaluation in a parameter range that is significant for the Sun. Consequences for the transport of angular momentum inside solar and stellar radiative regions are discussed.

ANTH

Observation and Modeling of the Solar-Cycle Variation of the Meridional Flow,e loss in the active region belt (the only existing quantitative model). We find that the model and the data are in qualitative agreement, although the amplitude of the solar-cycle variation of the meridional flow at 60?Mm is underestimated by the model.

去掉

橡子

,The Solar-Stellar Connection: Magneto-Acoustic Pulsations in 1.5, , – 2, , Peculiar A Stars, Sun. Yet the Sun is but one star, so stellar astronomy is of great interest to solar astronomers for its range of different conditions under which to test theoretical understanding gained from the study of the Sun. The rapidly oscillating peculiar A stars are of particular interest to solar astrono

JEER

Fourier Analysis of Gapped Time Series: Improved Estimates of Solar and Stellar Oscillation Parametof stellar oscillation. The precision of these measurements depends on the total length (.), quality, and completeness of the observations. Except in a few simple cases, the effect of gaps in the data on measurement precision is poorly understood, in particular in Fourier space where the convolution

pacifist

Perspectives in Global Helioseismology and the Road Ahead,allenges 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

無能力之人

Meridional Circulation and Global Solar Oscillations, Ritzwoller (.., 431, .). As an input flow we use various models of stationary meridional circulation obeying the continuity equation. This flow perturbs the eigenmodes of an equilibrium model of the Sun. We derive the signatures of the meridional circulation in the frequency multiplets of solar . m

Carcinogen

,Global Effects of Local Sound-Speed Perturbations in?the?Sun: A?Theoretical Study,mulations of the solar acoustic wave field. Extending the method of realization-noise subtraction (., Hanasoge, Duvall, and Couvidat, .., 1234, .) to global modes and exploiting the luxury of full spherical coverage, we are able to achieve very highly resolved frequency differences that are then use

ABASH

,Angular Momentum Transport in the Sun’s Radiative Zone by Gravito-Inertial Waves,nt in understanding the evolution of stellar rotation and can explain the Sun’s quasi-flat internal-rotation profile. Because the Sun’s rotation frequency is of the same order as that of the waves, it is now necessary to refine our description of wave propagation and to take into account the action

Genome