期刊
SOLAR PHYSICS
卷 284, 期 2, 页码 297-314出版社
SPRINGER
DOI: 10.1007/s11207-012-0172-9
关键词
Helioseismology, direct modeling; Waves, modes; Velocity fields, photosphere
资金
- Italian Space Agency (ASI)
- PRIN-INAF
There are three major issues in modeling solar evanescent oscillations: the variation of the intensity [I]-velocity [V] phase difference of p-modes close to the base of photosphere; the existence of a plateau of negative I-V phase differences below and between the ridges of the low-frequency p-modes; the explanation of the I-V cross-spectra of the evanescent oscillations. We present new interpretations for the first two issues, based on modeling intensity fluctuations taking steep temperature gradients, opacity, and non-adiabatic cooling into account. We also discuss consequences of our model for the explanation of power spectra and cross-power spectra of p-modes. In particular, we present evidence that the acoustic sources that generate evanescent waves produce a coherent background that explains the plateau-interridge regime of negative I-V phase difference.
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