arousal
发表于 2025-3-30 11:45:34
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ticlopidine
发表于 2025-3-30 14:33:15
The Structure of the Chromospheree relevant for the discussion of element fractionation, is limited. Given the dynamic nature of the chromosphere and the poorly understood magnetic linkage to the corona, it is unlikely that we will soon know the detailed processes leading to FIP fractionation.
aqueduct
发表于 2025-3-30 18:47:21
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Mystic
发表于 2025-3-30 21:51:30
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就职
发表于 2025-3-31 03:40:23
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AUGUR
发表于 2025-3-31 07:38:23
Sensitivity of Low Frequency Oscillations to Updated Solar Modelsequencies of p and g modes have been computed for a set of solar models with updated physics (Morel et al., 1997). We analyze their sensitivity to solar parameters like age and metallicity, and to various physical processes, like convective core overshoot and mass loss during the beginning of solar evolution
坚毅
发表于 2025-3-31 11:09:08
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朴素
发表于 2025-3-31 14:59:10
The ‘Standard’ Suniven these assumptions, the constraint that the model have the observed surface luminosity provides an estimate of the initial solar helium abundance. From helioseismic analyses further information can be obtained about the present composition, including a fairly precise measure of the envelope heli
Synchronism
发表于 2025-3-31 18:44:03
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Initiative
发表于 2025-3-31 22:06:49
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