Ingratiate
发表于 2025-3-23 11:53:11
SCORe ’96: Solar Convection and Oscillations and their Relationship978-94-011-5167-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
功多汁水
发表于 2025-3-23 14:21:39
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暴发户
发表于 2025-3-23 18:07:29
Near-Surface Constraints on the Structure of Stellar Convection ZonesBy simulating the convection in the upper layers of six different stars and matching these simulations to 1D-mixing length models using the same input physics, we have been able to infer the behaviour of the mixing-length parameter, α, as the stellar parameters changes.
Diatribe
发表于 2025-3-23 23:39:57
Sound Speed Variations Near the Photosphere Due to Entropy Perturbations in 3D Numerical ExperimentsResults on how the temperature distribution near the solar photosphere is altered by perturbing the entropy of rising fluid in the convection zone several megameters below the surface, are presented. Effects on the emergent intensity and implications for helioseismic observations are described.
Sinus-Rhythm
发表于 2025-3-24 04:55:43
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中和
发表于 2025-3-24 07:11:11
Excitation and Damping of Solar Acoustic Oscillations low degree modes is consistent with the observed rates. I describe how asymmetric line profiles of p-modes and the power spectrum above the acoustic cutoff frequency provide information about the source location in the convection zone.
CAB
发表于 2025-3-24 11:08:52
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/s/image/860122.jpg
IRK
发表于 2025-3-24 18:41:30
https://doi.org/10.1007/978-94-011-5167-23D; Chromosphere; Photosphere; Sun; Sunspot; helioseismology; simulation; solar
失望未来
发表于 2025-3-24 19:54:12
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Osteoporosis
发表于 2025-3-25 01:19:55
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