DEIFY
发表于 2025-3-21 19:11:16
书目名称Challenges to Theories of the Structure of Moderate-Mass Stars影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0223532<br><br> <br><br>书目名称Challenges to Theories of the Structure of Moderate-Mass Stars读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0223532<br><br> <br><br>
他很灵活
发表于 2025-3-21 22:01:03
Phanerozoic Phosphorite Depositional Systemsrequired to reproduce the results. A good fit was obtained with a kinetic energy spectrum which peaks at ℓ } 100 and decreases exponentially out to ℓ } 500 with an e-folding range of Δℓ } 90. A power law fit to the spectrum over this range in ℓ yields an exponent of about −2.75. No corrections for s
深渊
发表于 2025-3-22 00:42:42
Challenges to Theories of the Structure of Moderate-Mass StarsProceedings of a Con
Cpap155
发表于 2025-3-22 06:01:53
Helium gravitational settling below the solar convection zone,olar outer layers by as much as 20% in the standard models. However the necessity of explaining also the lithium destruction in the sun and solar type stars reduces the expected helium depletion to a few percent.
储备
发表于 2025-3-22 10:32:01
Helioseismic inversion,ructure and dynamics of the solar interior. Some basic concepts and a few inversion techniques are discussed. Results on solar rotation and radial stratification are reviewed, and finally the potential for investigating other moderate-mass stars seismologically is considered.
清澈
发表于 2025-3-22 16:34:18
On the 2-dimensional rotational inversion problem,the forward and inverse problem, in both the 1-dimensional case (with possible expansion in latitude and the full 2-dimensional case. Some preliminary results of running these programs are presented here, together with an outline of the whole package.
清澈
发表于 2025-3-22 17:52:40
http://reply.papertrans.cn/23/2236/223532/223532_7.png
Clumsy
发表于 2025-3-22 21:55:09
Prospects of solar Quantum Chaos,distribution of the spacings violates the Poisson distribution, which should hold under conditions of spherical symmetry of the equilibrium state of the sun. The relevance of this result in connection with inversion problems is briefly emphasised.
吵闹
发表于 2025-3-23 03:14:26
Granulation: Non-adiabatic patterns and shocks,ions of the solar granulation, and illustrate the corresponding pressure and velocity fields. In particular, the non-adiabatic part of the pressure fluctuation, which is a major source of stochastic excitation of P-modes, is shown.
quiet-sleep
发表于 2025-3-23 07:26:56
Theoretical spectrum of solar convection, by linearly superposing these modes to yield the model convective flux profile. The numerical results are compared with the observed spectrum of solar convection and the technique is applied to other stars.