故障 发表于 2025-3-21 19:52:49
书目名称Inside the Sun影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0467822<br><br> <br><br>书目名称Inside the Sun读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0467822<br><br> <br><br>烧烤 发表于 2025-3-22 00:17:48
Inside the Sun : Unsolved Problemshe meeting. In this brief overview of the presently unsolved questions I shall insist on some special aspects of the solar properties: the variations of the solar radius, the generation of the solar wind, some interesting effects due to the presence of a strong gradient of .He, the history of the roEXTOL 发表于 2025-3-22 00:57:39
The Standard Solar Modele given. The input parameters that cause the greatest uncertainties in the calculated neutrino fluxes are the nuclear rection rates, the chemical abundances, the radiative opacity, and the equation of state. This article is based, with permission of the publisher, on Chapters 1 and 4 of . by J. N. Bsperse 发表于 2025-3-22 05:11:05
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Comments on Solar Convectionon is a convective phenomenon that fits well into the gap between granulation and supergranulation. Apparently this observation justifies the view that the three members of the granulation family represent sections of a broad continuum of convective motions spanning the range of sizes from a yet unkessential-fats 发表于 2025-3-22 22:35:52
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Solar Neutrino Projectsr,…) to solve the solar neutrino problem that was raised by the chlorine and the Kamiokande results. The separation of the different sources of neutrinos in the Sun would contribute significantly to the astrophysical understanding of the Sun. Some of the planned experiments could be able to pinpoint