Retina
发表于 2025-3-21 18:11:57
书目名称Solar and Stellar Dynamos影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0871460<br><br> <br><br>书目名称Solar and Stellar Dynamos读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0871460<br><br> <br><br>
猜忌
发表于 2025-3-21 20:42:38
Solar and Stellar Dynamos978-3-642-32093-4Series ISSN 1861-7980 Series E-ISSN 1861-8227
misanthrope
发表于 2025-3-22 04:24:10
Saas-Fee Advanced Coursehttp://image.papertrans.cn/s/image/871460.jpg
fodlder
发表于 2025-3-22 05:49:28
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Choreography
发表于 2025-3-22 09:31:35
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问到了烧瓶
发表于 2025-3-22 14:36:56
Dynamo Models of the Solar Cycle,the chapter is on the sun, simply because the amount of available observational material on the solar magnetic field and its cycle dwarfs anything else in the astrophysical realm, in terms of spatial and temporal resolution, sensitivity, and time span.
outset
发表于 2025-3-22 20:41:58
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Anhydrous
发表于 2025-3-22 23:14:44
Magnetohydrodynamics, as magnetic energy, helicity, vector potential, flux-freezing and force-free magnetic fields are also introduced and discussed. The chapter closes with a simple example of a mechanical dynamo, and a discussion of the astrophysical dynamo problem in general terms.
Dappled
发表于 2025-3-23 02:50:08
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Crater
发表于 2025-3-23 09:19:33
Fluctuations, Intermittency and Predictivity,rities and time delay are considered in turn. The occurrence of intermittency in a subset of these models is then investigated, with an eye on explaining Grand Minima observed in the solar activity record. The chapter closes with a brief discussion of solar cycle prediction schemes based on dynamo models.