Capricious 发表于 2025-3-21 17:44:45

书目名称Virtual Astrophysical Jets影响因子(影响力)<br>        http://impactfactor.cn/if/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets影响因子(影响力)学科排名<br>        http://impactfactor.cn/ifr/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets网络公开度<br>        http://impactfactor.cn/at/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets网络公开度学科排名<br>        http://impactfactor.cn/atr/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets被引频次<br>        http://impactfactor.cn/tc/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets被引频次学科排名<br>        http://impactfactor.cn/tcr/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets年度引用<br>        http://impactfactor.cn/ii/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets年度引用学科排名<br>        http://impactfactor.cn/iir/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets读者反馈<br>        http://impactfactor.cn/5y/?ISSN=BK0983288<br><br>        <br><br>书目名称Virtual Astrophysical Jets读者反馈学科排名<br>        http://impactfactor.cn/5yr/?ISSN=BK0983288<br><br>        <br><br>

火海 发表于 2025-3-21 21:11:53

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试验 发表于 2025-3-22 01:20:21

The Origin of Jets from Young Stars: Steady State Disk Wind Models Confronted to Observationstoroidal velocities imply large ejection efficiencies (.), suggesting that thermal gradients (originating in an accretion heated disk corona for example) play an important role in accelerating the flow.

冒烟 发表于 2025-3-22 08:20:05

The Efficiency of the Magnetic Acceleration in Relativistic Jets flux ratio. We discuss how these values depend on the conditions near the origin of the flow. By employing self-similar solutions we verify the above result, and show that a Poynting-dominated flow near the source reaches equipartition between Poynting and matter energy fluxes, or even becomes matter-dominated, depending on the value of σ./..

过份艳丽 发表于 2025-3-22 09:47:42

On the MHD Acceleration of Astrophysical Jetsm poloidal magnetic field, we show how both the accretion flow and the acceleration of the outflow occur, and we present in detail which are the forces responsible for the jet launching and collimation. Our simulation also shows how the collimating forces due to the self-generated toroidal magnetic field can produce some peculiar knotty features.

Cabinet 发表于 2025-3-22 14:47:46

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古文字学 发表于 2025-3-22 20:11:35

eils im historischen Kontext betrachtet werden müssen. Dieser Titel erschien in der Zeit vor 1945 und wird daher in seiner zeittypischen politisch-ideologischen Ausrichtung vom Verlag nicht beworben.978-3-8070-0204-0978-3-642-96016-1

善变 发表于 2025-3-22 21:39:44

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无辜 发表于 2025-3-23 03:53:33

Nektarios VlahakisGewebsneubildungen sind. Das äußerliche Merkmal einer umschriebenen Anschwellung ist nicht ausschlaggebend, da es auch durch Exsudat und Transsudat hervorgerufen wird, und andererseits bei einem Teil der Geschwülste fehlen kann.

胡言乱语 发表于 2025-3-23 06:13:11

Oklahoma Notes, Anatomy contains self-assessment questions, geared to the current USMLE format; tables and figures to promote rapid self-assessment and review; a low price; and coverage of just the information needed to ensure Boards success.
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查看完整版本: Titlebook: Virtual Astrophysical Jets; Theory Versus Observ Silvano Massaglia,Gianluigi Bodo,Paola Rossi Book 2004 Springer Science+Business Media Dor