找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Virtual Astrophysical Jets; Theory Versus Observ Silvano Massaglia,Gianluigi Bodo,Paola Rossi Book 2004 Springer Science+Business Media Dor

[复制链接]
查看: 50700|回复: 59
发表于 2025-3-21 17:44:45 | 显示全部楼层 |阅读模式
书目名称Virtual Astrophysical Jets
副标题Theory Versus Observ
编辑Silvano Massaglia,Gianluigi Bodo,Paola Rossi
视频videohttp://file.papertrans.cn/984/983288/983288.mp4
概述Provides a global view on stellar jets and extragalactic jets unlike other books which deal with only one of these.The authors are among the most active scientists in the field of theoretical interpre
图书封面Titlebook: Virtual Astrophysical Jets; Theory Versus Observ Silvano Massaglia,Gianluigi Bodo,Paola Rossi Book 2004 Springer Science+Business Media Dor
描述These proceedings are the result of a three-day meeting held in Oogliani (Italy), on October 2-4 2003, whose title was "VIrtual Astrophysical Jets 2003". Our goal in convening this meeting was to gather some of the scientists among the most active in the field of numerical simulations and modelling of astrophysi­ cal jets. For keeping the participants close to the "real world", we also invited a few observers to give up-to-date reviews outlining the state-of-the-art of jet observations. The principal aim of the meeting was thus to present and critically discuss the state-of-the-art numerical simulations, analytical models and laboratory ex­ periments for reproducing the main aspects of astrophysical jets and compar­ ing them with observations. The discussion has been focused on the following topics: • Observations and intepretions of jets from young stars and AGNs, comparisons of models with observations; • MHO accelerations of jets: steady self-similar models, MHO numerical simula­ tions of time-dependent accelerations mechanisms; • Jet stability and interaction with the ambient: formation of knots in YSO jets, jet survival to instabilities, deceleration of relativistic jets in FR
出版日期Book 2004
关键词Accretion; Galaxy; astrophysics; relativistic jet; star; stellar
版次1
doihttps://doi.org/10.1007/978-1-4020-2664-5
isbn_softcover978-90-481-5856-0
isbn_ebook978-1-4020-2664-5
copyrightSpringer Science+Business Media Dordrecht 2004
The information of publication is updating

书目名称Virtual Astrophysical Jets影响因子(影响力)




书目名称Virtual Astrophysical Jets影响因子(影响力)学科排名




书目名称Virtual Astrophysical Jets网络公开度




书目名称Virtual Astrophysical Jets网络公开度学科排名




书目名称Virtual Astrophysical Jets被引频次




书目名称Virtual Astrophysical Jets被引频次学科排名




书目名称Virtual Astrophysical Jets年度引用




书目名称Virtual Astrophysical Jets年度引用学科排名




书目名称Virtual Astrophysical Jets读者反馈




书目名称Virtual Astrophysical Jets读者反馈学科排名




单选投票, 共有 0 人参与投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用户组没有投票权限
发表于 2025-3-21 21:11:53 | 显示全部楼层
发表于 2025-3-22 01:20:21 | 显示全部楼层
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.
发表于 2025-3-22 08:20:05 | 显示全部楼层
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./..
发表于 2025-3-22 09:47:42 | 显示全部楼层
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.
发表于 2025-3-22 14:47:46 | 显示全部楼层
发表于 2025-3-22 20:11:35 | 显示全部楼层
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
发表于 2025-3-22 21:39:44 | 显示全部楼层
发表于 2025-3-23 03:53:33 | 显示全部楼层
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.
发表于 2025-3-23 06:13:11 | 显示全部楼层
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.
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 吾爱论文网 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
QQ|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-8-5 12:10
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表