找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

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

[復制鏈接]
查看: 50773|回復: 59
樓主
發(fā)表于 2025-3-21 17:44:45 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Virtual Astrophysical Jets
副標題Theory Versus Observ
編輯Silvano Massaglia,Gianluigi Bodo,Paola Rossi
視頻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
圖書封面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
關鍵詞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

書目名稱Virtual Astrophysical Jets影響因子(影響力)




書目名稱Virtual Astrophysical Jets影響因子(影響力)學科排名




書目名稱Virtual Astrophysical Jets網絡公開度




書目名稱Virtual Astrophysical Jets網絡公開度學科排名




書目名稱Virtual Astrophysical Jets被引頻次




書目名稱Virtual Astrophysical Jets被引頻次學科排名




書目名稱Virtual Astrophysical Jets年度引用




書目名稱Virtual Astrophysical Jets年度引用學科排名




書目名稱Virtual Astrophysical Jets讀者反饋




書目名稱Virtual Astrophysical Jets讀者反饋學科排名




單選投票, 共有 0 人參與投票
 

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

您所在的用戶組沒有投票權限
沙發(fā)
發(fā)表于 2025-3-21 21:11:53 | 只看該作者
板凳
發(fā)表于 2025-3-22 01:20:21 | 只看該作者
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.
地板
發(fā)表于 2025-3-22 08:20:05 | 只看該作者
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./..
5#
發(fā)表于 2025-3-22 09:47:42 | 只看該作者
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.
6#
發(fā)表于 2025-3-22 14:47:46 | 只看該作者
7#
發(fā)表于 2025-3-22 20:11:35 | 只看該作者
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
8#
發(fā)表于 2025-3-22 21:39:44 | 只看該作者
9#
發(fā)表于 2025-3-23 03:53:33 | 只看該作者
Nektarios VlahakisGewebsneubildungen sind. Das ?u?erliche 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.
10#
發(fā)表于 2025-3-23 06:13:11 | 只看該作者
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.
 關于派博傳思  派博傳思旗下網站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網 吾愛論文網 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經驗總結 SCIENCEGARD IMPACTFACTOR 派博系數 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網安備110108008328) GMT+8, 2025-10-8 10:07
Copyright © 2001-2015 派博傳思   京公網安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
如皋市| 罗山县| 高雄市| 龙口市| 乌拉特后旗| 射阳县| 白河县| 永寿县| 阜南县| 黄石市| 承德市| 吉安县| 汝州市| 宾阳县| 金阳县| 娄烦县| 新沂市| 桐乡市| 绍兴市| 浦江县| 汾阳市| 阜南县| 辽阳县| 呼伦贝尔市| 尤溪县| 新建县| 佳木斯市| 牙克石市| 大同市| 九寨沟县| 防城港市| 庆元县| 米易县| 常熟市| 长阳| 上高县| 云龙县| 上栗县| 湛江市| 阳高县| 阿城市|