派博傳思國際中心

標題: Titlebook: Black Hole Gravitohydromagnetics; Brian Punsly Book 20011st edition Springer-Verlag Berlin Heidelberg 2001 Activie Galactic Nuclei.Black H [打印本頁]

作者: 文化修養(yǎng)    時間: 2025-3-21 18:41
書目名稱Black Hole Gravitohydromagnetics影響因子(影響力)




書目名稱Black Hole Gravitohydromagnetics影響因子(影響力)學科排名




書目名稱Black Hole Gravitohydromagnetics網絡公開度




書目名稱Black Hole Gravitohydromagnetics網絡公開度學科排名




書目名稱Black Hole Gravitohydromagnetics被引頻次




書目名稱Black Hole Gravitohydromagnetics被引頻次學科排名




書目名稱Black Hole Gravitohydromagnetics年度引用




書目名稱Black Hole Gravitohydromagnetics年度引用學科排名




書目名稱Black Hole Gravitohydromagnetics讀者反饋




書目名稱Black Hole Gravitohydromagnetics讀者反饋學科排名





作者: Cpr951    時間: 2025-3-21 21:54
Magnetically Dominated Time-Stationary Perfect MHD Winds,current (see Sect. 4.8). Thus, we expect that enough plasma is present in any viable energy extracting scheme so that any memory of the background vacuum electric field is erased from the magnetosphere. Locally, this condition is given by the Goldreich-Julian charge density [80].
作者: Between    時間: 2025-3-22 04:03

作者: 不出名    時間: 2025-3-22 08:10
Bestimmung der Umtriebszeit und Abtriebszeite horizon has no unipolar inductive properties like a Faraday wheel has at the end of a plasma-filled waveguide or transmission line (as discussed in Sect. 2.10). Thus, the event horizon plays no role in any GHM interaction except for being an effective sink for mass influx.
作者: 鳴叫    時間: 2025-3-22 10:31
Zur Statik des Durchforstungsbetriebescurrent (see Sect. 4.8). Thus, we expect that enough plasma is present in any viable energy extracting scheme so that any memory of the background vacuum electric field is erased from the magnetosphere. Locally, this condition is given by the Goldreich-Julian charge density [80].
作者: 確定的事    時間: 2025-3-22 14:50
https://doi.org/10.1007/978-3-662-36474-1ion axis of the black hole (unlike a neutron star), thus there can be no “l(fā)ighthouse effect” and therefore no pulsations. Hence, the new distinct class of compact magnetized objects, NP (nonpulsed) black holes. The term NP black hole refers to the entire electromagnetic structure, including the cent
作者: 有常識    時間: 2025-3-22 21:06
Introduction,o pulsar winds and extragalactic radio jets. It is now widely accepted that 1.. — 20.. black holes populate the galaxies that fill the Universe. Furthermore, water maser mappings with the VLBA (Very Long Baseline Array) and kinematical gas analyses with HST (The Hubble Space Telescope) make a convin
作者: 敬禮    時間: 2025-3-22 21:16

作者: Altitude    時間: 2025-3-23 05:09
Particle Trajectories in the Ergosphere, ., as measured from asymptotic infinity. The preparation of . < 0 matter must occur within the ergosphere. This is related to the fact that the outer boundary of the ergosphere, the stationary limit at . = .. occurs when ./. changes from a timelike vector field to a spacelike vector field (see defi
作者: Terminal    時間: 2025-3-23 05:31
Vacuum Electrodynamics,n the ergosphere. It addresses two core issues that can determine the global flow. Firstly, Maxwell’s equations can be used to determine the electrodynamic nature of spacetime near the event horizon. For example, if the event horizon can impose meaningful boundary conditions electrodynamincally, the
作者: 細頸瓶    時間: 2025-3-23 13:18

作者: avenge    時間: 2025-3-23 14:36
Perfect MHD Winds and Waves in the Ergosphere,t horizon is an asymptotic infinity to MHD winds and waves similar to the infinity of the semi-infinite plasma filled waveguide of Sect. 2.9.4. As we found in the study of electrodynamics of black holes in Chap. 4, the spacetime near the event horizon has no significance for the determination of a g
作者: exquisite    時間: 2025-3-23 18:44
Ergospheric Disk Dynamos,e GHM interaction of flux tubes that thread the equatorial plane of the ergosphere and therefore not the horizon. In this chapter we look at a highly idealized model in which a disk of ergospheric plasma is the dynamo (see Fig. 8.1). This has two simplifying features. Firstly, the equatorial disk ac
作者: 憤慨點吧    時間: 2025-3-23 22:41

作者: 有幫助    時間: 2025-3-24 04:27

作者: PANG    時間: 2025-3-24 10:18

作者: 權宜之計    時間: 2025-3-24 10:48
Book 20011st editioneractions that combine the effects of gravity and a strong magnetic field, in the vicinity (ergosphere) of a rapidly rotating black hole. This topic was created in response to the astrophysical quest to understand the central engines of radio loud extragalactic radio sources. The theory describes a
作者: Compass    時間: 2025-3-24 18:36

作者: inflame    時間: 2025-3-24 23:01
Relativistic Plasma Physics,an induce currents to flow in a wind far from the hole if, and only if, a wave packet carrying the appropriate information requiring the current flow is transmitted from the ergospheric plasma and received by the wind plasma far from the hole. The relativistic structure of plasma waves is the prime emphasis of this chapter.
作者: 侵略者    時間: 2025-3-24 23:11

作者: 斷言    時間: 2025-3-25 05:48

作者: 儀式    時間: 2025-3-25 08:09
Begriff und Geschichte der Forststatikational energy of the hole powers the outgoing wind. The solution emphasizes the crucial role of the Alfvén wave radiation from the dynamo and strong dissipative cross-field currents in the dynamo region.
作者: AORTA    時間: 2025-3-25 13:54

作者: 微生物    時間: 2025-3-25 18:05
Ergospheric Disk Dynamos,ational energy of the hole powers the outgoing wind. The solution emphasizes the crucial role of the Alfvén wave radiation from the dynamo and strong dissipative cross-field currents in the dynamo region.
作者: Omniscient    時間: 2025-3-25 23:19
Winds from Event Horizon Magnetospheres,rmination of the field line angular velocity is far from trivial. Thus, .. can be estimated only by utilizing a deep understanding of the GHM causality of ergospheric dynamos as described in Chap. 7 and elucidated by the example of Chap. 8.
作者: 浮雕寶石    時間: 2025-3-26 03:23

作者: ERUPT    時間: 2025-3-26 05:21

作者: 有說服力    時間: 2025-3-26 09:35
Statik des Durchforstungsbetriebeslobal flow (e.g., the constants of motion in a magnetic flux tube), except that it is a sink for mass influx. Most of this chapter is concerned with the MHD causal structure of black hole GHM. We continue to emphasize the differences between oblique Alfvén waves and fast waves beyond just the wave speeds.
作者: CHYME    時間: 2025-3-26 14:36

作者: forebear    時間: 2025-3-26 20:17
Begriff und Geschichte der Forststatikth a look at evidence for a structure to the central engine in relation to the unified scheme for radio loud AGN that was discussed in the Introduction. The remainder of the chapter shows how these spectral diagnostics of the central engines occur naturally in the black hole GHM theory of extragalactic radio sources.
作者: Conspiracy    時間: 2025-3-26 22:44
Introduction,). Thus, one expects that the interactions of magnetized plasma with the gravitational fields of black holes permeate the Universe and the astrophysical consequences should be spectacular. This monograph is the first text designed to be a formal study of this new branch of physics which is such a fundamental part of our Universe.
作者: 江湖郎中    時間: 2025-3-27 05:08

作者: heterogeneous    時間: 2025-3-27 05:15
Begriff und Geschichte der ForststatikThis is by far the shortest chapter in the book, yet it is the most important as it synthesizes the fundamental physics of all ergospheric dynamos that create and sustain a toroidal magnetic flux (and the currents that support it). The content is not more than a typical section of the book, but is broken off into its own chapter for emphasis.
作者: 珠寶    時間: 2025-3-27 13:03
Ergosphere Driven Winds,This is by far the shortest chapter in the book, yet it is the most important as it synthesizes the fundamental physics of all ergospheric dynamos that create and sustain a toroidal magnetic flux (and the currents that support it). The content is not more than a typical section of the book, but is broken off into its own chapter for emphasis.
作者: Tinea-Capitis    時間: 2025-3-27 16:31

作者: 手段    時間: 2025-3-27 20:10
Rechnungsgr??en und deren Abkürzungen ., as measured from asymptotic infinity. The preparation of . < 0 matter must occur within the ergosphere. This is related to the fact that the outer boundary of the ergosphere, the stationary limit at . = .. occurs when ./. changes from a timelike vector field to a spacelike vector field (see definition of . in (1.36a)).
作者: STRIA    時間: 2025-3-27 23:53
Particle Trajectories in the Ergosphere, ., as measured from asymptotic infinity. The preparation of . < 0 matter must occur within the ergosphere. This is related to the fact that the outer boundary of the ergosphere, the stationary limit at . = .. occurs when ./. changes from a timelike vector field to a spacelike vector field (see definition of . in (1.36a)).
作者: languor    時間: 2025-3-28 06:06

作者: NUDGE    時間: 2025-3-28 07:25

作者: 旋轉一周    時間: 2025-3-28 12:13
Subjektive ?ffentliche Pflichten und Rechteo pulsar winds and extragalactic radio jets. It is now widely accepted that 1.. — 20.. black holes populate the galaxies that fill the Universe. Furthermore, water maser mappings with the VLBA (Very Long Baseline Array) and kinematical gas analyses with HST (The Hubble Space Telescope) make a convin
作者: 后退    時間: 2025-3-28 17:22
Die Elemente der Vorkalkulationontext is essential before delineating the particulars on a black hole background. In a plasma-filled magnetosphere, information can be transmitted from one region to another only by means of the modes of propagation allowed by the plasma state. For example, a plasma distribution in the ergosphere c
作者: superfluous    時間: 2025-3-28 19:46
Rechnungsgr??en und deren Abkürzungen ., as measured from asymptotic infinity. The preparation of . < 0 matter must occur within the ergosphere. This is related to the fact that the outer boundary of the ergosphere, the stationary limit at . = .. occurs when ./. changes from a timelike vector field to a spacelike vector field (see defi
作者: judiciousness    時間: 2025-3-29 00:17

作者: 謙虛的人    時間: 2025-3-29 03:19





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