標(biāo)題: Titlebook: Cosmic Magnetic Fields; Richard Wielebinski,Rainer Beck Book 2005 Springer-Verlag Berlin Heidelberg 2005 astrophysics.cosmic magnetic fiel [打印本頁(yè)] 作者: Agitated 時(shí)間: 2025-3-21 17:12
書(shū)目名稱Cosmic Magnetic Fields影響因子(影響力)
書(shū)目名稱Cosmic Magnetic Fields影響因子(影響力)學(xué)科排名
書(shū)目名稱Cosmic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Cosmic Magnetic Fields網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Cosmic Magnetic Fields被引頻次
書(shū)目名稱Cosmic Magnetic Fields被引頻次學(xué)科排名
書(shū)目名稱Cosmic Magnetic Fields年度引用
書(shū)目名稱Cosmic Magnetic Fields年度引用學(xué)科排名
書(shū)目名稱Cosmic Magnetic Fields讀者反饋
書(shū)目名稱Cosmic Magnetic Fields讀者反饋學(xué)科排名
作者: GEST 時(shí)間: 2025-3-21 20:27
978-3-642-42130-3Springer-Verlag Berlin Heidelberg 2005作者: Overstate 時(shí)間: 2025-3-22 03:23 作者: agonist 時(shí)間: 2025-3-22 08:14 作者: Override 時(shí)間: 2025-3-22 09:44 作者: affluent 時(shí)間: 2025-3-22 13:08
Structuralism and Postmodernism the Sun either as optical streamers during solar eclipses and by using remote sensing methods. Magnetic fields of the solar planets have been studied in situ by measurements made by magnetometers on various spacecraft. Stars, supernova remnants and pulsars have been shown to harbour magnetic fields作者: affluent 時(shí)間: 2025-3-22 19:02 作者: Wallow 時(shí)間: 2025-3-23 01:14
Structuralism and Postmodernisms supernovae and stellar winds. This energy stimulates turbulence in the H., which cascades up the turbulent wavenumber spectrum. The spectral wavelengths extend all the way down to scales most easily quoted in Astronomical Units. H. and molecular clouds enjoy a synergistic relationship, with turbul作者: 軍械庫(kù) 時(shí)間: 2025-3-23 04:20
The Foundations of Postmodernismpre-main sequence and on late- and early-type main sequence stars, with some discussion also of red giants and white dwarfs, and with a brief reference to neutron stars. The current observational situation is reviewed, and some of the consequences for our ideas on star formation, on stellar structur作者: 慢跑鞋 時(shí)間: 2025-3-23 09:16 作者: 壓倒 時(shí)間: 2025-3-23 11:12 作者: 哀悼 時(shí)間: 2025-3-23 17:11
Importance of Magnetic Helicity in Dynamos,nal algebraic alpha quenching. The seriousness of this dynamical alpha quenching is particularly evident in the case of closed or periodic boxes. The explicit connection with catastrophic alpha quenching is reviewed and the alleviating effects of magnetic and current helicity fluxes are discussed.作者: 小淡水魚(yú) 時(shí)間: 2025-3-23 19:57
Richard Wielebinski,Rainer BeckIncludes supplementary material: 作者: 傳染 時(shí)間: 2025-3-23 22:45 作者: Congruous 時(shí)間: 2025-3-24 06:15
Cosmic Magnetic Fields978-3-540-31396-0Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 莊嚴(yán) 時(shí)間: 2025-3-24 07:56 作者: 淡紫色花 時(shí)間: 2025-3-24 10:43
Book 2005lanced account of both theoretical and observational aspects. Written as a set of advanced lectures and tutorial reviews that lead up to the forefront of research, this book?offers?both a modern source of reference for the experienced researchers as well as a high-level introductory text for postgra作者: Maximizer 時(shí)間: 2025-3-24 17:15
Magnetic Fields in the Milky Way, Derived from Radio Continuum Observations and Faraday Rotation St. Also the diffuse Milky Way has been shown to possess magnetic fields by many methods. Possibly the whole Universe is intimately governed by the presence of magnetic fields. This review will summarize the observational results and discuss some of the implications of the presence of magnetic fields in the Milky Way.作者: 含糊 時(shí)間: 2025-3-24 21:46 作者: 過(guò)剩 時(shí)間: 2025-3-25 02:59 作者: Constituent 時(shí)間: 2025-3-25 04:09 作者: 輕快來(lái)事 時(shí)間: 2025-3-25 08:02 作者: 粗俗人 時(shí)間: 2025-3-25 14:12
Numerical Magnetohydrodynamics in Astrophysics,es have been achieved in the field of flux tube dynamics, magnetic turbulence in accretion and galactic disks, magnetic Herbig--Haro flows from young stellar objects and the evolution of primordial magnetic fields in galaxy clusters.作者: 使苦惱 時(shí)間: 2025-3-25 18:20 作者: 抒情短詩(shī) 時(shí)間: 2025-3-25 21:19
Postmodernism in Business Studiestic dynamos, had to await the formation of the first non-linear structures. The history of star formation is controlled, at least in part, by how and when galaxies and their precursors acquired their fields. The build-up of magnetic fields is an important aspect of the overall cosmogonic process.作者: Carcinoma 時(shí)間: 2025-3-26 04:07 作者: 改革運(yùn)動(dòng) 時(shí)間: 2025-3-26 04:56 作者: 遍及 時(shí)間: 2025-3-26 12:05
Stellar Magnetic Fields,e to neutron stars. The current observational situation is reviewed, and some of the consequences for our ideas on star formation, on stellar structure and evolution and on stellar rotation are summarized.作者: 摘要記錄 時(shí)間: 2025-3-26 13:35
Book 2005 of research, this book?offers?both a modern source of reference for the experienced researchers as well as a high-level introductory text for postgraduate students and nonspecialist researchers working in related areas.作者: 具體 時(shí)間: 2025-3-26 19:59
0075-8450 orial reviews that lead up to the forefront of research, this book?offers?both a modern source of reference for the experienced researchers as well as a high-level introductory text for postgraduate students and nonspecialist researchers working in related areas.978-3-642-42130-3978-3-540-31396-0Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: ARY 時(shí)間: 2025-3-26 21:29 作者: 宣誓書(shū) 時(shí)間: 2025-3-27 01:36
Structuralism and Postmodernisment energy, angular momentum, magnetic fields, and matter flowing across the boundaries in both directions. The molecular clouds form stars, which in turn act as energy sources to round the circle and make star formation a feedback process.作者: legislate 時(shí)間: 2025-3-27 08:51 作者: G-spot 時(shí)間: 2025-3-27 11:03
Mesoscale Magnetic Structures in Spiral Galaxies,ed and maintained more recently in a relatively mature galaxy. In what follows, we briefly review the current understanding of the origin of the mesoscale magnetic structures and their implications for the origin of galactic magnetic fields.作者: Exposure 時(shí)間: 2025-3-27 16:30 作者: AV-node 時(shí)間: 2025-3-27 21:17
Magnetic Fields in Galaxies,gravitation. They affect the gas flows in spiral arms (Gómez and Cox, 2002). The effective sound speed of the gas is increased by the presence of strong fields which reduce the shock strength. The interstellar fields are closely connected to gas clouds. They affect the dynamics of the gas clouds (El作者: 大炮 時(shí)間: 2025-3-27 22:43 作者: Lacunar-Stroke 時(shí)間: 2025-3-28 03:56
Magnetic Fields in the Milky Way, Derived from Radio Continuum Observations and Faraday Rotation St the Sun either as optical streamers during solar eclipses and by using remote sensing methods. Magnetic fields of the solar planets have been studied in situ by measurements made by magnetometers on various spacecraft. Stars, supernova remnants and pulsars have been shown to harbour magnetic fields作者: cinder 時(shí)間: 2025-3-28 08:32 作者: 爭(zhēng)吵加 時(shí)間: 2025-3-28 13:02
Magnetic Fields in Diffuse H, and Molecular Clouds,s supernovae and stellar winds. This energy stimulates turbulence in the H., which cascades up the turbulent wavenumber spectrum. The spectral wavelengths extend all the way down to scales most easily quoted in Astronomical Units. H. and molecular clouds enjoy a synergistic relationship, with turbul作者: Arteriography 時(shí)間: 2025-3-28 16:24
Stellar Magnetic Fields,pre-main sequence and on late- and early-type main sequence stars, with some discussion also of red giants and white dwarfs, and with a brief reference to neutron stars. The current observational situation is reviewed, and some of the consequences for our ideas on star formation, on stellar structur作者: miscreant 時(shí)間: 2025-3-28 19:44 作者: 極小 時(shí)間: 2025-3-29 01:41
Numerical Magnetohydrodynamics in Astrophysics,rithms and computational methods have been developed for simulating the time-evolution of magnetic field configurations in the astrophysical environment. The most recent trends go in the direction of fully conservative schemes and adaptive mesh refinement for large-scale supercomputing. The most pop作者: 咆哮 時(shí)間: 2025-3-29 03:28
The Foundations of Postmodernismstars (Mestel, 1990). . distributes energy from supernova explosions within the ISM (Subramanian, 1998) and regenerates the field via . (Wielebinski, R., Krause, 1993, Beck et al., 1996; Sect. 6). . is a possible heating source for the ISM and halo gas (Birk et al., 1998). Magnetic fields also contr作者: Incumbent 時(shí)間: 2025-3-29 09:51
Magnetic Fields in Galaxies,stars (Mestel, 1990). . distributes energy from supernova explosions within the ISM (Subramanian, 1998) and regenerates the field via . (Wielebinski, R., Krause, 1993, Beck et al., 1996; Sect. 6). . is a possible heating source for the ISM and halo gas (Birk et al., 1998). Magnetic fields also contr作者: maverick 時(shí)間: 2025-3-29 14:54
Magnetic Fields in Galaxy Systems, Clusters and Beyond,
