標(biāo)題: Titlebook: Magnetohydrodynamics in Binary Stars; C. G. Campbell Book 2018Latest edition Springer Nature Switzerland AG 2018 AM Herculis stars.Accreti [打印本頁] 作者: Interjection 時間: 2025-3-21 16:39
書目名稱Magnetohydrodynamics in Binary Stars影響因子(影響力)
書目名稱Magnetohydrodynamics in Binary Stars影響因子(影響力)學(xué)科排名
書目名稱Magnetohydrodynamics in Binary Stars網(wǎng)絡(luò)公開度
書目名稱Magnetohydrodynamics in Binary Stars網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Magnetohydrodynamics in Binary Stars被引頻次
書目名稱Magnetohydrodynamics in Binary Stars被引頻次學(xué)科排名
書目名稱Magnetohydrodynamics in Binary Stars年度引用
書目名稱Magnetohydrodynamics in Binary Stars年度引用學(xué)科排名
書目名稱Magnetohydrodynamics in Binary Stars讀者反饋
書目名稱Magnetohydrodynamics in Binary Stars讀者反饋學(xué)科排名
作者: contrast-medium 時間: 2025-3-21 23:12
Disrupted Discs: Stellar Spin Evolution,The torques exerted on the magnetic primary star due to its interaction with the accretion disc and curtain flow are considered.作者: constitute 時間: 2025-3-22 01:52
https://doi.org/10.1007/978-3-319-97646-4AM Herculis stars; Accretion discs in binary star systems; Accretion torque; Curtain flow; Disrupted acc作者: 憤慨點(diǎn)吧 時間: 2025-3-22 06:28
978-3-030-07382-4Springer Nature Switzerland AG 2018作者: 結(jié)構(gòu) 時間: 2025-3-22 09:32 作者: Conducive 時間: 2025-3-22 16:03
C. G. CampbellPresents a thoroughly revised edition of a well-cited text which centers on magnetohydrodynamics problems associated with accretion processes in binary star systems.Adds new work on magnetic coupling 作者: Inelasticity 時間: 2025-3-22 20:58 作者: arrogant 時間: 2025-3-23 00:28 作者: bioavailability 時間: 2025-3-23 02:58
C. G. Campbelll data are needed to better understand the magnitude and direction of environmental change related to both natural and anthropogenic causes, as well as to assess patterns of natural variability. The paucity of instrumental data requires that proxy methods be used. The abundance of lakes throughout t作者: 連接 時間: 2025-3-23 06:17
C. G. Campbellof group-specific oligonucleotides to RNA extracted from lakewater. Nonmetric, multidimensional scaling (MDS) analysis of relative bacterial phylotype densities revealed complex relationships among assemblages sampled from depth profiles in July, August and September of 1997 through 1999. CL500-11 g作者: Urologist 時間: 2025-3-23 13:40 作者: Bricklayer 時間: 2025-3-23 15:30 作者: 松緊帶 時間: 2025-3-23 20:14
C. G. Campbellllion Euro belong to the group of family firms (Klein, 2000). In the US, 20% of Fortune 500 firms have a family as the largest holder of voting rights (Villalonga and Amit, 2006). Family firms and their role in the economy have been widely debated in the academic literature. In his seminal works . a作者: stratum-corneum 時間: 2025-3-24 00:46
C. G. Campbello because they are commonly assumed to be more long-term oriented than comparable non-family firms. This view, however, is largely based on - amples and case studies, while large-scale quantitative studies are so far missing. In more detail, we have very limited knowledge about how family and non-fa作者: 艦旗 時間: 2025-3-24 05:30
C. G. Campbell4 until December 2007 the ComCoast project (Combined Fu- tions in Coastal Defence Zones) was carried out within the Interreg IIIB framework. The objective of this project was to investigate and to test the options for spatial coastal protection concepts. The mission statement of the project over its作者: 異常 時間: 2025-3-24 09:48 作者: 抱狗不敢前 時間: 2025-3-24 13:30 作者: 破布 時間: 2025-3-24 17:41 作者: extemporaneous 時間: 2025-3-24 19:05 作者: 白楊 時間: 2025-3-24 23:19
C. G. Campbellearning in elementary school) Experienced junior high school students in Grades 7 and 8 in School A and 73 Non-experienced students from School B. After removing five participants for missing data, 69 ELES Experienced and 71 Non-experienced participants were retained (see Table 3.1). For School A, b作者: Resign 時間: 2025-3-25 07:11
C. G. Campbell system. It attempts to identify those domains most sensitive to early English instruction by employing a state-of-the-art quantitative research methodology. English education was formally introduced in Japan for fifth and sixth graders in 2011 and is still in its infancy as a program. This study co作者: paroxysm 時間: 2025-3-25 11:30 作者: formula 時間: 2025-3-25 14:14 作者: essential-fats 時間: 2025-3-25 16:17
Theoretical Prerequisites,e then combined with the equations of hydrodynamics to derive the equations of MHD, with viscosity and the associated energy transport equations included. The main types of magnetic wave solutions are derived, and their relevance to different types of flows is considered. Mathematical representation作者: 在駕駛 時間: 2025-3-25 22:11 作者: 流出 時間: 2025-3-26 02:08 作者: 小步舞 時間: 2025-3-26 06:23
AM Her Stars: The Maintenance of Synchronism,que present to balance the accretion torque. In general, a 3D torque is required and the balance must be stable. Because the secondary star has at least a convective envelope, and is rapidly rotating due to tidal synchronization, it is likely to have a large-scale magnetic field generated by dynamo 作者: Left-Atrium 時間: 2025-3-26 09:57
AM Her Stars: The Attainment of Synchronism,s state is a magnetic orientation corresponding to a minimum in a potential energy well. As corotation is approached from an over-synchronous state, the primary must be able to lose its remaining synodic rotational energy plus the energy gained via the accretion torque over a synodic period to preve作者: Headstrong 時間: 2025-3-26 16:43 作者: 值得贊賞 時間: 2025-3-26 17:39 作者: exquisite 時間: 2025-3-26 23:05
Intrinsic Magnetism in Accretion Discs,ndard mean-field dynamos are considered, which can generate large-scale magnetic fields in discs. Toroidal magnetic field is generated by the shearing of the radial field, while turbulence with Coriolis force and vertical stratification lead to the .-effect which converts toroidal field to poloidal 作者: 相信 時間: 2025-3-27 01:11 作者: Nomadic 時間: 2025-3-27 07:03
Stellar Magnetic Winds,es the generation of large-scale magnetic fields in such stars very likely, and magnetically influenced wind flows from the stellar surface would then lead to magnetic braking. The secondary would be spun down to an under-synchronous state and tides would then operate to spin the star up at the expe作者: 協(xié)定 時間: 2025-3-27 10:10
Accretion Disc Magnetic Winds, become collimated parallel to the disc rotation axis. It is known that a differentially rotating, turbulent disc can have a large-scale magnetic field generated by dynamo action. Magnetically channelled winds are effective at removing angular momentum from accretion discs, provided that the initial作者: 作繭自縛 時間: 2025-3-27 17:10
Book 2018Latest edition major revision of the first edition. The material has been updated and extended, including additional chapters on the origins of the stellar magnetic fields and accretion disc magnetic winds. A comprehensive account is given of the subject, from the early work up to the latest results. The unifying作者: floaters 時間: 2025-3-27 18:16
0067-0057 s in binary star systems.Adds new work on magnetic coupling .Magnetism in binary stars is an area of central importance in stellar astrophysics. The second edition of "Magnetohydrodynamics in Binary Stars" is a major revision of the first edition. The material has been updated and extended, includin作者: Minikin 時間: 2025-3-27 23:33
AM Her Stars: Stream Channelling and the Accretion Torque,cretion torques are considered here, as well as the effects of partial field channelling. For a dipolar magnetic field and moderate degrees of asynchronism, the normal components of the accretion torque average to zero over a synodic rotation period, while the parallel component has a conservative averaged form for total field channelling.作者: fructose 時間: 2025-3-28 03:38
Disc Disruption and Accretion Curtains, vertical expansion due to magnetic heating. Expanding material can be accelerated through a sonic point and then flow through a magnetically channelled curtain region to accrete on to the star through a narrow shock region. A detailed study of disc disruption and the curtain flow is presented here.作者: Pepsin 時間: 2025-3-28 10:02
Stellar Magnetic Winds,ere, with particular emphasis on the fast rotator regime. This is applied to derive mass transfer rates in binaries with periods ??3.0 h, for a range of laws relating the secondary’s surface magnetic field to its rotation rate. Explanations for the period gap, and why AM Herculis binaries appear not to be affected by the gap, are discussed.作者: noxious 時間: 2025-3-28 13:38
Magnetism in Binary Stars,scs..Sub-thermal magnetic fields lead to a magnetorotational instability in accretion discs which is believed to be the source of the turbulent viscosity needed to account for the inflow. Disc dynamos can generate large-scale magnetic fields which can lead to radial transport of angular momentum, or作者: Flatus 時間: 2025-3-28 17:48
Theoretical Prerequisites,gravitational radiation and magnetic braking are described. The steady viscous accretion disc model is presented, and the fundamental time-scales in discs are derived. The essentials of spin dynamics are given, in relation to the response of compact stellar components to torques and in the analysis 作者: RAGE 時間: 2025-3-28 22:14
AM Herculis Stars,ure of the required balancing torque. Certain conditions are necessary for the attainment of synchronism. Asynchronous rotation of the primary can significantly affect the mass transfer rate, due to magnetic spin-orbit coupling. The essential properties of the AM Her binaries are described here, tog作者: PAC 時間: 2025-3-28 23:47 作者: Congestion 時間: 2025-3-29 05:42
AM Her Stars: The Attainment of Synchronism,hen results, with a variation of the angular velocity due to the periodic imbalance of the torques. A stronger surface magnetic field on the primary favours the attainment of synchronism by raising the value of ... These restrictions do not occur for an under-synchronous primary.作者: 嫻熟 時間: 2025-3-29 10:57 作者: Traumatic-Grief 時間: 2025-3-29 13:11
Intrinsic Magnetism in Accretion Discs,retion disc model is then presented, with a large-scale, dynamo generated magnetic field of quadrupolar symmetry, including the determination of the radial and vertical disc structures. Turbulence plays a dual role of contributing to the .-effect in the dynamo and in partly driving the disc inflow v作者: NADIR 時間: 2025-3-29 17:31 作者: 不法行為 時間: 2025-3-29 19:56 作者: Lament 時間: 2025-3-30 02:48
Book 2018Latest edition on binary stars, much of the work on accretion discs and wind flows has more general astrophysical relevance. Convenient formulae are included that can be compared to observations, making the book useful to observers as well as theorists, and there are extensive reference lists. The material is mai作者: 逢迎春日 時間: 2025-3-30 04:22 作者: 無思維能力 時間: 2025-3-30 10:58
C. G. Campbellirms that draws on several data sources, the author then tests his - potheses using leading-edge empirical methods. Noteworthy, he not only proceeds by classica978-3-8349-1959-5978-3-8349-8412-8Series ISSN 2627-1168 Series E-ISSN 2627-1184 作者: 贊成你 時間: 2025-3-30 15:11
C. G. Campbellcontinuously demonstrated his ability to bring me back to earth. Additionally, I would like to thank my colleague Dr. Thomas Klenke, who gave me the chance to be part of a challenging European project consortium and who supported me with his expertise on the project and the disserta978-3-642-42631-5978-3-642-01774-2作者: Dissonance 時間: 2025-3-30 17:02
