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標(biāo)題: Titlebook: Accretion Disks and Magnetic Fields in Astrophysics; Proceedings of the E G. Belvedere Conference proceedings 1989 Springer Science+Busines [打印本頁(yè)]

作者: raff淫雨霏霏    時(shí)間: 2025-3-21 19:27
書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics影響因子(影響力)




書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




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書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics被引頻次學(xué)科排名




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書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics讀者反饋




書(shū)目名稱(chēng)Accretion Disks and Magnetic Fields in Astrophysics讀者反饋學(xué)科排名





作者: precede    時(shí)間: 2025-3-21 22:06
The Radiologic Evaluation of Renal Massesield dynamo models. Nonlinear solutions provide examples of chaotic time-dependent behaviour and illustrate the development of complicated spatial structure. However, it is difficult to extrapolate from slow rotators like the Sun to rapidly rotating, highly active stars.
作者: 喃喃訴苦    時(shí)間: 2025-3-22 00:54
S. Trattnig,P. Hübsch,F. Frühwaldain sequence star. These binary systems are very common, well documented by observations in the optical wavelength region since a long time. These objects are therefore particularly well suited to study properties of accretion disks.
作者: AMITY    時(shí)間: 2025-3-22 07:54

作者: 調(diào)整    時(shí)間: 2025-3-22 12:28
https://doi.org/10.1007/978-3-319-17539-3g profile. Our results are compared to standard theoretical and numerical models. We find that the stream of cold gas falling on the compact star forms the disk in the conventional way, a strong shock develops and penetrates deep into the disk. However, since our numerical viscosity is still high we cannot establish if spiral shocks are forming.
作者: 使成核    時(shí)間: 2025-3-22 15:14

作者: 可以任性    時(shí)間: 2025-3-22 17:31

作者: bromide    時(shí)間: 2025-3-22 23:46

作者: Magnificent    時(shí)間: 2025-3-23 03:47
G. Stuart Rutherfoord,R. H. Hewlettby introducing a magnetodynamic picture which is related to the sweeping-magnetic-twist mechanism proposed by Uchida and Shibata (1985) for the production of molecular bipolar flows from forming stars.
作者: 初學(xué)者    時(shí)間: 2025-3-23 08:22
https://doi.org/10.1007/978-3-211-99763-5n especially attractive in protostellar, neutron star and AGN disks, where the traditional ‘a(chǎn)ngular momentum problem’ is most severe. It is shown that spiral shocks are also good locations for producing energetic protons, and I propose that this is the way in which the energetic particles inferred in many AGN’s are produced.
作者: bromide    時(shí)間: 2025-3-23 12:58

作者: 嬰兒    時(shí)間: 2025-3-23 16:48

作者: Mortal    時(shí)間: 2025-3-23 21:31
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/a/image/143795.jpg
作者: 真實(shí)的你    時(shí)間: 2025-3-24 00:49

作者: crescendo    時(shí)間: 2025-3-24 03:26

作者: Constrain    時(shí)間: 2025-3-24 10:13

作者: 束縛    時(shí)間: 2025-3-24 12:37

作者: Mirage    時(shí)間: 2025-3-24 18:16

作者: 問(wèn)到了燒瓶    時(shí)間: 2025-3-24 21:35

作者: habitat    時(shí)間: 2025-3-24 23:37
https://doi.org/10.1007/978-3-211-99763-5tra-galactic radio sources and infra-red bipolar sources. An overview is given of recent theoretical work on magnetohydrodrynamics of accretion disks and on the magnetic mechanism for the formation and collimation of narrow jets.
作者: dura-mater    時(shí)間: 2025-3-25 04:07
Max Nerheim BSEE, MSEE,Andrew F. Hinz B.S.lis- and buoyancy forces on the added mass, and of radiation pressure are considered. The results are applied to a linear stability analysis for a circular fluxtube in the equatorial plane of the disk.
作者: 抵押貸款    時(shí)間: 2025-3-25 10:10

作者: Override    時(shí)間: 2025-3-25 13:05
Principles of Confocal In Vivo Microscopy,present in synchronous systems (“polars”) and could be absent in non-synchronous systems (“intermediate polars”) for orbital periods < 5hr. This result is a consequence of the hypothesis that white dwarf magnetic moments in polars and intermediate polars are . ≈ 10.-10. Gcm.: this hypothesis is stro
作者: lambaste    時(shí)間: 2025-3-25 16:15

作者: 巨頭    時(shí)間: 2025-3-25 20:42
Atlas of Contrast-Enhanced Mammographyin a confused theoretical situation it is useful to evaluate results on the basis of their frequency of recurrence. Some important results are isolated but a comprehensive review is not attempted. The various categories of theory associated with jets from non-relativistically compact objects are sur
作者: 克制    時(shí)間: 2025-3-26 01:27

作者: Lice692    時(shí)間: 2025-3-26 08:11
https://doi.org/10.1007/978-3-319-17539-3le Hydrodynamic interpolation method to solve the fluid dynamic equations. This method seems quite promising for its simplicity and efficient computing profile. Our results are compared to standard theoretical and numerical models. We find that the stream of cold gas falling on the compact star form
作者: Ventilator    時(shí)間: 2025-3-26 11:45

作者: 悄悄移動(dòng)    時(shí)間: 2025-3-26 16:30
Annapoorna Kini,Jagat Narula,Samin Sharmaor the association of such disks with energetic bipolar outflows from these objects. In addition, the projected magnetic field vecotrs around these sources are generally found to be well aligned with the direction of the outflow and the axis of the associated disk, pointing to the possible dynamical
作者: Indelible    時(shí)間: 2025-3-26 17:22

作者: Lyme-disease    時(shí)間: 2025-3-26 23:22

作者: 危險(xiǎn)    時(shí)間: 2025-3-27 01:27
Accretion Disks and Magnetic Fields in Astrophysics978-94-009-2401-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 易發(fā)怒    時(shí)間: 2025-3-27 06:12
0067-0057 Overview: 978-94-010-7581-7978-94-009-2401-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 兩種語(yǔ)言    時(shí)間: 2025-3-27 09:27
https://doi.org/10.1007/978-3-211-99763-5tra-galactic radio sources and infra-red bipolar sources. An overview is given of recent theoretical work on magnetohydrodrynamics of accretion disks and on the magnetic mechanism for the formation and collimation of narrow jets.
作者: cutlery    時(shí)間: 2025-3-27 15:08

作者: engrossed    時(shí)間: 2025-3-27 18:27
G. Stuart Rutherfoord,R. H. Hewlettadicals created by the energy loss of the impinging ions. It is in particular investigated, by means of a Monte Carlo simulation, the relevance of the model of grains adopted. Some preliminary results are given.
作者: GROWL    時(shí)間: 2025-3-27 22:39
Atlas of Color-Coded Doppler SonographyI review the current status of accretion disc theory and its relation to observations.
作者: Feature    時(shí)間: 2025-3-28 02:27

作者: BLAZE    時(shí)間: 2025-3-28 07:24
978-94-010-7581-7Springer Science+Business Media Dordrecht 1989
作者: definition    時(shí)間: 2025-3-28 13:25

作者: 打擊    時(shí)間: 2025-3-28 15:19

作者: narcissism    時(shí)間: 2025-3-28 20:36
Dynamo Processes in Stars,evelops guidelines using small demonstration programs which .This is the missing X Window book. While others have shown what the X Window system has available, this book shows how to convert this potential into working tools to fulfil your visualisation needs. It is of the show-me class of books...T
作者: disparage    時(shí)間: 2025-3-28 23:30
,Nonlinear Rossby-Alfvén Global Waves on the Surface of a Rotating Sphere,vels of abstraction from system level to circuitlevel and technology. Its objective is to guide industrial andacademic engineers and researchers in the selection of methods,technologies and tools and to provide a baseline for furtherdevelopments. Furthermore the book has been written to serve as ate
作者: painkillers    時(shí)間: 2025-3-29 07:06
Instabilities in dwarf nova accretion disks,8. Throughout the following 36 years, microelectronics has advanced in productivity and performance at a pace unmatched in technological history. Minimum feature size F has declined by about a factor of 1/50; die area .. has increased by approximately 170 times; packing efficiency PE, defined as the
作者: 激怒    時(shí)間: 2025-3-29 08:45

作者: 總    時(shí)間: 2025-3-29 12:19
Magnetohydrodynamic Flows in Accretion Disks and Jets,o the deep sub-micron regime, the on-chip interconnect has become the primary bottleneck in signal flow within high complexity, high speed integrated circuits (ICs).The smaller feature size in DSM technology nodes reduces the delay of the active devices, however, the effect on delay due to the passi
作者: 絆住    時(shí)間: 2025-3-29 18:47
Magnetic Fields in the Accretion Disks of Cataclysmic Variables,ng the material, but also in practical and functional implem.This book guides the reader through the design of circuits and wireless IoT devices deployed in applications demanding low power, small size, and high levels of integration. The design of a sub-1V wireless-LAN receiver is detailed along wi
作者: CLAY    時(shí)間: 2025-3-29 20:41
Accretion Discs and Magnetic Cataclysmic Variables,ast one plasma-involved processing step, starting from surface cleaning via coating to etching. In total, the range of the treated substrates covers some orders of magnitude: Trenches and linewidths of commercially available devices have - ready passed the boundary of 100 nm, decorative surface trea
作者: 衣服    時(shí)間: 2025-3-30 01:44

作者: gimmick    時(shí)間: 2025-3-30 08:00

作者: Diskectomy    時(shí)間: 2025-3-30 11:11
Hydromagnetic Flows from Rapidly Rotating Compact Objects and the Formation of Relativistic Jets,ar neutrino puzzle and the question: What happens to the neutrinos on their way from the sun to the earth? 2. The growing evidence that our universe is filled with about 10 times more matter than is visible and the question: What is dark matter made of? 3. The supernovae explosions and the question:
作者: 口音在加重    時(shí)間: 2025-3-30 15:16

作者: 圣歌    時(shí)間: 2025-3-30 18:29

作者: 羞辱    時(shí)間: 2025-3-30 21:26
The Relevance of Magnetic Fields to Stars and Accretion Disks,cal suggestions for all surgeons, perfusionists, scrub-nurses, and anesthesiologists who are engaged in pediatric cardiac surgery. It will also appeal to pediatric cardiologists and medical device manufacturers. The book is intended to share the author’s experience and actual data with readers who h
作者: 使熄滅    時(shí)間: 2025-3-31 04:18
,Nonlinear Rossby-Alfvén Global Waves on the Surface of a Rotating Sphere,om the Foreword:. .`... This global nature of design for low power was well understood byWolfgang Nebel and Jean Mermet when organizing the NATO workshop whichis the origin of the book. They invited the best experts in the fieldto cover all aspects of low power design. As a result the chapters inthis book are978-0-7923-8103-7978-1-4615-5685-5
作者: 追逐    時(shí)間: 2025-3-31 05:28

作者: 不理會(huì)    時(shí)間: 2025-3-31 10:13

作者: 遠(yuǎn)足    時(shí)間: 2025-3-31 15:55
Accretion Discs and Magnetic Cataclysmic Variables,uality of conventional materials can be improved by plasma treatment:Cottonbecomesmorecrease-resistant,leathermoredurable,andthe shrinking of wool ?bers during the washing process can be signi?cantly reduced. To cut a long story short: More than 150 years after the discovery of the sputtering e?ect
作者: Collision    時(shí)間: 2025-3-31 20:07
Radio Emission of Dwarf Novae,e neue Form von Gesellschaft. Da diese Publikation auch die Vorlesung ”Horizontale V- dichtungsformen im Wohnbau”, die ich an der TU Wien abhalte, begleiten soll, sind einige Passagen (z.B. die - schichte des Deutschen Werkbunds) ziemlich genau - halten, w?hrend andere Bereiche (z.B. Bauphysik usw.)
作者: antidepressant    時(shí)間: 2025-3-31 22:15

作者: zonules    時(shí)間: 2025-4-1 03:12
Hydromagnetic Flows from Rapidly Rotating Compact Objects and the Formation of Relativistic Jets,1987 at which the above subjects and their experimental investigation were discussed. The proposed experimental methods are very new. They involve frontier developments in low temperature and solid-state physics. The book should be useful to researchers and students who actively work on these subjec
作者: syring    時(shí)間: 2025-4-1 07:29

作者: Entirety    時(shí)間: 2025-4-1 11:39





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