標(biāo)題: Titlebook: Accretion Flows in Astrophysics; Nikolay Shakura Book 2018 Springer International Publishing AG, part of Springer Nature 2018 Models of ac [打印本頁] 作者: 交叉路口 時間: 2025-3-21 17:49
書目名稱Accretion Flows in Astrophysics影響因子(影響力)
書目名稱Accretion Flows in Astrophysics影響因子(影響力)學(xué)科排名
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書目名稱Accretion Flows in Astrophysics網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Accretion Flows in Astrophysics被引頻次
書目名稱Accretion Flows in Astrophysics被引頻次學(xué)科排名
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書目名稱Accretion Flows in Astrophysics年度引用學(xué)科排名
書目名稱Accretion Flows in Astrophysics讀者反饋
書目名稱Accretion Flows in Astrophysics讀者反饋學(xué)科排名
作者: 拋物線 時間: 2025-3-21 23:51 作者: enormous 時間: 2025-3-22 03:58
Relativistic Twisted Accretion Disc,uter-aided design (CAD) tools to manage the designcomplexity in the available design time, that is ever decreasing dueto tightening time-to-market constraints. The purpose of .Low-PowerDesign Techniques. .and CAD Tools for Analog and RF IntegratedCircuits. is to provide an overview of very recent re作者: AV-node 時間: 2025-3-22 07:44 作者: debble 時間: 2025-3-22 08:44
Transient Dynamics of Perturbations in Astrophysical Discs,it us to understand the mechanisms that control the performance, particularly the power dissipation, of a logic circuit. Several CMOS design styles, such as pseudo-NMOS, dynamic logic and NORA, are presented. Other circuit variations of the static complementary CMOS, which are suitable for low-power作者: depreciate 時間: 2025-3-22 15:32 作者: 好忠告人 時間: 2025-3-22 18:17
On the Properties of Velikhov-Chandrasekhar MRI in Ideal and Non-ideal Plasmas,tate-of-the-art, vision-enabled WSN nodes.Includes details o.This book presents a comprehensive, systematic approach to the development of vision system architectures that employ sensory-processing concurrency and parallel processing to meet the autonomy challenges posed by a variety of safety and s作者: ZEST 時間: 2025-3-22 21:47 作者: Airtight 時間: 2025-3-23 02:40
Nikolay ShakuraThe book gives a systematic description of the standard model of disc accretion and also covers some topics beyond the standard model.Discusses stationary and non-stationary, Newtonian and general-rel作者: 出血 時間: 2025-3-23 06:03 作者: 圣人 時間: 2025-3-23 12:00 作者: synovial-joint 時間: 2025-3-23 17:09
978-3-030-06567-6Springer International Publishing AG, part of Springer Nature 2018作者: Neutral-Spine 時間: 2025-3-23 22:03 作者: 閑逛 時間: 2025-3-23 23:50
Theoretical Aspects of Cryosurgeryn, thereby unraveling the physics of distant objects. This is possible due to the presence of viscosity, driven by turbulent motions in accretion discs. In this chapter, we describe the equations for disc accretion in the framework of the standard model. We outline basic elements of the theory of tu作者: APO 時間: 2025-3-24 03:27
Theoretical Aspects of Cryosurgerys. The study of this motion is necessary for understanding the inner structure of the disc tilted to the equatorial plane of the rotating black hole. Moreover, this chapter uses a special approach to find out how the values that are measured in a local Lorentz frame of observers falling freely in an作者: 擦試不掉 時間: 2025-3-24 10:21 作者: minion 時間: 2025-3-24 14:18 作者: impale 時間: 2025-3-24 15:23 作者: 使乳化 時間: 2025-3-24 20:31
Nikolai N. Korpan,Jaroslav V. Zharkovisc interiors may be effectively viscous in spite of the absence of magnetorotational instability. In this case, a rotational homogeneous inviscid flow with a Keplerian angular velocity profile is spectrally stable, making the transient growth of perturbations a candidate mechanism for energy transf作者: novelty 時間: 2025-3-25 01:20 作者: patriot 時間: 2025-3-25 06:35
https://doi.org/10.1007/978-3-030-45964-2KB analysis of hydromagnetic axially symmetric flows shows that in the Rayleigh-unstable hydrodynamic case where the angular momentum decreases with radius, the MRI branch becomes stable, and the magnetic field suppresses the Rayleigh instability at small wavelengths. We investigate the limiting tra作者: 積極詞匯 時間: 2025-3-25 08:44
On the Properties of Velikhov-Chandrasekhar MRI in Ideal and Non-ideal Plasmas,led WSN nodes; Includes details of specifications and challenges of vision-enabled WSNs; Explains architectures for low-energy CMOS vision chips with embedded, programmable spatial filtering capabilities; Includes considerations pertaining to the integration of vision chips into off-the-shelf WSN platforms.978-1-4899-9540-7978-1-4614-2392-8作者: 泥土謙卑 時間: 2025-3-25 15:28 作者: 絕緣 時間: 2025-3-25 18:19 作者: 我不重要 時間: 2025-3-25 20:59
Pancreas Cryosurgery. An Animal Experimentd estimation of the neutron star magnetic field. In equilibrium pulsars with independently measured magnetic fields, the model enables the stellar wind velocity to be independently estimated. For non-equilibrium pulsars, there exists a maximum spin-down rate of the accreting neutron star. The model 作者: ADORN 時間: 2025-3-26 04:12 作者: 首創(chuàng)精神 時間: 2025-3-26 04:36
The Standard Model of Disc Accretion,measurement of the CO.-dependent thermal time constant of the transducer. The readout circuit periodically heats up the transducer and uses a phase-domain delta-sigma modulator to digitize the CO.-dependent phase shift of the resulting temperature transients. Compared to the ratiometric steady-state作者: 爵士樂 時間: 2025-3-26 11:19
Relativistic Standard Accretion Disc,ad-spectrum nature of the signal. This is crucial to low-power design: minimizing converter resolution is tantamount to minimizing its power consumption, and every consideration is made at the system level to keep the required number of bits down to the absolute lowest possible value.作者: 有惡意 時間: 2025-3-26 15:08
Relativistic Twisted Accretion Disc,scillators, filters, butalso complete transceiver front-ends, are discussed and analyzed in amethodological way, and their modeling and simulation, both at thecircuit level and at the architectural level, are treated. In thisway, the eleven contributions of this book combine in a unique waydesigns with method978-1-4757-8396-4978-0-306-48089-8作者: Melanocytes 時間: 2025-3-26 17:56 作者: 感情脆弱 時間: 2025-3-27 01:01
Quasi-Spherical Subsonic Accretion onto Magnetized Neutron Stars,n implementation..The book is a self-contained low-power, high-level synthesis text for Nanoscale VLSI design engineers and researchers. Each chapter has simple relevant examples for a better grasp of the principles presented. Several algorithms are given to provide a better understanding of the und作者: Scintillations 時間: 2025-3-27 02:45 作者: 線 時間: 2025-3-27 09:03
0067-0057 important aspects of turbulent viscosity generation. The book is aimed at specialists as well as graduate students interested in the field of theoretical astrophysics..978-3-030-06567-6978-3-319-93009-1Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 隨意 時間: 2025-3-27 12:03 作者: 后天習(xí)得 時間: 2025-3-27 14:43
Book 2018everal chapters cover the underlying physics of viscosity in astrophysical discs with some important aspects of turbulent viscosity generation. The book is aimed at specialists as well as graduate students interested in the field of theoretical astrophysics..作者: Alienated 時間: 2025-3-27 20:55
Nikolai N. Korpan,Jaroslav V. Zharkovg into account Einstein’s relativistic precession. At the end of the chapter, a calculation of the shape of a stationary relativistic twisted accretion disc for different values of free parameters of the model is done.作者: 形容詞 時間: 2025-3-28 01:00 作者: 無聊的人 時間: 2025-3-28 04:10
Theoretical Aspects of Cryosurgerycal values in general relativity. These basic principles, which are systematically presented in the next chapter, are required for a more comprehensive understanding the structure of relativistic tilted accretion discs.作者: libertine 時間: 2025-3-28 07:40
Liver Cryosurgery. An Animal Experiment allows the position of the inner disc radius and hence the black hole spin to be inferred from observations. In addition, the standard accretion disc is the basis for more complicated theories of warped (twisted) accretion discs, which are formed when the accreting matter moves outside the equatorial plane of a rotating black hole.作者: 船員 時間: 2025-3-28 13:40 作者: 六邊形 時間: 2025-3-28 14:36
https://doi.org/10.1007/978-3-030-45964-2 MRI mode completely disappears without the magnetic field. The effects of viscosity and magnetic diffusivity in the plasma on the MRI conditions in thin accretion discs are studied. We find the limits on the mean free-path of ions allowing MRI to operate in such discs.作者: atrophy 時間: 2025-3-28 18:49 作者: WAX 時間: 2025-3-29 00:55
10樓作者: 吸引人的花招 時間: 2025-3-29 03:42
10樓作者: Mast-Cell 時間: 2025-3-29 08:14
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