標(biāo)題: Titlebook: Magnetic Fields of Galaxies; A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloff Book 1988 Kluwer Academic Publishers 1988 Variation.cosmic ray. [打印本頁] 作者: Kennedy 時(shí)間: 2025-3-21 19:05
書目名稱Magnetic Fields of Galaxies影響因子(影響力)
書目名稱Magnetic Fields of Galaxies影響因子(影響力)學(xué)科排名
書目名稱Magnetic Fields of Galaxies網(wǎng)絡(luò)公開度
書目名稱Magnetic Fields of Galaxies網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Magnetic Fields of Galaxies被引頻次
書目名稱Magnetic Fields of Galaxies被引頻次學(xué)科排名
書目名稱Magnetic Fields of Galaxies年度引用
書目名稱Magnetic Fields of Galaxies年度引用學(xué)科排名
書目名稱Magnetic Fields of Galaxies讀者反饋
書目名稱Magnetic Fields of Galaxies讀者反饋學(xué)科排名
作者: stress-test 時(shí)間: 2025-3-21 21:20
Origin of Magnetic Fields,mes of radiogalaxies, in quasars and in other objects. Details of magnetic field configurations and their strengths are not always reliable, but the general result is certainty of the presence in galaxies and galactic-type objects of magnetic fields that cover wide ranges of spatial scales and stren作者: LURE 時(shí)間: 2025-3-22 03:34 作者: tympanometry 時(shí)間: 2025-3-22 08:05 作者: nonradioactive 時(shí)間: 2025-3-22 12:09 作者: 推遲 時(shí)間: 2025-3-22 13:41
Concluding Remarks,gnetic fields at galactic scales. This process of maintenance and generation of the magnetic field is called the hydromagnetic dynamo; the same term is usually applied to the motion itself, which provides the dynamo action. In spiral galaxies, the basic elements of the dynamo are the differential ro作者: 法律的瑕疵 時(shí)間: 2025-3-22 17:57
A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloffbetween a matrix and an embedded wh. Since LF wh movement out of finite complements is blocked in Hindi, an explanation along these lines is obviously not feasible for it. I show that there are two distinct sources for long-distance lists, neither of which require us to compromise locality in scope 作者: 縫紉 時(shí)間: 2025-3-22 23:12
A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloffned to IP is coindexed with a DP in the main clause and that this instantiates an operator-variable relation. In this chapter the semantics associated with this relation is made explicit. Treating the relative clause as a generalized quantifier and the main clause DP as a variable, I show how the tw作者: Presbyopia 時(shí)間: 2025-3-23 04:34 作者: 帶來 時(shí)間: 2025-3-23 06:34 作者: 虛情假意 時(shí)間: 2025-3-23 10:21 作者: IOTA 時(shí)間: 2025-3-23 17:02
Galaxies,collection used by Hubble. The catalogues compiled by G. de Vaucouleurs and van den Bergh included 2599 and 935 samples respectively and the modern assemblages comprise up to 32000 pieces. Figure II.1 shows a few drawings made by Vorontsov-Velyaminov (1978, p. 42) from the photographs of his catalogue.作者: separate 時(shí)間: 2025-3-23 19:57 作者: Meager 時(shí)間: 2025-3-24 00:55
Observation of Magnetic Fields,A direct indicator of magnetic fields in galaxies and other astronomical objects is their synchrotron emission. It is the emission of charged particles moving with relativistic velocities in the magnetic field (see, e.g., Ginzburg and Syrovatskii, 1964; Pacholczyk, 1970; 1977).作者: 悄悄移動(dòng) 時(shí)間: 2025-3-24 04:49
Interpretation of Observational Data,Astrophysics deals with objects remote in space and time. Active experiments are impossible (except for within the solar system), and observational data are usually incomplete. So, there is a vast field of interpretations, stretching between observations and a final picture of a phenomenon. This field often begins with data processing.作者: 大方不好 時(shí)間: 2025-3-24 07:21 作者: 托運(yùn) 時(shí)間: 2025-3-24 11:50
https://doi.org/10.1007/978-94-009-2835-0Variation; cosmic ray; galaxies; galaxy; quasars; star; star formation; stars; turbulence作者: Acclaim 時(shí)間: 2025-3-24 17:43
Concluding Remarks,gradient. The hydromagnetic dynamo is a universal process that also generates magnetic fields in the liquid cores of planets and the convective zones of stars. An advantageous peculiarity of the galactic dynamo is the fact that in galaxies the velocity field can be observed directly. Moreover, in our Galaxy we even reside . a dynamo machine.作者: BRUNT 時(shí)間: 2025-3-24 19:50 作者: 人充滿活力 時(shí)間: 2025-3-25 03:03 作者: Engaged 時(shí)間: 2025-3-25 03:19
The Galactic Dynamo,tic field origin. Second, the characteristic growth time of the field is only an order of magnitude shorter than the galactic lifetime. Therefore, it should be expected that the generation proceeds currently in the linear or in a weakly non-linear regime which inherits typical properties from the linear stage.作者: DEFT 時(shí)間: 2025-3-25 09:53
Problems of Magnetic Field Generation in Galactic Nuclei, Quasars and Radiogalaxies,e but a solution to the problem of their origin is still at its embryonic state. At this stage of development, only very general ideas will be discussed here. We concentrate on the basic question: whether or not the observed or probable motions in these objects can form and maintain magnetic fields?作者: artifice 時(shí)間: 2025-3-25 15:41
Origin of Magnetic Fields,eneral result is certainty of the presence in galaxies and galactic-type objects of magnetic fields that cover wide ranges of spatial scales and strengths. Let us now discuss the basic concepts of the origin of galactic magnetic fields.作者: 幼兒 時(shí)間: 2025-3-25 19:38
Magnetic Fields Around Galactic Discs,) of galaxies and even in the intergalactic gas of galaxy clusters. In this chapter we briefly discuss the information, scarce though it is, about these ‘over-galactic’ magnetic fields and views on their origin.作者: 面包屑 時(shí)間: 2025-3-25 21:08 作者: 間接 時(shí)間: 2025-3-26 01:39 作者: 打折 時(shí)間: 2025-3-26 07:26 作者: 悠然 時(shí)間: 2025-3-26 09:44 作者: debris 時(shí)間: 2025-3-26 14:24 作者: 最有利 時(shí)間: 2025-3-26 18:56
P. Stuckey McIntoshenerally, abnormality detection and data recording are performed manually, which is very prone to cause problems such as false detections, missing detections and recording errors because of lots of freight trains passing through the station simultaneously. In order to tackle these problems, we propo作者: 指耕作 時(shí)間: 2025-3-26 21:26
Maximizing Energy Efficiency for?Charger Scheduling of?WRSNsing and the service quality of network coverage. To guarantee the continuous coverage of the rechargeable sensors, continuous power supply for sensors becomes more important. In this paper, we focus on the Charging Scheduling problem with Maximized Energy Efficiency in WRSNs (CS-MEE Problem), in whi作者: 思考 時(shí)間: 2025-3-27 02:43 作者: 物質(zhì) 時(shí)間: 2025-3-27 08:16 作者: kidney 時(shí)間: 2025-3-27 11:00 作者: 拋媚眼 時(shí)間: 2025-3-27 14:57 作者: MOT 時(shí)間: 2025-3-27 19:27 作者: gonioscopy 時(shí)間: 2025-3-27 22:35 作者: xanthelasma 時(shí)間: 2025-3-28 05:01
Managing side effects on shared data,this paper we describe the data-sharing abstractions of the toolbox, and show how the toolbox may be used to construct efficient parallel programs without exposing the programmer to low-level parallel programming details, which are hidden by the toolbox implementation.作者: delta-waves 時(shí)間: 2025-3-28 08:06 作者: 愚蠢人 時(shí)間: 2025-3-28 10:35
Nancy N. Artus,Chris Somervilleained for structural characterization of solids..In the first group of examples presented, the local structure of amorphous and glassy materials is analyzed. It is shown that the coordination number and polymerization degree depend on the composition and relative distribution of ions. In the second 作者: lesion 時(shí)間: 2025-3-28 17:31 作者: Endoscope 時(shí)間: 2025-3-28 19:52
Ben Morganon to such psychological characteristics and tolerance of ambiguity and risk taking) influences the nature and probability of entrepreneurial success. Moreover, they explore the role of social media and social 978-3-319-37650-9978-3-319-05567-1Series ISSN 2197-5698 Series E-ISSN 2197-5701 作者: ingenue 時(shí)間: 2025-3-29 01:36 作者: 歡呼 時(shí)間: 2025-3-29 05:10 作者: 鋼筆尖 時(shí)間: 2025-3-29 09:50
