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標(biāo)題: Titlebook: Life Below Water; Walter Leal Filho,Anabela Marisa Azul,Tony Wall Living reference work 20200th edition Sustainability.Sustainable aquacu [打印本頁]

作者: audiogram    時間: 2025-3-21 16:43
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作者: Tortuous    時間: 2025-3-21 21:10
Living reference work 20200th editionns, especially but not only in developing countries, intensify. Therefore, there is an increasing need to search for integrated solutions to make development more sustainable.?The United Nations has acknowledged the problem?and approved the “2030 Agenda for Sustainable Development”. On 1st January 2
作者: 重力    時間: 2025-3-22 01:54
Living reference work 20200th editionserve and sustainably use the oceans, seas and marine resources for sustainable development.". Marine and coastal bio-resources, play an essential role in human well-being and social and economic development. This volume addresses this sustainability challenge providing the description of a range of
作者: ALT    時間: 2025-3-22 04:47

作者: reserve    時間: 2025-3-22 09:49
Artisanal Fisheries: Management and Sustainability,
作者: 威脅你    時間: 2025-3-22 16:11
Artisanal Fishing Gears and Sustainable Development,
作者: Classify    時間: 2025-3-22 18:24
Ecological and Economic Importance of Benthic Communities,
作者: 砍伐    時間: 2025-3-22 23:55

作者: 消音器    時間: 2025-3-23 02:52
Role of Microphytobenthos in the Functioning of Estuarine and Coastal Ecosystems,
作者: dermatomyositis    時間: 2025-3-23 07:07

作者: Nibble    時間: 2025-3-23 12:13

作者: Motilin    時間: 2025-3-23 15:58

作者: Gustatory    時間: 2025-3-23 18:33
Harmful Algal Blooms: Effect on Coastal Marine Ecosystems,
作者: 從屬    時間: 2025-3-23 22:35

作者: Encephalitis    時間: 2025-3-24 05:39

作者: aerobic    時間: 2025-3-24 07:04
Mariana Palma,Ivan Viegasole of MHD processes in Standard Accretion Discs, and the physics of steady state MHD outflows, from the basic concepts and equations to modern self-similar solutions. Further lectures detail the various classes of steady magnetic-wind models currently discussed in the context of protostellar jets..
作者: trigger    時間: 2025-3-24 12:30
Filipe Martinhoole of MHD processes in Standard Accretion Discs, and the physics of steady state MHD outflows, from the basic concepts and equations to modern self-similar solutions. Further lectures detail the various classes of steady magnetic-wind models currently discussed in the context of protostellar jets..
作者: Sad570    時間: 2025-3-24 16:27
Daniel Crespo,Miguel ?ngelo Pardalver that brown dwarfs can drive outflows. In this review of spectro-astrometry, we shall discuss the technique beginning with a revision of angular resolution and astrometry. The limitations of the technique are described, and the uses to which it has been put to date are extensively discussed.
作者: defeatist    時間: 2025-3-24 20:58

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作者: 抵消    時間: 2025-3-25 06:51

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作者: 個阿姨勾引你    時間: 2025-3-25 15:57

作者: audiologist    時間: 2025-3-25 22:50
Trilok Kumar Jain,Nirupa Jainaturally formed in the rapidly rotating magnetospheres of geometrically thin accretion disks around rotating black holes. Disk fields generated by dynamo effects in the boundary layer between disk and rotating hole immerse the hole in a rotating magnetosphere which is loaded by plasma from the disk.
作者: 引水渠    時間: 2025-3-26 02:57

作者: 擁擠前    時間: 2025-3-26 04:24
Heitor Oliveira Braga,Joelson Musiello-Fernandesions and key questions for jet physics: ? Higher resolution 3D simulations, including large-eddy or direct simulations. ? Three dimensional studies of jet disruption and the transition to turbulence in jets: Norman, Burns and Sulkanen (1988) have shown that the passage of a 2D jet through a shock ca
作者: 慷慨援助    時間: 2025-3-26 08:37

作者: Stable-Angina    時間: 2025-3-26 15:53

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作者: DAMN    時間: 2025-3-26 23:34
Rogélia Martins,Miguel Carneiroon of the four-year JETSET (Jet Simulations, Experiments and Theory) Marie Curie Research Training Network is to build an int- disciplinary European research community focused on the study of jets from yo978-3-642-08768-4978-3-540-68032-1Series ISSN 0075-8450 Series E-ISSN 1616-6361
作者: Budget    時間: 2025-3-27 02:22
2523-7403 t.". Marine and coastal bio-resources, play an essential role in human well-being and social and economic development. This volume addresses this sustainability challenge providing the description of a range of978-3-319-71064-8
作者: 以煙熏消毒    時間: 2025-3-27 07:00

作者: 不自然    時間: 2025-3-27 10:43

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作者: 鬼魂    時間: 2025-3-27 20:56
José C. Xavier,Peter Conveysearch and Training Network on JET Simulations, Experiments and Theory. At this school the lecturers gave an introduction to observational properties and basic models describing the launching and collimation mechanisms of jets. The first half of the book is devoted to general observational constrain
作者: Invigorate    時間: 2025-3-27 22:27

作者: MEEK    時間: 2025-3-28 02:31
Filipe Martinhosearch and Training Network on JET Simulations, Experiments and Theory. At this school the lecturers gave an introduction to observational properties and basic models describing the launching and collimation mechanisms of jets. The first half of the book is devoted to general observational constrain
作者: BULLY    時間: 2025-3-28 09:02
Rogélia Martins,Miguel Carneirorming a comprehensive account of jets from young starsAtomic jets and molecular out?ows from Young Stellar Objects (YSOs) are among the most spectacular of astrophysical phenomena. Approaching this topic, one gets immediately trapped by the breathtaking beauty of the op- calimagestakenfromEarthorSpa
作者: FRAUD    時間: 2025-3-28 11:42
Daniel Crespo,Miguel ?ngelo Pardalelded a lot of new information regarding outflow activity and binarity. Using spectroscopy, one can investigate the kinematics and excitation conditions of jets close to where they are launched and resolve close binaries. The primary constraint to the use of spectroscopy in this manner is the maximu
作者: 性冷淡    時間: 2025-3-28 16:33
José S. Antunes do Carmo one gets immediately trapped by the breathtaking beauty of the op- calimagestakenfromEarthorSpacewithmoderntelescopes,onlytodiscover soonafterthatthephysicsthatregulatestheirpropertiesisevenmoreintri- ing. Out?ows are believed to play a fundamental role in the formationprocess of a new star and its
作者: AWL    時間: 2025-3-28 22:17

作者: integrated    時間: 2025-3-29 00:32
Miguel Carneiro,Rogélia Martinselded a lot of new information regarding outflow activity and binarity. Using spectroscopy, one can investigate the kinematics and excitation conditions of jets close to where they are launched and resolve close binaries. The primary constraint to the use of spectroscopy in this manner is the maximu
作者: progestogen    時間: 2025-3-29 06:31
Jo?o Ser?dio,David M. Patersony spherically symmetric winds to highly collimated jets. In some cases, e.g., in jets associated with young stellar objects, the bulk outflow speeds are nonrelativistic, while in others, e.g., in jets associated with active galactic nuclei or gamma-ray bursts, it can even be highly relativistic. The
作者: 模范    時間: 2025-3-29 09:29
Jo?o Ser?dio,Johann Lavaudccurred within the domains of astronomical observations, astrophysical modeling and numerical simulations, but the recent advent of high energy density facilities has added experimental control to jet studies...Front-line research on jet launching and collimation requires a highly interdisciplinary
作者: 玷污    時間: 2025-3-29 14:05

作者: CANE    時間: 2025-3-29 19:08
Trilok Kumar Jain,Nirupa Jainspeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows
作者: intimate    時間: 2025-3-29 22:56
Priscila F. M. Lopesspeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows
作者: 冰河期    時間: 2025-3-30 02:04
Heitor Oliveira Braga,Joelson Musiello-Fernandes in the introduction, this reflects very much the quite different mode of energy transport in the two classes of source. Another parameter which also highlights the differences between the two types of jet is the velocity. This can be written in the form: .. = 430 km s...... (./..)...For class I jet
作者: Pepsin    時間: 2025-3-30 05:52

作者: Chronic    時間: 2025-3-30 11:03

作者: Nonconformist    時間: 2025-3-30 13:24

作者: 領(lǐng)導(dǎo)權(quán)    時間: 2025-3-30 16:38
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