標(biāo)題: Titlebook: High Energy Density Laboratory Astrophysics; G.A. Kyrala Book 2005 Springer Science+Business Media B.V. 2005 Accretion.MHD.Plasma.astrophy [打印本頁(yè)] 作者: GERM 時(shí)間: 2025-3-21 18:56
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics影響因子(影響力)
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics被引頻次
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics被引頻次學(xué)科排名
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics年度引用
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics年度引用學(xué)科排名
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics讀者反饋
書(shū)目名稱(chēng)High Energy Density Laboratory Astrophysics讀者反饋學(xué)科排名
作者: 抗原 時(shí)間: 2025-3-21 20:27
s such as intense lasers and z-pinches. Research is underway in many areas, such as compressible hydrodynamic mixing, strong shock phenomena, radiation flow, radiative shocks and jets, complex opacities, equations of stat, and relativistic plasmas. Beyond this current research and the papers it is p作者: farewell 時(shí)間: 2025-3-22 03:37
Laboratory Experiments of Stellar Jets from the Perspective of an Observer,ed jets with velocities and Mach numbers similar to those within stellar jets, and the field seems poised to make significant advances by connecting observations and theories with experiments. This article points out several aspects of stellar jets that might be clarified by such experiments.作者: BAIT 時(shí)間: 2025-3-22 05:45 作者: LIMIT 時(shí)間: 2025-3-22 12:35
. These protocols are used for the evaluation of compounds that can be carried out by a single individual in a Category 3 containment laboratory. The number of compounds analyzed would be about 10, which is a convenient number to fill a single 96-well p24 enzyme-linked immunosorbent assay (ELISA) plate.作者: 合乎習(xí)俗 時(shí)間: 2025-3-22 15:17 作者: 空氣 時(shí)間: 2025-3-22 17:22 作者: 法官 時(shí)間: 2025-3-23 01:01
Hypernovae and Gamma-Ray Bursts,. The abundance patterns of hypernovae are characterized by large ratios (Zn, Co)/Fe and small ratios (Mn, Cr)/Fe, indicating a significant contribution of hypernovae to the early Galactic chemical evolution.作者: 嫌惡 時(shí)間: 2025-3-23 02:26 作者: 溺愛(ài) 時(shí)間: 2025-3-23 07:58 作者: BORE 時(shí)間: 2025-3-23 13:22 作者: OUTRE 時(shí)間: 2025-3-23 16:58
lymphoblastoid cell lines, preparation of peripheral blood mononuclear cells (PMMCs), and determination of the infectivity of the HIV stock-supernatant and antiviral assays. The assays described use both acutely and chronically infected cells. Toxicity of compounds is assessed by measuring .C uptake作者: fatty-acids 時(shí)間: 2025-3-23 20:30
J.C. Wheeler,S. Akiyama,P.T. Williams. The catalytic domain is contained within the N-terminal third of the protein, and the remainder comprises a structural “scaffold” protein. The scaffold protein is independently expressed in excess to the polyprotein from an internal initiation codon. The protease cleaves the polyprotein at two sit作者: bronchodilator 時(shí)間: 2025-3-23 23:35 作者: Affection 時(shí)間: 2025-3-24 05:45 作者: 有害 時(shí)間: 2025-3-24 06:38 作者: Femine 時(shí)間: 2025-3-24 14:11
J. Martin Laming,Una HwangNAs – of viral or cellular origin – affect many aspects of virus biology, and replication of many, if not all, mammalian viruses can be suppressed by RNAi.. Antiviral RNAi: Concepts, Methods, and Applications .provides a collection of protocols for the analysis of viral small RNAs and natural antivi作者: NAVEN 時(shí)間: 2025-3-24 16:46
A.D. Edens,T. Ditmire,J.F. Hansen,M.J. Edwards,R.G. Adams,P. Rambo,L. Ruggles,I.C. Smith,J.L. PorterNAs – of viral or cellular origin – affect many aspects of virus biology, and replication of many, if not all, mammalian viruses can be suppressed by RNAi.. Antiviral RNAi: Concepts, Methods, and Applications .provides a collection of protocols for the analysis of viral small RNAs and natural antivi作者: Astigmatism 時(shí)間: 2025-3-24 20:20
R. Paul DrakeNAs – of viral or cellular origin – affect many aspects of virus biology, and replication of many, if not all, mammalian viruses can be suppressed by RNAi.. Antiviral RNAi: Concepts, Methods, and Applications .provides a collection of protocols for the analysis of viral small RNAs and natural antivi作者: transplantation 時(shí)間: 2025-3-24 23:38
J.F. Hansen,M.J. Edwards,D. Froula,G. Gregori,A. Edens,T. DitmireNAs – of viral or cellular origin – affect many aspects of virus biology, and replication of many, if not all, mammalian viruses can be suppressed by RNAi.. Antiviral RNAi: Concepts, Methods, and Applications .provides a collection of protocols for the analysis of viral small RNAs and natural antivi作者: 獨(dú)行者 時(shí)間: 2025-3-25 04:15 作者: Expertise 時(shí)間: 2025-3-25 10:35
X. Ribeyre,V.T. Tikhonchuk,S. Bouquetation advice from the experts.Includes supplementary materia.Viruses and RNAi share an intricate relationship at many levels. RNAi is an important antiviral defense mechanism in plants and invertebrates, microRNAs – of viral or cellular origin – affect many aspects of virus biology, and replication 作者: 兒童 時(shí)間: 2025-3-25 11:41 作者: extract 時(shí)間: 2025-3-25 17:17 作者: 背心 時(shí)間: 2025-3-25 22:07
C. Courtois,R.A.D. Grundy,A.D. Ash,D.M. Chambers,R.O. Dendy,K.G. Mcclements,N.C. Woolseyation advice from the experts.Includes supplementary materia.Viruses and RNAi share an intricate relationship at many levels. RNAi is an important antiviral defense mechanism in plants and invertebrates, microRNAs – of viral or cellular origin – affect many aspects of virus biology, and replication 作者: WAG 時(shí)間: 2025-3-26 01:28
Patrick HartiganNAs – of viral or cellular origin – affect many aspects of virus biology, and replication of many, if not all, mammalian viruses can be suppressed by RNAi.. Antiviral RNAi: Concepts, Methods, and Applications .provides a collection of protocols for the analysis of viral small RNAs and natural antivi作者: Rct393 時(shí)間: 2025-3-26 07:40 作者: GLIB 時(shí)間: 2025-3-26 11:49 作者: conception 時(shí)間: 2025-3-26 14:19 作者: grandiose 時(shí)間: 2025-3-26 17:01 作者: acrimony 時(shí)間: 2025-3-26 22:11 作者: 叫喊 時(shí)間: 2025-3-27 01:09 作者: 使成波狀 時(shí)間: 2025-3-27 07:46 作者: ARM 時(shí)間: 2025-3-27 09:47
Effects of Initial Conditions on Compressible Mixing in Supernova-Relevant Laboratory Experiments,) instabilities. In addition, perturbation growth can result from material expansion in large-scale velocity gradients behind the shock front. Laser-driven experiments are designed to produce a strongly shocked interface whose evolution is a scaled version of the unstable hydrogen-helium interface i作者: Clumsy 時(shí)間: 2025-3-27 13:56
Laboratory Astrophysics Experiments for Simulation Code Validation: A Case Study, laboratory. In addition to the opportunity to perform basic research into the nature and properties of materials in astrophysical environments, laboratory astrophysics experiments serve beautifully for validating calculations performed by simulation codes designed to model astrophysical phenomena. 作者: GOAT 時(shí)間: 2025-3-27 18:58
Studies of Laser-Driven Radiative Blast Waves, passage through a background gas on the hydrodynamical evolution of blast waves was examined. The laser’s passage heated a channel in the gas, creating a region where a portion of the blast wave front had an increased velocity, leading to the formation of a bump-like protrusion on the blast wave. T作者: BINGE 時(shí)間: 2025-3-27 23:45
Radiative Shocks in Astrophysics and the Laboratory,ptical depth of the upstream region and the downstream region both affect the behavior of radiative shocks. Optically thick systems such as stellar interiors or supernovae permit only limited shock-induced increases in density. At the other limit, the radiation and shock dynamics in optically thin s作者: sperse 時(shí)間: 2025-3-28 02:58
Laboratory Simulations of Supernova Shockwave Propagation,lar shocks in the laboratory by focusing laser pulses onto the tip of a solid pin surrounded by ambient gas; ablated material from the pin rapidly expands and launches a shock through the surrounding gas. Laser pulses were typically 5 ns in duration with ablative energies ranging from 1–150 J. Shock作者: Gesture 時(shí)間: 2025-3-28 07:50 作者: 嘲弄 時(shí)間: 2025-3-28 11:40
Analytical Study of Supernova Remnant Non-Stationary Expansions, by blowing pulsar wind. The most dangerous perturbations correspond to wavelengths comparable to the shell thickness. We analyze the fragility of the supernova remnant shell in function of the initial perturbation amplitude and the shell thickness.作者: 開(kāi)頭 時(shí)間: 2025-3-28 16:47
Hypernovae and Gamma-Ray Bursts,o the enigmatic Gamma-Ray Bursts. The optical properties of hypernovae indicate that they are significantly aspherical. Synthetic light curves and late-phase spectra of aspherical supernova/hypernova models are presented. These models can account for the optical observations of SNe 1998bw and 2002ap作者: 發(fā)牢騷 時(shí)間: 2025-3-28 18:53
Radiation Hydrodynamics in Supernovae,e and thermonuclear supernovae. In supernovae, one of the main issues is the coupling between a radiation field and properties of the matter. Due to the low densities, nonthermal excitation by high-energy photons from radioactive decays and the time dependence of the problem, significant departures 作者: 陳舊 時(shí)間: 2025-3-28 23:09
Experiment on Collisionless Plasma Interaction with Applications to Supernova Remnant Physics,rnova remnant (SNR) are discussed. Ideal magneto-hydrodynamic scaling indicates that the experimental plasma matches the SNR plasma at 500 ps. Experimental data show that the magnetic field can alter the plasma density profile when two similar plasmas interact in a colliding geometry. These results 作者: Aromatic 時(shí)間: 2025-3-29 05:16 作者: Spangle 時(shí)間: 2025-3-29 10:00 作者: Costume 時(shí)間: 2025-3-29 13:12 作者: 頭腦冷靜 時(shí)間: 2025-3-29 16:01 作者: Freeze 時(shí)間: 2025-3-29 21:00
,Hydrogen EOS at Megabar Pressures and the Search for Jupiter’s Core, from ～0.1.. to ～80.. (1.. = Jupiter mass = 1.9.30g), comprising hydrogen-rich giant planets (mass < 13..) and brown dwarfs (mass > 13.. but ～<80..), the so-called substellar objects (SSOs). Formation of giant planets may involve nucleated collapse of nebular gas onto a solid, dense core of mass ～0.作者: 責(zé)任 時(shí)間: 2025-3-30 01:21 作者: 黃油沒(méi)有 時(shí)間: 2025-3-30 07:11
How Did Cassiopeia A Explode? A Chandra VLP,The Cassiopeia A supernova remnant will be observed by Chandra for 1 Ms this spring. We discuss our motivations and plans for acquiring and analyzing these data.作者: Exclaim 時(shí)間: 2025-3-30 10:42 作者: vascular 時(shí)間: 2025-3-30 15:03
https://doi.org/10.1007/1-4020-4162-4Accretion; MHD; Plasma; astrophysics; relativistic jet作者: 廣告 時(shí)間: 2025-3-30 16:41
Asymmetric Supernovae: Yes, Rotation and Magnetic Fields are Important,henomena are at work involving rotation and magnetic fields. We summarize the importance of the magnetorotational instability for the core collapse problem and sketch some of the effects that large magnetic fields, ～10. G, may have on the physics of the supernova explosion.作者: 溫室 時(shí)間: 2025-3-30 21:58
Radiative Shock Experiments at LULI,designed targets filled with xenon gaz at low pressure, the propagation of a strong shock with a radiative precursor is evidenced. The main measured quantities related to the shock (electronic density, propagation velocities, temperature, radial dimension) are presented and compared with various numerical simulations.作者: 低能兒 時(shí)間: 2025-3-31 03:02
Analytical Study of Supernova Remnant Non-Stationary Expansions, by blowing pulsar wind. The most dangerous perturbations correspond to wavelengths comparable to the shell thickness. We analyze the fragility of the supernova remnant shell in function of the initial perturbation amplitude and the shell thickness.作者: effrontery 時(shí)間: 2025-3-31 07:24 作者: 流逝 時(shí)間: 2025-3-31 10:31 作者: aerial 時(shí)間: 2025-3-31 15:22 作者: circuit 時(shí)間: 2025-3-31 18:39 作者: endoscopy 時(shí)間: 2025-3-31 21:43
Laboratory Simulations of Supernova Shockwave Propagation,to the heated gas. The second shock remains visible and continues to expand. A minimum condition for the formation of the second shock is that the original shock is super-critical, i.e., the temperature distribution ahead of the original shock has an inflexion point. In a non-radiative control exper作者: Canvas 時(shí)間: 2025-4-1 05:34 作者: 知道 時(shí)間: 2025-4-1 09:45
A Hed Laboratory Astrophysics Testbed Comes of Age: Jet Deflection via Cross Winds,plying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed作者: Ganglion 時(shí)間: 2025-4-1 13:13 作者: Infant 時(shí)間: 2025-4-1 18:20 作者: 金絲雀 時(shí)間: 2025-4-1 20:59 作者: offense 時(shí)間: 2025-4-2 00:28
attention on this emerging research area. The conference brought together different scientists interested in this emerging new field, with topics covering:..- Hydrodynamic instabilities in astrophysics,.- Supernovae and supernova remnant evolution,.- Astrophysical shocks, blast waves, and jets,.- Stellar opa978-90-481-6880-4978-1-4020-4162-4
