標(biāo)題: Titlebook: High Time Resolution Astrophysics; Don Phelan,Oliver Ryan,Andrew Shearer Book 2008 Springer Science+Business Media B.V. 2008 Astronomy boo [打印本頁(yè)] 作者: 不正常 時(shí)間: 2025-3-21 17:48
書目名稱High Time Resolution Astrophysics影響因子(影響力)
書目名稱High Time Resolution Astrophysics影響因子(影響力)學(xué)科排名
書目名稱High Time Resolution Astrophysics網(wǎng)絡(luò)公開(kāi)度
書目名稱High Time Resolution Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書目名稱High Time Resolution Astrophysics被引頻次
書目名稱High Time Resolution Astrophysics被引頻次學(xué)科排名
書目名稱High Time Resolution Astrophysics年度引用
書目名稱High Time Resolution Astrophysics年度引用學(xué)科排名
書目名稱High Time Resolution Astrophysics讀者反饋
書目名稱High Time Resolution Astrophysics讀者反饋學(xué)科排名
作者: Palliation 時(shí)間: 2025-3-21 21:58 作者: Mere僅僅 時(shí)間: 2025-3-22 01:43
978-90-481-7657-1Springer Science+Business Media B.V. 2008作者: 動(dòng)機(jī) 時(shí)間: 2025-3-22 08:33
High Time Resolution Astrophysics978-1-4020-6518-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: PARA 時(shí)間: 2025-3-22 10:42 作者: 失望未來(lái) 時(shí)間: 2025-3-22 14:43 作者: Flawless 時(shí)間: 2025-3-22 18:53
Andrew Shearer than their electronic counterparts, will be used extensively to link current silicon-based technology devices for information transport and elaboration. Near-field microscopy, which is capable of accessing the nanometer scale in the optical domain, allows us to enhance our comprehension of the loca作者: Addictive 時(shí)間: 2025-3-22 23:55 作者: GULP 時(shí)間: 2025-3-23 05:16
Tariq Shahbaza p- cision suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or AFM. The STM relies on electrons tunneling between tip and sample whereas the AFM depends on the force acting on the tip when it was placed near th作者: 我不死扛 時(shí)間: 2025-3-23 06:02
C. Simon Jefferyel Prize of 1986 on Sc- ningTunnelingMicroscopysignaled a new era in imaging. The sc- ning probes emerged as a new - strument for imaging with a p- cision suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or AFM.作者: Offstage 時(shí)間: 2025-3-23 10:06
T. R. Marshel Prize of 1986 on Sc- ningTunnelingMicroscopysignaled a new era in imaging. The sc- ning probes emerged as a new - strument for imaging with a p- cision suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or AFM.作者: 天文臺(tái) 時(shí)間: 2025-3-23 17:46
Dainis Dravinsa p- cision suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or AFM. The STM relies on electrons tunneling between tip and sample whereas the AFM depends on the force acting on the tip when it was placed near th作者: Palter 時(shí)間: 2025-3-23 22:03 作者: NATTY 時(shí)間: 2025-3-24 00:11 作者: 觀察 時(shí)間: 2025-3-24 05:20 作者: headway 時(shí)間: 2025-3-24 10:02 作者: BOOST 時(shí)間: 2025-3-24 13:48 作者: Predigest 時(shí)間: 2025-3-24 17:22
Oliver Ryan,Mike Redfernel Prize of 1986 on Sc- ning Tunneling Microscopy sig- led a new era in imaging. The sc- ning probes emerged as a new i- trument for imaging with a pre- sion suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or A作者: Stricture 時(shí)間: 2025-3-24 21:25 作者: 把…比做 時(shí)間: 2025-3-25 03:11
L. Strüder,G. Kanbach,N. Meidinger,F. Schopper,R. Hartmann,P. Holl,H. Soltau,R. Richter,G. Lutzre showing that qualitatively new behavior in the physical phenomena is often produced by the size constraints. Although such changes in behavior can be the dominant effects in nanoscale structures, we still have remarkably little experience or intuition for the expected phenomena and their practica作者: Adj異類的 時(shí)間: 2025-3-25 04:26
Don Phelan,Alan P. Morrisonl, semiconductor and insulating surfaces. The same chemical compounds give rise to different structures, depending on several factors, such as the adsorbate coverage, the substrate orientation or the temperature. Self-assembled patterns formed on the step edges of insulating surfaces — or raised fro作者: 不滿分子 時(shí)間: 2025-3-25 09:13
Roger W. Romani,Thomas J. Bay,Jennifer Burney,Blas Cabreral, semiconductor and insulating surfaces. The same chemical compounds give rise to different structures, depending on several factors, such as the adsorbate coverage, the substrate orientation or the temperature. Self-assembled patterns formed on the step edges of insulating surfaces — or raised fro作者: hemorrhage 時(shí)間: 2025-3-25 12:08
O. H. W. Siegmund,J. V. Vallerga,B. Welsh,A. S. Tremsin,J. B. McPhateel Prize of 1986 on Sc- ning Tunneling Microscopy sig- led a new era in imaging. The sc- ning probes emerged as a new i- trument for imaging with a pre- sion suf?cient to delineate single atoms. At ?rst there were two – the Scanning Tunneling Microscope, or STM, and the Atomic Force Mic- scope, or A作者: FIS 時(shí)間: 2025-3-25 15:51 作者: 突襲 時(shí)間: 2025-3-25 21:14
High Time Resolution Astrophysics and Pulsars,or integration times would normally be measured in minutes rather seconds and definitely not on sub-second time scales. At the start of the 21st century pulsar observations are still pushing the limits of detector/telescope capabilities. Flux variations on times scales less than 1 nsec have been obs作者: 遺傳 時(shí)間: 2025-3-26 02:09
High Time Resolution Observations of Cataclysmic Variables,. The most rapid timescales observed in CVs are of the order of a few seconds, and thus CVs are relatively slow objects compared to some phenomena studied by the high time-resolution community. However, the rich and varied processes which occur in CVs make high time-resolution observations powerful 作者: 樹(shù)膠 時(shí)間: 2025-3-26 05:36 作者: 考得 時(shí)間: 2025-3-26 11:42 作者: 吊胃口 時(shí)間: 2025-3-26 16:29 作者: Infinitesimal 時(shí)間: 2025-3-26 18:30
OPTIMA: A High Time Resolution Optical Photo-Polarimeter,y of the Max-Planck-Institut für Extraterrestrische Physik. This sensitive, portable detector is used to observe optical emissions of sources that radiate mainly at X- and gamma-ray energies, like pulsars and other highly variable compact sources. The single photon counting instrument is based on fi作者: 消息靈通 時(shí)間: 2025-3-26 23:37 作者: lesion 時(shí)間: 2025-3-27 01:53 作者: 不朽中國(guó) 時(shí)間: 2025-3-27 08:18
An Ultra-High-Speed Stokes Polarimeter forAstronomy,and magnetic field strengths to be investigated. In the context of high time resolution astrophysics polarimetry is particularly valuable in understanding the nature of the optical pulsations from pulsars, and whilst the averaged (over many cycles) linear polarization of the Crab nebula pulsar was d作者: 量被毀壞 時(shí)間: 2025-3-27 11:53
Use of an Extremely Large Telescope for HTRA,, at its most basic level, detection of the faintest stellar sources and instrinsic features, and detailed quantitative analysis of relatively bright sources. The development of such a telescope thus plays to the strengths of high time resolution (HTR) detectors which provide single photon detection作者: 寬容 時(shí)間: 2025-3-27 16:46
EMCCD Technology in High Precision Photometry on Short Timescales,is on probing the smallest structures in active galactic jets. Factors external to the EMCCD, rather than the architecture of the EMCCD itself, most often limit the precision of photometry that can be reached with groundbased observations. Although EMCCDs can be used in photon-counting mode, reliabl作者: Eviction 時(shí)間: 2025-3-27 19:57
The Development of Avalanche Amplifying pnCCDs: A Status Report,ns in astronomy and other fields. In 2005 we have started to develop pnCCDs with high quantum efficiency for fast imaging of single optical photons in the wavelength range ∽350–1100 nm. The concept is based on fully depleted, back-illuminated pnCCDs with a sensitive thickness of 450 μmum which were 作者: 名次后綴 時(shí)間: 2025-3-27 22:35 作者: itinerary 時(shí)間: 2025-3-28 03:29
Transition Edge Cameras for Fast Optical Spectrophotometry, is to use very large focal plane arrays, for a high multiplex advantage; this is a natural driver in extragalactic survey science. The other avenue to efficiency applies to single source science, where a large field of view is not necessary, but energy resolution over a broad wavelength range, high作者: 取消 時(shí)間: 2025-3-28 07:54
Imaging Photon Counting Detectors for High Time Resolution Astronomy,resolution imaging with fast event timing capability have been a significant technical challenge. We have developed a high-temporal and -spatial resolution, high-throughput sealed tube microchannel plate detector with electronic readout as a tool for HTRA applications. The design is based on a 25 mm作者: DUCE 時(shí)間: 2025-3-28 11:26
High-Speed Optical Observations of X-ray Binaries,作者: 正論 時(shí)間: 2025-3-28 16:21
ULTRACAM: An Ultra-Fast, Triple-Beam CCD Camera for High-Speed Astrophysics,作者: 支柱 時(shí)間: 2025-3-28 20:41 作者: BILE 時(shí)間: 2025-3-28 23:37
Andrew Shearerrameters to be studied and understood for final device engineering. PM-SNOM tailors micropolarimetry to the nanometer scale. Quantitative measurements of the birefringent and dichroic properties of single nanocrystals, thin films, organic/inorganic photonic crystals and waveguides demonstrate the wi作者: stroke 時(shí)間: 2025-3-29 03:33
S. P. Littlefair different instruments appeared. There are signi?cant differences between the Scanning Probe Microscopes or SPM, and others such as the Scanning Electron Microscope or SEM. The probe microscopes do not require preparation of the sample and they operate in ambient atmosphere, whereas, the SEM must op作者: 健談 時(shí)間: 2025-3-29 09:34 作者: 暫時(shí)過(guò)來(lái) 時(shí)間: 2025-3-29 15:13 作者: 改革運(yùn)動(dòng) 時(shí)間: 2025-3-29 19:16 作者: 浪蕩子 時(shí)間: 2025-3-29 19:59
G. Kanbach,A. Stefanescu,S. Duscha,M. Mühlegger,F. Schrey,H. Steinle,A. Slowikowska,H. Spruit different instruments appeared. There are signi?cant differences between the Scanning Probe Microscopes or SPM, and others such as the Scanning Electron Microscope or SEM. The probe microscopes do not require preparation of the sample and they operate in ambient atmosphere, whereas, the SEM must op作者: 溫順 時(shí)間: 2025-3-30 02:07 作者: Console 時(shí)間: 2025-3-30 04:11 作者: 背叛者 時(shí)間: 2025-3-30 09:00
Niall Smith,Alan Giltinan,Aidan O’Connor,Stephen O’Driscoll,Adrian Collins,Dylan Loughnan,Andreas Paproperties of the individual molecules will be performed. Internal degrees of freedoms of the molecules and mechanical instabilities are rather complex phenomena, which will need both experimental and computational efforts to achieve the required degree of control of these novel molecular electronic作者: figurine 時(shí)間: 2025-3-30 13:24
L. Strüder,G. Kanbach,N. Meidinger,F. Schopper,R. Hartmann,P. Holl,H. Soltau,R. Richter,G. Lutzr desired characteristics..We hope that the few examples reported here will stimulate researchers to engage in the exploration of this exciting world..We would like to thank Mattia Fanetti, Maria Grazia Betti, Carlo Mariani and Cinzia Cepek as collaborators for the results we presented here. The nan作者: Classify 時(shí)間: 2025-3-30 20:10
Don Phelan,Alan P. Morrisonproperties of the individual molecules will be performed. Internal degrees of freedoms of the molecules and mechanical instabilities are rather complex phenomena, which will need both experimental and computational efforts to achieve the required degree of control of these novel molecular electronic作者: 蘆筍 時(shí)間: 2025-3-30 23:11 作者: 破布 時(shí)間: 2025-3-31 02:41 作者: Irremediable 時(shí)間: 2025-3-31 06:20 作者: Popcorn 時(shí)間: 2025-3-31 10:58
An Ultra-High-Speed Stokes Polarimeter forAstronomy,lution. This imposes certain constraints on the design of the polarimeter, which rules out all of the popular designs. We describe the design of a novel polarimeter which will be able to meet these constraints.This is based upon a design by Compain and Drevillon [1] in which their design is modified
