Titlebook: High Time Resolution Astrophysics; Don Phelan,Oliver Ryan,Andrew Shearer Book 2008 Springer Science+Business Media B.V. 2008 Astronomy boo

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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

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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

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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

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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

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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

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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