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Traditionally astrophysics has concerned itself with minimum time-scales measured in hours rather than seconds. This was understandable as the available recording media were slow; e.g. chart recorders and photographic plates. In the 1950s, 60s and 70s wavebands away from the optical were developed; from ground based radio studies to space and balloon borne high energy work. In contrast to optical wavelengths instrumentation in these (high and low energy) regimes was capable of time resolutions of less than a second | ASTROPHYSICS AND SPACE SCIENCE LIBRARY Don Phelan Oliver Ryan Andrew Shearer Editors High Time Resolution Astrophysics 0S SL 0 Springer High Time Resolution Astrophysics Astrophysics and Space Science Library EDITORIAL BOARD Chairman W. B. BURTON National Radio Astronomy Observatory Charlottesville Virginia U.S.A. bburton@nrao.edu University of Leiden The Netherlands burton@strw. leidenuniv.nl F. BERTOLA University of Padua Italy J. P CASSINELLI University of Wisconsin Madison U.S.A. C. J. CESARSKY European Southern Observatory Garching bei Mũnchen Germany P. EHRENFREUND Leiden University The Netherlands O. ENGVOLD University of Oslo Norway A. HECK Strasbourg Astronomical Observatory France E. P. J. VAN DEN HEUVEL University of Amsterdam The Netherlands V M. KASPI McGill University Montreal Canada J. M. E. KUIJPERS University of Nijmegen The Netherlands H. VANDERLAAN University of Utrecht The Netherlands P G. MURDIN Institute of Astronomy Cambridge UK F. PACINI Istituto Astronomia Arcetri Firenze Italy V RADHAKRISHNAN Raman Research Institute Bangalore India B. V. SOMOV Astronomical Institute Moscow State University Russia R. A. SUNYAEV Space Research Institute Moscow .
