Period, Q_p and Amplitude of the Pole Tide     

Robert G. Currie 《Geophysical Journal International》1975,43(1):73-86

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The Propagation of Surface Waves in an Elastic Medium with Orthorhombic Symmetry   总被引：1，自引：0，他引：1  

Robert Stoneley 《Geophysical Journal International》1963,8(2):176-186

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Spatial and temporal correlation of underwater sunlight fluctuations in the sea     

Fraser  A. Walker  R. Jurgens  F. 《Oceanic Engineering, IEEE Journal of》1980,5(3):195-198

A submerged linear array of photodetectors was used to measure sunlight irradiance fluctuations caused by ocean surface waves. Decorrelation times and lengths were found to be functions of depth. It was also found that the sensor depth selects a dominant temporal frequency from the random surface waves.  相似文献   

Multiple Reflection of Plane P and SV Waves By a Dipping Layer     

Hiroshi Ishii  Robert M. Ellis 《Geophysical Journal International》1970,20(1):11-30

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Numerical explorations of the rectilinear problem of three bodies     

R. Broucke  D. E. Walker 《Celestial Mechanics and Dynamical Astronomy》1980,21(1):73-81

We present some results of a numerical exploration of the rectilinear problem of three bodies, with the two outer masses equal. The equations of motion are first given in relative coordinates and in regularized variables, removing both binary collision singularities in a single coordinate transformation. Among our most important results are seven periodic solutions and three symmetric triple collision solutions. Two of these periodic solutions have been continued into families, the outer massm ₃ being the family parameter. One of these families exists for all masses while the second family is a branch of the first at a second-kind critical orbit. This last family ends in a triple collision orbit.Proceedings of the Sixth Conference on Mathematical Methods in Celestial Mechanics held at Oberwolfach (West Germany) from 14 to 19 August, 1978.  相似文献   

One Hundredth Anniversary: Geographical Society of Finland     

Arnold Alanen  Robert Morrill 《The Professional geographer》1989,41(2):206-207

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The 1984 Round Valley, California Earthquake Sequence     

Keith F. Priestley  Kenneth D. Smith  Robert S. Cockerham 《Geophysical Journal International》1988,95(2):215-235

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First results from the Very Small Array – I. Observational methods     

Robert A. Watson  Pedro Carreira  Kieran Cleary  Rod D. Davies  Richard J. Davis  Clive Dickinson  Keith Grainge †  Carlos M. Gutiérrez  Michael P. Hobson  Michael E. Jones  Rüdiger Kneissl  Anthony Lasenby  Klaus Maisinger  Guy G. Pooley  Rafael Rebolo  José Alberto Rubiño-Martin ‡  Ben Rusholme §  Richard D. E. Saunders  Richard Savage  Paul F. Scott  An&#;e Slosar  Pedro J. Sosa Molina  Angela C. Taylor  David Titterington  Elizabeth Waldram  Althea Wilkinson 《Monthly notices of the Royal Astronomical Society》2003,341(4):1057-1065

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INGRID: A near-infrared camera for the William Herschel Telescope     

Christopher Packham  Keith L. Thompson  Almudena Zurita  Johan H. Knapen  Ian Smail  Robert Greimel  Daniel F. M. Folha  Chris Benn  rew Humphrey  Rene Rutten  David Ciardi  Matthieu Bec  Richard Bingham  Simon Craig  Kevin Dee  Derek Ives  Paul Jolley  Peter Moore  Marti Pi i Puig  Simon Rees  Gordon Talbot  Sue Worswick 《Monthly notices of the Royal Astronomical Society》2003,345(2):395-405

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A concept for a superconducting tunnelling junction based spectrograph     

Mark Cropper  M. Barlow  M. A. C. Perryman  Keith Horne  R. Bingham  M. Page  P. Guttridge  A. Smith  A. Peacock  D. Walker  P. Charles 《Monthly notices of the Royal Astronomical Society》2003,344(1):33-44

We describe a multi-order spectrograph concept suitable for 8-m class telescopes, using the intrinsic spectral resolution of superconducting tunnelling junction detectors to sort the spectral orders. The spectrograph works at low orders, 1–5 or 1–6, and provides spectral coverage with a resolving power of   R ≃ 8000  from the atmospheric cut-off at 320 nm to the long-wavelength end of the infrared H or K band at 1800 nm or 2400 nm. We calculate that the spectrograph would provide substantial throughput and wavelength coverage, together with high time resolution and sufficient dynamic range. The concept uses currently available technology, or technologies with short development horizons, restricting the spatial sampling to two linear arrays; however, an upgrade path to provide more spatial sampling is identified. All of the other challenging aspects of the concept – the cryogenics, thermal baffling and magnetic field biasing – are identified as being feasible.  相似文献