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Short Ileal Microvillus Length Phenotype Associates with Progression from Inflammatory to Complicated Disease Behavior in Pediatric Crohn's Disease. [PDF]
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Science, 1985
The Very Long Baseline Array is a high-resolution synthesis radio telescope consisting of ten antennas, each 25 meters in diameter, located throughout the United States from Puerto Rico to Hawaii. Each antenna will be equipped with low-noise receivers spaced throughout the frequency range from 330 megahertz to 43 gigahertz, a hydrogen-maser frequency ...
K I, Kellermann, A R, Thompson
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The Very Long Baseline Array is a high-resolution synthesis radio telescope consisting of ten antennas, each 25 meters in diameter, located throughout the United States from Puerto Rico to Hawaii. Each antenna will be equipped with low-noise receivers spaced throughout the frequency range from 330 megahertz to 43 gigahertz, a hydrogen-maser frequency ...
K I, Kellermann, A R, Thompson
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Long term baseline atmospheric monitoring
Journal of Chemical Education, 1975Discusses some of the activities regarding atmospheric monitoring at the Mauna Loa Observatory in Hawaii.
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Physics Today, 1969
THE RAPID DEVELOPMENT of electronic technology has given man the ability to control electrical events in the time domain with extraordinary precision, just as the mechanical revolution of the last century improved, by orders of magnitude, our power to control linear dimensions of physical objects. Perhaps the only failure in the analogy is quantitative;
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THE RAPID DEVELOPMENT of electronic technology has given man the ability to control electrical events in the time domain with extraordinary precision, just as the mechanical revolution of the last century improved, by orders of magnitude, our power to control linear dimensions of physical objects. Perhaps the only failure in the analogy is quantitative;
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LONG BASELINE NEUTRINO EXPERIMENTS
Particle Physics in Laboratory, Space and Universe, 2005The evidence of neutrino oscillation in the atmospheric neutrinos discovered by Super-Kamiokande (SK) [1] is being confirmed by the first accelerator-based long baseline (LBL) oscillation experiment, K2K [2]. Also, implications of neutrino oscillation in the solar neutrino [3] is now confirmed by a reactor-based LBL experiment, KamLAND [4].
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Optical Long Baseline Interferometry
2016Optical Long Baseline Interferometry provides unrivalled angular resolution on bright and compact astrophysical sources. The link between the observables (interferometric phase and contrast ) and the image of the source is a Fourier transform expressed first by van Cittert and Zernike .
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Very long baseline interferometry
Radio Science, 1986A general review is given of very long baseline interferometry, touching on basic principles and applications, current instrumentation, organization and future developments. Some astronomical highâlights are discussed.
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Very Long Baseline Interferometry
1997The practice of Very Long Baseline Interferometry (VLBI) has undergone a great deal of development since the first demonstrations of the technique in 1967. High quality images including spectroscopy and polarimetry are now routinely produced for a variety of high brightness radio sources.
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