Results 171 to 180 of about 18,093 (220)
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AIP Conference Proceedings, 1995
The Laser Interferometer Gravitational‐Wave Observatory (LIGO) is part of an international effort to search for gravitational waves emitted by astrophysical sources. Detector sites at Hanford, Washington and Livingston, Louisiana, will consist of interferometers to detect the small displacements of suspended test masses induced by the gravitational ...
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The Laser Interferometer Gravitational‐Wave Observatory (LIGO) is part of an international effort to search for gravitational waves emitted by astrophysical sources. Detector sites at Hanford, Washington and Livingston, Louisiana, will consist of interferometers to detect the small displacements of suspended test masses induced by the gravitational ...
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Inference: International Review of Science, 2016
Though some American astronomers were reluctant to accept that gravitational wave physics is indeed astronomy, this was not at all the case in France.
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Though some American astronomers were reluctant to accept that gravitational wave physics is indeed astronomy, this was not at all the case in France.
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Physik in unserer Zeit, 2018
In dem Datensatz des zweiten Messlaufs der beiden LIGO‐Detektoren haben Forscher ein fünftes Gravitationswellensignal gefunden. Es stammt erneut von zwei verschmelzenden Schwarzen Löchern, die mit 12 und 7 Sonnenmassen leichter waren als die bisher nachgewiesenen.
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In dem Datensatz des zweiten Messlaufs der beiden LIGO‐Detektoren haben Forscher ein fünftes Gravitationswellensignal gefunden. Es stammt erneut von zwei verschmelzenden Schwarzen Löchern, die mit 12 und 7 Sonnenmassen leichter waren als die bisher nachgewiesenen.
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1996
1. Stemplės, skrandžio ir žarnyno ligos. J. Šimanauskas6 1. 1. Ūminis ezofagitas6 1. 2. Lėtinis ezofagitas8 1. 3. Lėtinis pepsinis (refliuksinis) ezofagitas10 1. 4. Diafragmos stemplinės angos išvarža12 1. 5. Įskrandžio achalazija16 1. 6. Ūminis gastritas19 1. 7. Lėtinis gastritas23 1. 8. Opaligė28 1. 9. Operuoto skrandžio sindromai37 1. 9. 1. Dempingo
Danilevičius, Juozas Steponas +9 more
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1. Stemplės, skrandžio ir žarnyno ligos. J. Šimanauskas6 1. 1. Ūminis ezofagitas6 1. 2. Lėtinis ezofagitas8 1. 3. Lėtinis pepsinis (refliuksinis) ezofagitas10 1. 4. Diafragmos stemplinės angos išvarža12 1. 5. Įskrandžio achalazija16 1. 6. Ūminis gastritas19 1. 7. Lėtinis gastritas23 1. 8. Opaligė28 1. 9. Operuoto skrandžio sindromai37 1. 9. 1. Dempingo
Danilevičius, Juozas Steponas +9 more
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1996
The most promising anticipated source for the United States Laser Interferometer Gravitational-wave Observatory (LIGO) [1], or its French/Italian counterpart VIRGO [4], is the radiation emitted during the final moments of inspirai before the coalescence of a neutron star — neutron star (ns-ns) binary system [24].
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The most promising anticipated source for the United States Laser Interferometer Gravitational-wave Observatory (LIGO) [1], or its French/Italian counterpart VIRGO [4], is the radiation emitted during the final moments of inspirai before the coalescence of a neutron star — neutron star (ns-ns) binary system [24].
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The status of LIGO installation and commissioning
Classical and Quantum Gravity, 2001Summary: LIGO is engaged in installation and commissioning of three suspended-mass interferometers at observatory sites in Hanford and Livingston. We are commissioning the first instance of any subsystem installed, prior to completion of the entire detector, so we may apply lessons learned to later installations. We have installed all seismic-isolation
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LIGO: Identifying Gravitational Waves
1997We discuss the statistical challenges presented by data from large-scale gravitational-wave interferometers now under construction. Extracting information from signals requires measuring parameters, and sophisticated algorithms may be required to attain maximal possible accuracy.
Schutz, B., Nicholson, D.
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1996
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is being developed to detect gravitational waves emitted from Astrophysical sources. The facility will consist of two widely separated laboratories housing highly sensitive long baseline interferometers using suspended test masses. The technique and status of the project are discussed.
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The Laser Interferometer Gravitational-Wave Observatory (LIGO) is being developed to detect gravitational waves emitted from Astrophysical sources. The facility will consist of two widely separated laboratories housing highly sensitive long baseline interferometers using suspended test masses. The technique and status of the project are discussed.
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2006
Alergija - pakitusi organizmo reakcija į aplinką, kai padidėja jautrumas vienai ar kelioms genetiškai svetimoms organizmui medžiagoms po kartotinio kontakto su jomis. Sergantis alergija žmogus labai jautriai reaguoja į medžiagas, kurios beveik neveikia sveiko žmogaus. Šiandien akivaizdu, kad dėl įvairių priežasčių alergija pasireiškia vis dažniau, ypač
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Alergija - pakitusi organizmo reakcija į aplinką, kai padidėja jautrumas vienai ar kelioms genetiškai svetimoms organizmui medžiagoms po kartotinio kontakto su jomis. Sergantis alergija žmogus labai jautriai reaguoja į medžiagas, kurios beveik neveikia sveiko žmogaus. Šiandien akivaizdu, kad dėl įvairių priežasčių alergija pasireiškia vis dažniau, ypač
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Lightsaber: A Simulator of the Angular Sensing and Control System in LIGO
Galaxies, 2021Jan Harms, Tomislav Andric
exaly