Zobrazeno 1 - 6
of 6
pro vyhledávání: '"W. E. Althouse"'
Publikováno v:
Review of Scientific Instruments. 72:3086-3094
The alignment of the Laser Interferometer Gravitational-Wave Observatory (LIGO) using the global positioning system (GPS) is described. The LIGO project is designed to detect gravitational waves from astrophysical sources by laser interferometry. The
Autor:
Alex Abramovici, W. E. Althouse, Deirdre Shoemaker, J. A. Giaime, F. J. Raab, S. E. Whitcomb, Jordan Camp, L. Sievers, A. Gillespie, D. Durance, Seiji Kawamura, A. Kuhnert, Robert Spero, M. E. Zucker, T. T. Lyons, R. E. Vogt, R. L. Savage, Rainer Weiss
Publikováno v:
Physics Letters A. 218:157-163
Sensitivity enhancements in the laser interferometer gravitational wave observatory (LIGO) project's 40 m interferometer have been achieved through two major instrumental improvements. Improved vibration isolation has reduced the noise due to ground
Autor:
Robert Spero, Michael E Zucker, Seiji Kawamura, W. E. Althouse, Yekta Gursel, Kip S. Thorne, David H. Shoemaker, S. E. Whitcomb, Alex Abramovici, Rainer Weiss, R. W. P. Drever, F. J. Raab, L. Sievers, R. E. Vogt
Publikováno v:
Science (New York, N.Y.). 256(5055)
The goal of the Laser Interferometer Gravitational-Wave Observatory (LIGO) Project is to detect and study astrophysical gravitational waves and use data from them for research in physics and astronomy. LIGO will support studies concerning the nature
Autor:
James H. Trainor, R. M. Joyce, E. C. Stone, W. E. Althouse, Frank B. McDonald, W. D. Davis, R. E. Vogt, T. L. Garrard, A. C. Cummings, D. E. Stilwell
The Voyager Cosmic Ray Experiment includes seven dE/dx- E telescopes to measure the energy and charge of particles of 1 ≤ Z ≤ 26 in the energy range 1-500 MeV/ nucleon and to measure electron energy in the range 3 ≤ E_e ≤ 110 MeV. Isotopic co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3276843e242d9db3ecbc42baac1cadf3
https://resolver.caltech.edu/CaltechAUTHORS:20140414-110553333
https://resolver.caltech.edu/CaltechAUTHORS:20140414-110553333
We describe a new instrument to be flown on ISEE-C which is optimized to measure the isotopic composition of solar and galactic cosmic rays with ~5 to ~250 MeV/nucleon. A mass resolution of ≾ 0.3 AMU should be achieved for all elements with charge
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::85fe99cdce29824f7030e7158e4e220f
https://resolver.caltech.edu/CaltechAUTHORS:20140205-074259302
https://resolver.caltech.edu/CaltechAUTHORS:20140205-074259302
A cosmic ray instrument for NASA's OGO-F spacecraft is described. The experiment consists of three charged particle detector systems which are designed to measure the spectra and chemical composition of galactic and solar cosmic rays over selected en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33cd48bc69a79fe72a991585b7f4baae
https://resolver.caltech.edu/CaltechAUTHORS:20151214-112326236
https://resolver.caltech.edu/CaltechAUTHORS:20151214-112326236