The Very Large Array in New Mexico... is the key to our chances for success.
El Observatorio de Nuevo México... es la clave de nuestro éxito.
VLA The Very Large Array in New Mexico, dark matter, the multiverse hypothesis 12.
El Very Large Array de Nuevo México, materia oscura, la hipótesis del multiverso. Fuente
The Very Large Array (VLA) in New Mexico, United States is one such series of radio telescopes working together as one.
El Very Large Array (VLA), ubicado en Nuevo México (Estados Unidos), es un ejemplo de una serie de radiotelescopios que funciona como un único telescopio.
The Very Large Array (VLA or Karl G. Jansky Very Large Array) is an interferometer radio telescope on the Plains of San Agustin, in New Mexico, named for Karl G. Jansky, the radio engineer who first discovered radio signals from astronomical distances.
29 de agosto de 2017/ Comente La detección del campo magnético de la galaxia se hizo gracias al equipamiento del observatorio astronómico Karl G. Jansky Very Large Array, en las Llanuras de San Agustín en el desierto de Nuevo México.
The Very Large Array in New Mexico - Stock video...
The Very Large Array in Socorro, New Mexico, an interferometric array formed of 27 parabolic dish telescopes.
Otro radiotelescopio muy conocido es el Very Large Array (VLA), en Socorro, Nuevo México.
It was collected from a variety of sources, including NASA (Cape Cañaveral, Ames, Jet Propulsion Laboratory and Arecibo), The Very Large Array, Radio Astronomy and several educational institutions and private collaborators in the USA.
Se recogió de diversas fuentes, incluyendo la NASA (Cabo Cañaveral, Ames, el Jet Propulsion Laboratory y Arecibo), The Very Large Array, el Observatorio Nacional de Radio Astronomía y varias instituciones educativas y colaboradores privados en Estados Unidos.
It recommends priorities for both space- and ground-based programs, and was instrumental in the eventual construction of the Very Large Array.
Recomienda prioridades para los programas basados tanto en el espacio como en tierra, y fue fundamental en la construcción final del Very Large Array.
For example, the Very Large Array has 27 telescopes giving 351 independent baselines at once.
Por ejemplo el Very Large Array tiene 27 telescopios que dan 351 líneas de base independientes.
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