ESA Data Ontology: ESADO: VLA

Instruments > Solar/Space Observing Instruments > Radio Wave Detectors > VLA

VLA

The Very Large Array (VLA) is operated by the National Radio Astronomy Observary (NRAO), and located in Socorro, New Mexico. The array was officially completed in October 1980, but observations started in 1976 -- although with only a few antennas. The VLA archiving program will preserve all data taken after mid-1976. This radio telescope has three arms with 9 movable antenna's on each of the three arms. Each antenna has a crossection of 25 m. The telescope is operated in four configurations with various lengths of the antenna arms. The maximum antenna seperations for the four VLA configurations are: A-36 km, B-11 km, C-3 km, D-1 km. Hybrid configurations with a long north arm are used to produce a round beam for southern sources (south of -15 degree decination). For the following frequencies full capabilities exist 90, 20, 6, 3.6, 2, 1.3 cm, and the VLA has partial capability at 400 cm. Observers should note that in the years of sunspot maximum, daytime observations at 327 MHz are unlikely to be successful in the smaller configurations because of solar interference, and in the larger configurations because of a disturbed ionosphere. (en)

https://gcmd.earthdata.nasa.gov/kms/concept/d8b6c727-ccd1-407d-9751-95b94136b510

RDF/XML TURTLE JSON-LD Last modified 12/6/20

ESA Data Ontology