Very Long Baseline Array
(VLBA)
(radio interferometer stretching 8000 km)
The Very Long Baseline Array (VLBA)
is an interferometer consisting of 10 25-meter
radio telescopes spread across North America from
Hawaii to the Virgin Islands supporting a maximum
baseline of 5300 miles, i.e., very-long-baseline interferometry (VLBI).
Its control room is in Socorro, New Mexico.
It observes wavelengths from 28 cm to 3 mm
in eight bands plus two narrow longer-wavelength
bands.
It is also used with additional radio telescopes
for longer baselines, known as the HSA (for High-Sensitivity Array).
This gives them angular resolutions
for the shorter wavelengths
as small as fractions of a milliarcsecond.
(observatory,radio,interferometer,NRAO,array,VLBI,distributed)
Further reading:
https://en.wikipedia.org/wiki/Very_Long_Baseline_Array
http://www.vlba.nrao.edu/
https://ui.adsabs.harvard.edu/abs/1984IAUS..110..377K/abstract
https://ui.adsabs.harvard.edu/abs/1988IAUS..128..445F/abstract
https://ui.adsabs.harvard.edu/abs/1988IAUS..129..461R/abstract
https://ui.adsabs.harvard.edu/abs/1991ASPC...19..390N/abstract
https://ui.adsabs.harvard.edu/abs/1994IAUS..158..117N/abstract
https://ui.adsabs.harvard.edu/abs/1994IAUS..158..125D/abstract
https://ui.adsabs.harvard.edu/abs/1995ASPC...82...59N/abstract
https://ui.adsabs.harvard.edu/abs/1995ASPC...82..133W/abstract
https://ui.adsabs.harvard.edu/abs/1995ASPC...82..117B/abstract
https://ui.adsabs.harvard.edu/abs/2000ivsg.conf..155W/abstract
https://ui.adsabs.harvard.edu/abs/2006ASPC..356..109B/abstract
WaveL | Freq | Photon Energy | | |
3mm | 100GHz | 413μeV | begin | Very Long Baseline Array |
28cm | 1.1GHz | 4.5μeV | end | Very Long Baseline Array |
|
Referenced by pages:
angular resolution
Cosmic Lens All-sky Survey (CLASS)
Gould's Belt Distances Survey (GOBELINS)
Mauna Kea
Mauna Kea Observatories (MKO)
MOJAVE
National Radio Astronomy Observatory (NRAO)
Owens Valley Radio Observatory (OVRO)
very-long-baseline interferometry (VLBI)
Index