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VLBA
antennas are capable of observing at ten different wavelengths. The feeds
are sized according to the length of the wave being reflected into them.
The sizes available on these antennas, along with the frequency of the
wave observed are:
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Wavelength
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Frequency
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90 cm*
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327 MHz
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50 cm*
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610 MHz
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20 cm
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1.5 GHz
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13 cm
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2.3 GHz
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6 cm
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4.8 GHz
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4 cm
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8.4 GHz
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2 cm
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14 GHz
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1.3 cm
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23 GHz
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7 mm
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43 GHz
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3 mm
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86 GHz
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*In the middle of the subreflector
is a dipole antenna for observing at 90 cm and 50 cm. The wave
bounces from the dish directly to this UHF antenna.
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On the feed housing small heating elements focus on the apertures to
prevent the formation of ice crystals. St. Croix is the only antenna
that does not have heaters.
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Using this special setup of
dichroic and ellipsoid, the antenna can observe at two
frequencies simultaneously. The dichroic allows 13cm waves to
pass through to the 13cm aperture, while the remainder of the
waves are reflected to the ellipsoid (which is retracted in this
photo). The ellipsoid, in turn, bounces the 4cm waves into the
4cm aperture.
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Modified on
Friday, 26-Sep-2008 12:15:34 MDT
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