Radio window
From Wikipedia, the free encyclopedia
The radio window is the range of frequencies of electromagnetic radiation that the earth's atmosphere lets through. The wavelengths in the radio window run from about one centimetre to about eleven-metre waves.
Opacity of the Earth's atmosphere
[edit] See also
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Notable radio
telescopes |
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Single dish
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Interferometers
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- Allen Telescope Array (ATA, California, USA)
- Australia Telescope Compact Array (ATCA, Australia)
- Atacama Large Millimeter Array (ALMA, Chile)
- Combined Array for Research in Millimeter-wave Astronomy (CARMA, California, USA)
- European VLBI Network (Europe)
- Giant Metrewave Radio Telescope (GMRT, India)
- Low-Frequency Array (LOFAR, Netherlands)
- Multi-Element Radio Linked Interferometer Network (MERLIN, UK)
- Molonglo Observatory Synthesis Telescope (MOST, Australia)
- One-Mile Telescope (UK)
- Very Large Array (VLA, New Mexico, USA)
- Very Long Baseline Array (VLBA, USA)
- Westerbork Synthesis Radio Telescope (WSRT, Netherlands)
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Under construction
or proposed
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