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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
See also
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Radio telescopes
(List) | Individual
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| Interferometers |
- Allen Telescope Array (ATA, California, US)
- Atacama Large Millimeter Array (ALMA, Chile)
- Australia Telescope Compact Array (ATCA, Australia)
- Australian Square Kilometre Array Pathfinder (ASKAP, Australia)
- Canadian Hydrogen Intensity Mapping Experiment (CHIME, Canada)
- Combined Array for Research in Millimeter-wave Astronomy (CARMA, California, US)
- European VLBI Network (Europe)
- Event Horizon Telescope (EHT)
- Giant Metrewave Radio Telescope (GMRT, India)
- Green Bank Interferometer (GBI, West Virginia, US)
- Korean VLBI Network (KVN, South Korea)
- Large Latin American Millimeter Array (LLAMA, Argentina/Brazil)
- Long Wavelength Array (LWA, New Mexico, US)
- Low-Frequency Array (LOFAR, Netherlands)
- MeerKAT (South Africa)
- Molonglo Observatory Synthesis Telescope (MOST, Australia)
- Multi-Element Radio Linked Interferometer Network (MERLIN, UK)
- Murchison Widefield Array (MWA, Australia)
- Northern Cross Radio Telescope (Italy)
- Northern Extended Millimeter Array (France)
- One-Mile Telescope (UK)
- Primeval Structure Telescope (PaST, China)
- Square Kilometre Array (SKA, Australia, South Africa)
- Submillimeter Array (SMA, US)
- Very Large Array (VLA, New Mexico, US)
- Very Long Baseline Array (VLBA, US)
- Westerbork Synthesis Radio Telescope (WSRT, Netherlands)
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Astronomy by
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