Linked from

The 18 pages that link to Aperture synthesis, each with the reason it gives.

• Radio astronomyRelated: It lets radio arrays resolve fine structure without building a single enormous dish.

• Very Long Baseline InterferometryRelated: VLBI relies on aperture synthesis to turn sparse baseline data into radio images.

• Radio telescopeRelated: Earth’s rotation and antenna baselines let arrays build detailed maps of radio sources.

• Event Horizon TelescopeRelated: The EHT uses Earth’s rotation and changing baselines to fill gaps in its image measurements.

• Angular resolutionRelated: It improves angular resolution by using the distance between instruments as an effective aperture.

• Radio interferometryRelated: Earth rotation and multiple baselines let an array synthesize a much larger aperture.

• Very Large ArrayRelated: Earth’s rotation and antenna positions let the array sample many spatial frequencies.

• Fraunhofer diffractionRelated: The Fourier relationship between aperture distribution and far-field pattern underlies image reconstruction.

• Square Kilometre ArrayRelated: Earth's rotation and many antenna pairs let the array build images from sampled spatial frequencies.

• Astronomical interferometerRelated: Earth rotation and multiple telescope pairs fill spatial-frequency coverage for imaging.

• Atacama Large Millimeter/submillimeter ArrayRelated: ALMA uses this technique to achieve the resolving power of an array spanning kilometers.