KnowraRadio interferometryLinked fromLinked fromThe 17 pages that link to Radio interferometry, each with the reason it gives.All 17Broader topic 1Related 5Narrower topic 9Compared with 2Very Long Baseline InterferometryNarrower topic: VLBI is a form of radio interferometry that extends baselines across large distances.Event Horizon TelescopeNarrower topic: It provides the broader measurement framework behind the array’s observations.Aperture synthesisNarrower topic: Aperture synthesis is the imaging form of radio interferometry.Very Large ArrayNarrower topic: The array uses this technique to act like a much larger telescope.Very Long Baseline ArrayNarrower topic: The VLBA applies this broader method across continent-scale distances.National Radio Astronomy ObservatoryNarrower topic: Interferometry is the core method behind the VLA, VLBA, and ALMA.Square Kilometre ArrayNarrower topic: The array's sensitivity and angular resolution depend on combining signals across its stations.Antony HewishNarrower topic: Hewish’s telescope work grew from the interferometric methods central to Cambridge radio astronomy.Low-Frequency ArrayNarrower topic: LOFAR synthesizes a large effective aperture by correlating signals from geographically separated stations.