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We describe the motivation, design and implementation of the CORNISH survey,an arcsecond resolution radio continuum survey of the inner Galactic plane at 5GHz using the Karl G. Jansky Very Large Array (VLA). It is a blind surveyco-ordinated with the northern Spitzer GLIMPSE I region covering 10 deg < l <65 deg and |b| < 1 deg at similar resolution. We discuss in detail the strategythat we employed to control the shape of the synthesised beam across thissurvey that covers a wide range of fairly low declinations. Two snapshotsseparated by 4 hours in hour angle kept the beam elongation to less that 1.5over 75% of the survey area and less than 2 over 98% of the survey. The primescientific motivation is to provide an unbiased survey for ultra-compact HIIregions to study this key phase in massive star formation. A sensitivity around2 mJy will allow the automatic distinction between radio loud and quiet mid-IRsources found in the Spitzer surveys. This survey has many legacy applicationsbeyond star formation including evolved stars, active stars and binaries, andextragalactic sources. The CORNISH survey for compact ionized sourcescomplements other Galactic plane surveys that target diffuse and non-thermalsources as well as atomic and molecular phases to build up a complete pictureof the ISM in the Galaxy.

The Co-ordinated Radio and Infrared Survey for High Mass Star Formation (The CORNISH Survey) - I. Survey Design