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The Australian SKA Pathfinder (ASKAP) is a next generation radio telescopecurrently under construction in Western Australia. The fast survey speed andwide field of view make it an ideal instrument for blind transients searches.The ASKAP Variable and Slow Transients (VAST) survey is a one of the majorscience programs planned for ASKAP. The scientific goals of VAST include thedetection and characterisation of a wide range of transient and variablephenomena, from gamma-ray burst afterglows to extreme scattering events, ontimescales of 5 seconds or longer.  We describe the data and processing challenges involved in running the VASTreal-time transient detection pipeline. ASKAP will produce 2.5 GB of visibilitydata per second, transformed into one 8GB image cube every 5 seconds. Each cubewill contain approximately twenty 100 megapixel images with 100s of radiosources detected in each epoch. The VAST pipeline will measure and monitor allof these sources, detect variables and transients and generate alerts using theVOEvent framework.  The goal of the VAST Design Study is to develop a prototype pipeline toestablish and demonstrate the functionality of the final ASKAP pipeline. Wegive an overview of the prototype pipeline's functionality, technicalimplementation and current status.

VAST - a real-time pipeline for detecting radio transients and variables on the Australian SKA Pathfinder (ASKAP) telescope