The receivers convert directly a 100 MHz bandwidth to the base band. Each receiver is connected to both a low band antenna and an high band antenna; only one of these can be selected at a time. The 100 MHz signal will be buffered for ~1 sec for Cosmic Ray detection and Transient Processing.

The maximum total bandwidth to be processed will be 32 MHz. Each remote station delivers a single dual polarization beam at 32 MHz, or 8 dual polarization beams at 4 MHz or any combination in between. The resulting output data rate is ~2.5 Gbit/s on the whole. The stations will be located following an exponential distribution in exponential shells with an increment factor of 1.6, up to a maximum baseline of roughly 100 Km. The shells start at 1.2 Km and are elliptical in shape, extending in the North-South direction with an 1.3 axial ratio.