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We estimate efficiency of a conceivable Euro-Asian network (EAN) of gravitational wave (GW) interferometers that might be realized having in mind a plan of construction of third generation interferometer in Novosibirsk region. The quality of network in question is considered on the base of typical numerical criteria of efficiency for detecting GW signals of known structure - radiation of relativistic binary coalescence and rotational instabilities of proto-neutron stars during core collapse. We compare EAN efficiency with two reference networks and choose optimal orientation angle for Novosibirsk detector.