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These two instruments work using the same principle, but the Wide Resonance Scanner is used to analyze signals being emitted from ships and structures, while the Narrow Resonance Scanner detects signals being emitted from potential beacons, which may lead into anomalies. There are two types of Resonance Simulators developed so far: wide and narrow.
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That instrument is the Resonance Simulator. Later analysis of this signal showed that neutrino resonances from different sources have different oscillation characteristics and the distance decay effect is negligible, so an instrument was built to record and display the analysis of the received signal. Since then, CONCORD, in conjunction with the Four Empires and the Sisters, have been analyzing these signals and named this type of signal Neutrino Resonance Wave, or NRW for short. It can come from a celestial or a ship: it occurs as long as such neutrinos exist. The sources of these signals are very diverse. Shortly thereafter, people in the parallel universe discovered a special resonance effect that occurs when such neutrinos pass through different objects, an effect that can be recognized as a new kind of signal. The supernova also produced a large number of special neutrinos. In the original EVE universe, the process of probe scanning was to use probes to analyze specific areas, increasing the intensity of the probes by continually narrowing their detection range, and thus eventually locating different celestials, ships, and other objects.ĭuring the supernova event, the parallel universe Echoes emerged.
#WARP STABILIZER WON'T ANALYZE UPDATE#
As scanning is extremely important part of our upcoming Exploration update (early June), we'd like to share a basic introduction of scanning.