HAWAII MR1
Introduction The '''HAWAII MR1''' is a seafloor imaging system developed by the Hawaii Mapping Research Group (HMRG) in 1991.HAWAII MR1 is short for HIGP (Hawaii Institute of Geophysics and Planetology) Acoustic Wide Angle Imaging Instrument, Mapping Researcher 1.This system is the first to use all-digital signal processing. It has been used in the discovery of several objects and locations of note, examples being the USS ''Yorktown'' and the HMRG Deep.
Description The MR1 system is relatively small and stable, and is towed at a depth of 80 to 100 meters. Because it is not hull-mounted, this data collection system has the ability to withstand rough conditions.The HAWAII MR1 also has the capability to measure and collect bathymetric and backscatter data simultaneously, and record raw acoustic data independently of human supervision. After collecting data, the data can be processed with software available from HMRG.The width of a scan produced by the system varies, depending upon whether it is producing a bathymetry swath or a sidescan swath; the swath while recording bathymetry data is 3.4 times the water depth and the swath while recording sidescan data is 7.5 times the water depth.
Discoveries The HAWAII MR1 was chosen to be used on an expedition headed by Robert Ballard, the person who discovered the RMS ''Titanic''. The goal of the expedition was to find the USS ''Yorktown'', which they did successfully. Ballard said of the sonar, "It was the University of Hawaii mapping team's sonar that enabled us to find it." Bruce Appelgate, at the time director of field operations at HMRG, noted that they were fortunate in finding the ship, as it was at the very edge of the MR1's resolution. The ship was 17,000 feet (5.2 km) underwater.The mapping system was also used in the discovery of the HMRG Deep, the second deepest spot in the world (after the Challenger Deep).
References
External links * Data archive of surveys done with the HAWAII MR1* Hawaii Institute of Geophysics and Planetology homepage