################################################## ### Magnetic Data Processing on R/V Melville ### ################################################## Description by S.M.Smith, SIO/GDC, January 1995 DATA LOGGING: ------------- Earth total field magnetic data are collected from a Geometrics Mod. 801 Marine Proton magnetometer and logged by program 'mag-log' on the realtime computer (mlvl61). An analogue paper record is also recorded with two pens, one at 100 nT full scale and a second at 1000 nT full scale. Time and magnetic total field value in nanoTesslas from each magnetometer 5.5 second cycle are logged to realtime log file 'MAGinpf'. Once each day the file is timestamped with the date and this MAGinpf.[date] file is transferred to the offline machine for postprocessing. See 'MAGinpf.file.description'. NEAR REALTIME DISPLAY (on mlvl61): --------------------------------- Magnetic total field is displayed in the "Lab-Display' window on the u/w watch terminal and is updated at approximately 1 minute intervals. Profiles of magnetic total field vs time going back for about the last 12 hours can be displayed in a window of the u/w watch terminal by executing program 'profile'(??change name). (program DOget.MAGinpf must be running to make data available to the 'profile??' program.) A profile of the magnetic anomaly (IGRF removed) residuals can also be displayed along track on the Realtime navigation plot. DATA PROCESSING: ---------------- The MAGinpf file is input to program 'MAGconvert' which averages the data for 1 minute intervals and writes a file, 'mag_uwts.[date]'. (See mag_uwts.file.description). This file is passed through program 'uwchek' which checks the file for time gaps and flags consecutive values whose difference exceeds the range specified. The mag_uwts.[date] file is then concatenated with the previous mag_uwts files into a cumulative file, mag_uwts.[CRUISE], which is merged by program 'uwmerg' with navigation, depth and gravity into a binary file, 'uwmrg.[CRUISE]' (see 'uw_merge.description'). The magnetic anomaly is calculated during merging by subtracting the International Geomagnetic Reference Field (IGRF) from the total field value. (The IGRF is calculated by determining the IGRF values at the corners of a one degree square centered on the first point and then interpolating the IGRF on this plane as long as the location of subsequent values stay within the one degree square.) #end