LAST CHANGED : 2010/04/06 00:40:09 CRUISE NAME(S) : P6_leg2 (mv1001) CRUISE DATES : 2010/01/05 to 2010/02/10 SHIP NAME : Melville PORTS : Papeete, Tahiti to Valparaiso, Chile CHIEF SCIENTIST : Ruth Curry DATABASE NAME : aship DATA FILES : mv2010_005_78756.raw to mv2010_039_64800.raw STATUS : to do done ------ ----------- averaged [ x ] loaded [ x ] check heading correction [ x ] calibration [ x ] edited [ x ] re-check heading correction [ x ] check editing [ x ] figures [ x ] ready for JASADCP INSTRUMENT : os150 ACQUISITION : PROGRAM : uhdas PING TYPE : nb PARAMETERS : BT : bottom track mode (on or off) SI : sampling interval or averaging period for ensemble (sec) NB : number of bins BL : bin length (m) TD : transducer depth (m) BK : blanking length (m) HO : heading offset applied by DAS (deg) HB : heading bias (deg) CRPH : compensation for roll-pitch-heading, 1:on, 0:off) yy/mm/dd hh:mm:ss BT SI NB BL TD BK HO HB CRPH 2010/01/06 21:57:40 off 300 70 8 5 4 0.00 0.00 0001 HEADING : PRIMARY : gyro CORRECTION : ashtech POSITIONS : gps (specify more detail if available) CALIBRATION : original heading alignment: 0.0 additional rotation 0.44 final transducer angle is (original transducer angle) - (rotate_angle) 0.0 - (0.44) = -0.44 original scale factor 1 additional scale factor 1.007 bot consistent with previous leg COMMENTS : gaps in heading correction dday 13.2 - dday 14.8 dday 21.3 - dday 21.7 dday 32.5 - dday 32.65 OS150 basically doesn't work on station (transducer well usually fills up with air). PROCESSOR : J Hummon #=========================================== reprocessing from scratch to regain data in regions of low scattering. # rsync config from the data directory to here; # modify to have useful paths (1) # make processing directory adcptree.py MV1001_os150nb --datatype uhdas --configbase MV1001 --configpath config (2) # set up control file cd $procdir cat << EOF > q_py.cnt --yearbase 2010 --pingtype nb --cfgbase MV1001 --cruisename MV1001 --instclass os --instname os150 --dbname aship --datatype uhdas --datadir path_to_data/MV1001/raw/os150 --cfgpath $basedir/config --ens_len 300 --ping_headcorr --hcorr_inst ashtech --use_topo4edit --delblks 1 --auto EOF (3) quick_adcp.py --cntfile q_py.cnt --mplplots all --npycalc all (4) check rotation Ashtech gaps -- fix cd cal/rotate # copy file in, edit for this case python hcorr_patch.py # makes newhcorr.ang, newhcorr.asc cp Hcorrplot_script.py Hcorrplot_newhcorr.py # edit, run, look at pictures -- all OK? rotate unrotate.tmp rotate rotate1.tmp cd ../.. quick_adcp.py --yearbase 2010 --use_refsm --steps2rerun \ calib:matfiles --auto --mplplots all --npycalc all ** watertrack ** Number of edited points: 130 out of 139 amp = 0.0001 + 1.0069 (t - 25.4) phase = -0.00 + 0.4212 (t - 25.4) median mean std amplitude 1.0070 1.0069 0.0042 phase 0.4705 0.4212 0.2495 ===> tweak calibration before editing quick_adcp.py --yearbase 2010 --use_refsm --steps2rerun \ rotate:navsteps:calib:matfiles --auto --mplplots all --npycalc all \ --rotate_angle .44 --rotate_amplitude 1.007 ** watertrack ** Number of edited points: 130 out of 139 amp = 0.0001 + 0.9999 (t - 25.4) phase = -0.00 + -0.0187 (t - 25.4) median mean std amplitude 1.0000 0.9999 0.0042 phase 0.0255 -0.0187 0.2495 That's better; now edit (5) edit quick_adcp.py --yearbase 2010 --use_refsm --steps2rerun \ apply_edit:navsteps:calib:matfiles --auto --mplplots all --npycalc all ** watertrack ** Number of edited points: 123 out of 127 amp = 0.0001 + 0.9999 (t - 25.1) phase = -0.01 + -0.0093 (t - 25.1) median mean std amplitude 1.0000 0.9999 0.0042 phase 0.0260 -0.0093 0.2687 review editing ================================= (7) web plots mkdir webpy cp ../MV1001_os75nb/webpy/sectinfo.txt webpy/ quick_web.py --instping os150nb --cruiseid MV1001_os150nb --redo done