Study 000571: Acronym: ar_vel_fast_scan The goal of this study is to track the evolution of plasma velocity in loop footpoints, in order to detect possible periodical up and downflows. Therefore this study is to be repeated over several days. To that end, cadence of about 40 minutes is used, with medium exposure times (30 s) and a sparse scan (4" step). Since we do not know in what footpoints the pulsations could occur, the study features a wide FOV (300"x512"). TARGET: Active Region EXPOSURE TIME: 30s RASTER: Scanning SLIT: 2" STEP SIZE: 4" FOV: 300"x512" RASTER DURATION: 42 min 46 s VOLUME: 86.3 Mbit RATE: 34.5 kbit/s COMPRESSION: DPCM The primary lines for each data window are: 1 180.40 32 # Fe XI 180.401 2 182.10 32 # Ca XV 181.900, Fe XI 182.167, Fe X 182.310 3 184.33 32 # O VI 184.117, Fe X 184.536 4 185.21 80 # Fe VIII 185.213 186.75 32 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880 5 188.40 48 # Ar XIV 187.964, Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675 6 192.47 56 # Fe XXIV 192.040, Fe XII 192.394, Fe XI 192.813, Ca XVII 192.858, O V 192.906 7 194.10 40 # Fe X 193.715, Ca XIV 193.874, Ar XIV 194.396 8 195.12 24 # Fe XII 195.119, Fe XII 195.179 9 197.86 24 # Fe IX 197.862 10 201.05 24 # Ca XV 200.972, Fe XIII 201.121 11 202.04 24 # Fe XIII 202.044 12 203.83 24 # Fe XII 203.720, Fe XIII 203.826 13 208.50 32 # Ca XV 208.324, Ca XVI 208.604, Fe XIII 208.679, Ca XV 208.722 14 211.32 24 # Fe XIV 211.316 15 255.00 32 # Fe XVII 254.87, Fe XXIV 255.100 16 256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686 17 258.37 24 # Si X 258.375 18 262.98 24 # Fe XVI 262.984 19 264.30 72 # Fe XXIII 263.760, S X 264.233, Fe XIV 264.787, Fe XVI 265.003 20 270.52 24 # Mg VI 270.394, Fe XIV 270.519 21 275.40 24 # Si VII 275.368, Fe XVII 275.54 22 276.30 40 # Mg VII 276.153, Mg V 276.579 23 278.40 32 # Mg VII 278.402, Si VII 278.445 24 280.39 56 # Mg VII 280.39, O IV 279.933 25 284.16 24 # Al IX 284.015, Fe XV 284.160 Pointing: --------- The FOV should contain a full bundle of loops (including both footpoint regions). In addition, a quiet Sun region at the top or bottom of the FOV would be very helpful for the velocity calibration. Instructions to planners: ------------------------- Repeat the study run if more TM become available Info. to be added. Warning: ------- 4" steps are taken between exposures (sparse raster)