Study 000466: ACRONYM: hh_flare_180x152f This study is to hunt for various flow structures in solar flares. It can also be used for studies of active regions. Target: Active region / Flare Type: scanning raster Field of view: 180"x152" Exposure time: 4.0 s Slit: 2" Step size: 6" Raster Duration: 3m27s Data volume: 3515kbits Lines: O V : detection of TR response at the impulsive phase Fe X : hunting of reconnection inflow Fe XII : hunting of reconnection inflow Fe XIV : study of normal coronal loops with density sensitive pairs Fe XV : study of flare loops in a cooling phase Fe XVI : study of flare loops in a cooling phase Fe XVII : study of flare-loop heating and reconnection outflow Ca XVII : study of reconnection outflow Fe XXIII: study of loop-top hot region and reconnection outflow Fe XXIV : study of loop-top hot region and reconnection outflow The non-thermal velocity component in solar flares is studied by combinations of Fe XXIII and Fe XXIV. Pointing: --------- Active region including those with the potential for flaring Instruction to planners: ------------------------ 1) Center the raster on an expected site in an active region. 2) When flare hunting, adjust the raster repeat for a maximum run-time possible, accounting for the telemetry constraint. Note: ----- The default compression is JPEG75. For a short-time run, the compression parameter should be changed to JPEG85. Warning: -------- None