## NONE ## CCK.flarewatch1600_uv A sequence for flare observations. With no EUV. ## NONE ## CCK.four_tops flexible multi-target sequence with up to five ## NONE ## CCK.scene.flexible Flexible multiwavelength scene. ## NONE ## CJS.EUV.WLtracking.1x1 at top1, 90 sec. cadence for WL, 45 sec. for 171 interleaved, ## NONE ## CJW.wlflareresponse flare response for ,CJW.wlflarewatch no EUV allowed ## NONE ## CJW.wlflarewatch A sequence for white light flare observations. With no EUV. ## NONE ## COM.af1_front_al Front Aluminum filter integrity ## NONE ## HPW.flareresp flare response for HPW.flarewatch ## NONE ## HPW.flareresp1600_uv flare response for HPW.flarewatch1600_uv, no EUV allowed ## NONE ## HPW.flareresp195 flare response for HPW.flarewatch ## NONE ## HPW.flarewatch A sequence for flare observations. ## NONE ## HPW.flarewatch A sequence for flare observations. ## NONE ## HPW.flarewatch1600 A sequence for flare observations. ## NONE ## HPW.flarewatch1600_uv A sequence for flare observations. With no EUV. ## NONE ## HPW.flarewatch1600_uv A sequence for flare observations. With no EUV. ## NONE ## HPW.flarewatch195avg A sequence for flare observations. ## NONE ## RAS.all_images used as an intermediate to call RAS.uvfull and RAS.euvfull ## NONE ## RAS.dynamics_2 a customizable sequence for smaller fov and fast cadence ## NONE ## RAS.dynamics_3 a customizable sequence for smaller fov and fast cadence ## NONE ## RAS.dynamics_4 a customizable sequence for smaller fov and fast cadence ## NONE ## RAS.flare_response the response sequence for RAS.dynamics_4 ## NONE ## RAS.night_linger checks for night via the $HLZ flag, returns when flag is ## NONE ## RAS.radtest test radiation checker, run through SAA and HLZ ## NONE ## RAS.seq_flare.2 a proto-type flare sequence ## NONE ## RAS.test.transient ## NONE ## RAS.testcomp.long some packing and JPEG tests, intended to ferret out ## NONE ## RAS.testcomp.short some packing and JPEG tests, intended to ferret out ## NONE ## RAS.testqs ## NONE ## RAS.uvcenterlist uses general registers to take a set of UV images ## NONE ## STD.CCDsafe checks for CCD safety ## NONE ## STD.CCDsafe_init initializes counters for CCD safety ## NONE ## STD.dynamics a customizable sequence, handles most single pointing observations ## NONE ## STD.dynamics3 ## NONE ## STD.fast1600 ## NONE ## STD.fast171 ## NONE ## STD.fast195 ## NONE ## STD.fast195v2 ## NONE ## STD.flare1600 flares in 1600, options for EUV response also ## NONE ## STD.flarewatch A sequence for flare observations. Modified from HPW.flarewatch ## NONE ## STD.forever195 A sequence for flare observations using only 195. ## NONE ## STD.radiation.EUV.check checks for radiation in first EUV frame that would be used ## NONE ## STD.responseEUV_for_flare1600 the EUV response sequence, phase one or two ## NONE ## STD.response_for_flare1600 the response sequence, phase one ## NONE ## TDT.any_frames TDT.any_frames.useq ## NONE ## TDT.dummy for making a load of frames only ## NONE ## TDT.dummy17 for making a load of frames only ## NONE ## TDT.dummy2 for making a load of frames only $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $aaz RAS.euvfull uses general registers to take a set of EUV images $aaz RAS.euvfull uses general registers to take a set of EUV images $aaz RAS.euvfull uses general registers to take a set of EUV images $aaz RAS.euvfull uses general registers to take a set of EUV images $aaz RAS.euvfullnolinger modified from RAS.euvfull, does not wait for radiation $aaz RAS.euvfullnolinger modified from RAS.euvfull, does not wait for radiation $aaz RAS.euvfullnolinger modified from RAS.euvfull, does not wait for radiation $aaz RAS.uvfull uses general registers to take a set of UV images $aaz RAS.uvfull uses general registers to take a set of UV images $aaz RAS.uvfull uses general registers to take a set of UV images $aaz RAS.uvfull uses general registers to take a set of UV images $g0 BNH.fdm.loop Continuously loop through mosaics until stopped. $g0 CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center $g0 STD.CDSsynoptic Provide images at all wavelengths on central meridian $g0 STD.CDSsynoptic171 Provide images at all wavelengths on central meridian $g0 STD.CDSsynoptic_uv Provide images at all wavelengths on central meridian $g0==1 CJS.UVdynamics.1x1.EUVcontext Obtain a sequence of lyman alpha images at moderate cadence. $g0==1 CJS.UVdynamics.1x1.EUVcontext Obtain a sequence of lyman alpha images at moderate cadence. $g1 RAS.brightest_ar.t1 a proto-type flare sequence $l3 STD.fdm.bulletproof make a full-disk mosaic at selected wavelengths, based $l3>=20 RAS.limb.1x1.all a movie with wavelengths interleaved, first movie at the limb $l3>=20 RAS.limb.1x1.all a movie with wavelengths interleaved, first movie at the limb @nomove TDT.trnotsofast Fast fluctuations in the transition region ar1 RAS.brightest_ar.t1 a proto-type flare sequence ar1 RAS.flare.sample1 a proto-type flare sequence ar1 RAS.testing.FE1_euvonly take a big picture in each wavelength (5 here) and downlink ar1 RAS.testing.FE1_sanseuv take a big picture in each wavelength (5 here) and downlink ar2 RAS.brightest_ar.t1 a proto-type flare sequence ar3 RAS.brightest_ar.t1 a proto-type flare sequence ar4 RAS.brightest_ar.t1 a proto-type flare sequence named.pos07 CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian named.pos18 CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian named.pos27 CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian named.pos30 CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian qr1 RAS.dynamics.1x1.all.1 the 30 day plan states that this will be 2 hours at top1 RAS.dynamics.1x1.all.2 movie tests, 30 minutes each at 5 wavelengths, try fore/back top1 RAS.dynamics.1x1.all.3 movie tests, 60 minutes each at 5 wavelengths, try fore/back top1 RAS.dynamics.1x1.all.4 similar to RAS.dynamics.1x1.all.3 but wavelengths interleaved top1 RAS.fast171 just a bare bones seq top1 RAS.flare1.t1 a proto-type flare sequence top1 RAS.movie.1x1.1EUV a test movie, we have 8 hours, keep it simple, just Fe XII 195 top1 RAS.test.imax.imin I max/I min test, revised and more complicated for top1 RAS.testsnapshots.1x1.all top1 RAS.testsnapshots.1x1.all top1 RAS.testsnapshots.1x1.all top1 RAS.testsnapshots.a take a big picture in each wavelength (8 here) and downlink top1 RAS.testsnapshots.b does a 2 hour WL tracking test top1 RAS.testsnapshots.c takes UV/WL movies to fill 16 hours, re-target every 30 minutes top1 RAS.testsnapshots.c takes UV/WL movies to fill 16 hours, re-target every 30 minutes top1 RAS.wl.flaretest for ground testing of flare flag top3 RAS.limb.1x1.all a movie with wavelengths interleaved, first movie at the limb