## None ## CCK.four_tops flexible multi-target sequence with up to five
## None ## CCK.scene.flexible Flexible multiwavelength scene.
## None ## RAS.all_images used as an intermediate to call RAS.uvfull and RAS.euvfull
## None ## RAS.dynamics.1x1.all.1 the 30 day plan states that this will be 2 hours at
## None ## RAS.dynamics.1x1.all.2 movie tests, 30 minutes each at 5 wavelengths, try fore/back
## None ## RAS.dynamics.1x1.all.3 movie tests, 60 minutes each at 5 wavelengths, try fore/back
## None ## RAS.dynamics.1x1.all.4 similar to RAS.dynamics.1x1.all.3 but wavelengths interleaved
## 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.euvfull uses general registers to take a set of EUV images
## None ## RAS.euvfullnolinger modified from RAS.euvfull, does not wait for radiation
## None ## RAS.fast171 just a bare bones seq
## None ## RAS.flare_response the response sequence for RAS.dynamics_4
## None ## RAS.limb.1x1.all a movie with wavelengths interleaved, first movie at the limb
## None ## RAS.movie.1x1.1EUV a test movie, we have 8 hours, keep it simple, just Fe XII 195
## 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.test.transient
## None ## RAS.testing.FE1_euvonly take a big picture in each wavelength (5 here) and downlink
## None ## RAS.testing.FE1_sanseuv take a big picture in each wavelength (5 here) and downlink
## None ## RAS.testqs
## None ## RAS.testsnapshots.1x1.all
## None ## RAS.testsnapshots.a take a big picture in each wavelength (8 here) and downlink
## None ## RAS.testsnapshots.b does a 2 hour WL tracking test
## None ## RAS.testsnapshots.c takes UV/WL movies to fill 16 hours, re-target every 30 minutes
## None ## RAS.uvcenterlist uses general registers to take a set of UV images
## None ## RAS.uvfull uses general registers to take a set of UV images
## 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.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
Software Tests RAS.brightest_ar.t1 a proto-type flare sequence
Software Tests RAS.flare.sample1 a proto-type flare sequence
Software Tests RAS.flare1.t1 a proto-type flare sequence
Software Tests RAS.seq_flare.2 a proto-type flare sequence
Software Tests RAS.test.imax.imin I max/I min test, revised and more complicated for
Software Tests RAS.testcomp.long some packing and JPEG tests, intended to ferret out
Software Tests RAS.testcomp.short some packing and JPEG tests, intended to ferret out
Software Tests RAS.wl.flaretest for ground testing of flare flag
1: Active Region CCK.flarewatch1600_uv A sequence for flare observations. With no EUV.
1: Active Region CJW.wlflareresponse flare response for ,CJW.wlflarewatch no EUV allowed
1: Active Region CJW.wlflarewatch A sequence for white light flare observations. With no EUV.
1: Active Region HPW.flareresp flare response for HPW.flarewatch
1: Active Region HPW.flareresp1600_uv flare response for HPW.flarewatch1600_uv, no EUV allowed
1: Active Region HPW.flareresp195 flare response for HPW.flarewatch
1: Active Region HPW.flarewatch A sequence for flare observations.
1: Active Region HPW.flarewatch A sequence for flare observations.
1: Active Region HPW.flarewatch1600 A sequence for flare observations.
1: Active Region HPW.flarewatch1600_uv A sequence for flare observations. With no EUV.
1: Active Region HPW.flarewatch1600_uv A sequence for flare observations. With no EUV.
1: Active Region HPW.flarewatch195avg A sequence for flare observations.
1: Active Region STD.flarewatch A sequence for flare observations. Modified from HPW.flarewatch
1: Active Region STD.forever195 A sequence for flare observations using only 195.
3: Bright Points CJS.EUV.WLtracking.1x1 at top1, 90 sec. cadence for WL, 45 sec. for 171 interleaved,
5: Calibration CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian
5: Calibration CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center
5: Calibration STD.CDSsynoptic Provide images at all wavelengths on central meridian
5: Calibration STD.CDSsynoptic171 Provide images at all wavelengths on central meridian
5: Calibration STD.CDSsynoptic_uv Provide images at all wavelengths on central meridian
6: Ccd STD.CCDsafe checks for CCD safety
6: Ccd STD.CCDsafe_init initializes counters for CCD safety
7: Chromosphere; 8: ChCJS.UVdynamics.1x1.EUVcontext Obtain a sequence of lyman alpha images at moderate cadence.
15: Emerging Flux CJS.EUV.WLtracking.1x1 at top1, 90 sec. cadence for WL, 45 sec. for 171 interleaved,
17: Flares CCK.flarewatch1600_uv A sequence for flare observations. With no EUV.
17: Flares CJW.wlflareresponse flare response for ,CJW.wlflarewatch no EUV allowed
17: Flares CJW.wlflarewatch A sequence for white light flare observations. With no EUV.
17: Flares HPW.flareresp flare response for HPW.flarewatch
17: Flares HPW.flareresp1600_uv flare response for HPW.flarewatch1600_uv, no EUV allowed
17: Flares HPW.flareresp195 flare response for HPW.flarewatch
17: Flares HPW.flarewatch A sequence for flare observations.
17: Flares HPW.flarewatch A sequence for flare observations.
17: Flares HPW.flarewatch1600 A sequence for flare observations.
17: Flares HPW.flarewatch1600_uv A sequence for flare observations. With no EUV.
17: Flares HPW.flarewatch1600_uv A sequence for flare observations. With no EUV.
17: Flares HPW.flarewatch195avg A sequence for flare observations.
17: Flares STD.flarewatch A sequence for flare observations. Modified from HPW.flarewatch
17: Flares STD.forever195 A sequence for flare observations using only 195.
19: Flows CJS.EUV.WLtracking.1x1 at top1, 90 sec. cadence for WL, 45 sec. for 171 interleaved,
21: Hardware Tests COM.af1_front_al Front Aluminum filter integrity
36: Quiet Sun CJS.EUV.WLtracking.1x1 at top1, 90 sec. cadence for WL, 45 sec. for 171 interleaved,
47: Spicules TDT.trnotsofast Fast fluctuations in the transition region
49: Synoptic BNH.fdm.loop Continuously loop through mosaics until stopped.
49: Synoptic CJS.scene.CDSsynoptic Provide images at all wavelengths on central meridian
49: Synoptic CJS.scene.caldiskcenter.1x1.all Provide images at all wavelengths and darks at disk center
49: Synoptic STD.CDSsynoptic Provide images at all wavelengths on central meridian
49: Synoptic STD.CDSsynoptic171 Provide images at all wavelengths on central meridian
49: Synoptic STD.CDSsynoptic_uv Provide images at all wavelengths on central meridian
49: Synoptic STD.fdm.bulletproof make a full-disk mosaic at selected wavelengths, based
53: Transition Region TDT.trnotsofast Fast fluctuations in the transition region
55: Waves TDT.trnotsofast Fast fluctuations in the transition region