The closure of two climate cycles in Jupiter's atmosphere during the Juno era

0 Assigned ID: 3863 ----- Attempting Submission 1 (Sat Oct 22 00:36:54 GMT 2022) ----- FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser The specified GS Acq Scenario is not in the current list of valid scenarios. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser The specified GS Acq Scenario is not in the current list of valid scenarios. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser The specified GS Acq Scenario is not in the current list of valid scenarios. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser The specified GS Acq Scenario is not in the current list of valid scenarios. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser The specified GS Acq Scenario is not in the current list of valid scenarios. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser Resubmit with updated timing info for Visit 8. -2131447032 ----- Attempting Submission 1 (Thu Dec 01 02:11:13 GMT 2022) ----- HST Phase II Proposal 17275 successfully submitted. Receipt: # 17275-1 ----- Attempting Submission 2 (Sat Dec 03 00:06:20 GMT 2022) ----- ----- Attempting Submission 3 (Sat May 27 00:23:40 GMT 2023) ----- ----- Attempting Submission 4 (Thu Aug 17 01:00:10 GMT 2023) ----- ----- Attempting Submission 5 (Thu Sep 21 06:58:51 GMT 2023) ----- ----- Attempting Submission 6 (Wed Aug 07 19:09:23 GMT 2024) ----- Warning: FLASH too low Warning: POS TARG + PATTERN + QUAD placements Flash is not needed for bright extended targets like this (scattered light in PSF wings flashes columns for us). POS TARGs have been used to position the target as close as possible to UVIS center to avoid guide star re-acquisition. We are aware of quad filter edge effects. Orbit Planner warning and Visit Planner warning: These tools were run right before submission. I think the warning is generated because this phase 2 proposal includes "completed" visits. Note: Target 8 has a constraint of CML between 285 and 408. Will this be correctly interpreted? I was not sure how to properly input the numbers because of how longitude wraps past 360. The closure of two climate cycles in Jupiter's atmosphere during the Juno era Two climate cycles on Jupiter---one in the North Equatorial Belt (NEB) and one in the Equatorial Zone (EZ)---have been underway for one and four years, respectively. Conditions in the NEB and EZ now show sudden indications of resolving back to their normal states, urgently requiring new data to characterize the evolution of these climate cycles. In the NEB, the cycle involves a transition from typical globally-distributed convective storms to convective storms erupting only at a specific active longitude. Now, the activity seems to be reverting to a wider longitude range, and characterizing the evolution of this climate cycle may solve questions of how convective styles on Jupiter are related to the volatile abundance in the atmosphere. In the EZ, a dramatic darkening/reddening in 2018 also shows sudden signs of weakening back to the typical white state. Intensified observations as the climate cycle closes are needed to coordinate with Juno observations to provide the first evidence that cloud/haze properties are tied to compositional changes in the deeper sub-cloud region. HST imaging at UV wavelengths provide spectral constraints, in addition to the physical constraints, on the evolution of haze properties by completing temporal sampling of the climate cycle. These HST data will provide broad benefit beyond the proposed study of climate cycles in the EZ and the NEB, by providing visible/UV context imaging for Juno atmospheric microwave scans. As the spacecraft track precesses onto the night side of the planet during Cycle 30, Juno will lose the ability to provide its own visible-wavelength context imaging with JunoCam. Image full disk of Jupiter in a series of filters. Each visit is a single orbit. Visits are either: * carefully timed (and with CML constraints) to image the sub-spacecraft track of Juno during one of its perijove passes, or * loosely timed (but with CML constrained) to image a special "active longitude" that is significant to a climate transition in Jupiter's North Equatorial Belt in late 2022. Visits are: 2 --- Jan 22 2023 --- Juno PJ 48 3 --- Jan 2023 --- NEB active longitude (solar conjunction) 4 --- July 31 2023 --- Juno PJ 53 1,5,6 --- Sep 7 2023 --- Juno PJ 54 + NEB active longitude 7 --- Oct 15 2023 --- Juno PJ 55 + NEB active longitude in single orbit 8 --- Nov 22 2023 --- Juno PJ 56 A set of 3 orbits near PJ 54 will provide coverage of most longitudes on Jupiter. This includes one orbit focused on the stealth superstorm longitude, plus two orbits to cover an expanded range of longitudes for Juno. _____ For 2K subarrays (including Quad-subs), POS TARGS are used to shift Jupiter closer to UVIS center, to enable the same guide stars to be used for the whole orbit. The POS TARGs for the Quad-subs are smaller because of filter edge effects. The offsets are as described in Wong et al. 2020 (ApJS). Michael H. Wong is an experienced user of WFC3/UVIS for giant planet observations. As a member of Juno science team, he will coordinate scheduling with Juno, and curate the HST data to maximize its application to Juno science from the inside of the Juno team. For the wider planetary community, data will be archived at an existing HLSP page developed by Dr. Wong for a prior Juno-supporting WFC3 imaging context program. Glenn Orton is a member of the Juno team and leads the overall Earth-based support observing program. He is also conducting research on Juno MWR and JunoCam data, and supplied MWR data for proposal figures. Shawn Brueshaber is a Juno postdoctoral scholar, researching the "stealth superstorm" in previous Juno and HST data. He will include proposed data in his analysis of the evolving convective activity in the NEB. He has experience with dynamical simulations of giant planet atmospheres as well as terrestrial atmospheric science. Amy Simon is an experienced user of HST and the PI of the OPAL program, which obtains Jupiter observations at an annual cadence. She has substantial experience characterizing and analyzing photometric trends in giant planet atmospheric data, which will be applied to the evolving chromophore haze in the EZ. Solar System Astronomy 3 false false false false false true false false AVAILABLE SOLAR SYSTEM YES Can be expanded to CML betw 160,240 if necessary for scheduling PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 175 240 EARTH SOLAR SYSTEM YES Can be expanded to CML betw 160,240 if necessary for scheduling PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 305 358 EARTH SOLAR SYSTEM YES Can be expanded to CML betw 82,162 if necessary for scheduling PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 99 162 EARTH SOLAR SYSTEM YES If necessary, CML observing window can be shifted to increase scheduling opportunities, but the interval should remain 97-37 = 62 deg after shifting. Any shift may also require CML windows for visits 5 and 6 to be shifted (contact PI to confirm). PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 35 97 EARTH SOLAR SYSTEM YES If necessary, CML observing window can be shifted to increase scheduling opportunities, but the interval should remain 226-164 = 62 deg after shifting. Any shift may also require CML windows for visits 1 and 5 to be shifted (contact PI to confirm). PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 164 226 EARTH SOLAR SYSTEM YES If necessary, CML observing window can be shifted to increase scheduling opportunities, but the interval should remain 352-290 = 62 deg after shifting. Any shift may also require CML windows for visits 1 and 6 to be shifted (contact PI to confirm). PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 290 352 EARTH SOLAR SYSTEM YES 106.69 PJ 55 actual PJ lon 115.30 average 123.92 PJ 55 storm lon See phase I: target +/- 40 deg from 115 W, midway between storm and PJ longitudes. PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 75 155 EARTH SOLAR SYSTEM YES Can be expanded to CML betw 285,434 if necessary for scheduling. (Lonigitude values greater than 360 used to correctly express a continuous longitude range using only 2 numbers) PLANET Jupiter STD=JUPITER CML OF JUPITER FROM EARTH BETWEEN 285 408 EARTH WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N POS-TARG DITHER 0.87 LINE false false 2 46.84 WFC3-UVIS-DITHER-LINE 1

false

1670025567111 Using ephemeris for target 17275-02-JUPITER-PJ48-22-JAN-2023 ephemeris data for target 17275-02-JUPITER-PJ48-22-JAN-2023 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.213 to 24.182. ephemeris interval: 22.334 to 24.336 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. Juno PJ 48 at Earth is 2023-01-22 06:27 (Lon 199.9 W) Closest time with CML = 200 is 2023-Jan-22 08:30 Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1674373122000 64.30000000000001 (Tic-Visit :proposal-id 17275 :visit-id "02" :proposal-version -1 :trans-version "20220630" :date "02-Dec-2022 18:59:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 455632 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "02" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2413 :al-overhead-at-end 0 :internal-dur-at-end 534 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only Request BLADE=A for this exposure only 1670025568489 Using ephemeris for target 17275-03-JUPITER-STORMS-JAN-2023 ephemeris data for target 17275-03-JUPITER-STORMS-JAN-2023 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.213 to 24.182. ephemeris interval: 22.334 to 24.336 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. 1673636191000 63.0 (Tic-Visit :proposal-id 17275 :visit-id "03" :proposal-version -1 :trans-version "20220630" :date "02-Dec-2022 18:59:28.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 455632 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "03" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2413 :al-overhead-at-end 0 :internal-dur-at-end 534 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only Request BLADE=A for this exposure only 1688752335723 Using ephemeris for target 17275-04-JUPITER-PJ53-31-JUL-2023 ephemeris data for target 17275-04-JUPITER-PJ53-31-JUL-2023 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.347 to 24.182. ephemeris interval: 23.120 to 25.121 The scheduling data was generated by CASM 31.0. CASM was run in Phase II mode. Juno PJ 53 at Earth is 2023-07-31 09:46 (Lon 121.9 W) Closest time with CML = 122 is 2023-Jul-31 12:50 Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1690843884000 251.72000000000003 (Tic-Visit :proposal-id 17275 :visit-id "04" :proposal-version -1 :trans-version "20220630" :date "07-Jul-2023 13:52:15.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 703872 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "04" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2462 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only 1692230585261 Using ephemeris for target 17275-01-JUPITER-PJ54A-07-SEP-2023 ephemeris data for target 17275-01-JUPITER-PJ54A-07-SEP-2023 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.347 to 24.214. ephemeris interval: 23.212 to 25.213 The scheduling data was generated by CASM 31.0. CASM was run in Phase II mode. Juno PJ 54 at Earth is 2023-09-07 12:34 (Lon 186 W) Closest time with CML = 186 is 2023-Sep-07 15:40 This visit covers longitudes to the east of the perijove longitude. Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1694265846000 234.88013123439072 (Tic-Visit :proposal-id 17275 :visit-id "01" :proposal-version -1 :trans-version "20230418" :date "16-Aug-2023 17:03:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 703872 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2462 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only 1692230586208 Using ephemeris for target 17275-06-JUPITER-PJ54B-07-SEP-2023 ephemeris data for target 17275-06-JUPITER-PJ54B-07-SEP-2023 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.347 to 24.214. ephemeris interval: 23.212 to 25.213 The scheduling data was generated by CASM 31.0. CASM was run in Phase II mode. Juno PJ 54 at Earth is 2023-09-07 12:34 (Lon 186 W) Closest time with CML = 186 is 2023-Sep-07 15:40 Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1694277251000 234.87958180431048 (Tic-Visit :proposal-id 17275 :visit-id "06" :proposal-version -1 :trans-version "20230418" :date "16-Aug-2023 17:03:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 703872 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "06" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2462 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only 1692230587009 Using ephemeris for target 17275-05-JUPITER-PJ54C+STORMS ephemeris data for target 17275-05-JUPITER-PJ54C+STORMS does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.347 to 24.214. ephemeris interval: 23.212 to 25.213 The scheduling data was generated by CASM 31.0. CASM was run in Phase II mode. Juno PJ 54 at Earth is 2023-09-07 12:34 (Lon 186 W) Closest time with CML = 186 is 2023-Sep-07 15:40 This visit covers longitudes to the west of the perijove longitude, including the stealth superstorm longitude. Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1694254441000 234.8806655064085 (Tic-Visit :proposal-id 17275 :visit-id "05" :proposal-version -1 :trans-version "20230418" :date "16-Aug-2023 17:03:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 703872 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "05" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2462 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only 1695279055417 Juno PJ 55 at Earth is 2023-10-15 11:26 (Lon 106.7 W) Storm lon is 124, average of the two is 115, with closest time at 2023-Oct-15 14:41 Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. 1697201977000 272.6693108290866 (Tic-Visit :proposal-id 17275 :visit-id "07" :proposal-version -1 :trans-version "20230626" :date "20-Sep-2023 23:50:55.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 703872 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "07" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2462 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3136 :pcs-gap 0 ) false 1 0 Request BLADE=A for this exposure only 1723057167848 Using ephemeris for target 17275-08-JUPITER-PJ65-20-SEP-2024 ephemeris data for target 17275-08-JUPITER-PJ65-20-SEP-2024 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 22.347 to 25.213. ephemeris interval: 24.213 to 26.213 The scheduling data was generated by CASM 32.1.1. CASM was run in Phase II mode. /private/var/folders/z9/xhlqthqs1w95pdn5zzb0332h0000gn/T/OPVisit8850918517498693154.xml Juno PJ 65 at Earth is 2024-09-20 03:09 (PJ Lon 8.3 W, EQX Lon 34 W, Occultation Lons 325, 341 W) Closest time with CML in range of 325 W to 8 W is 2024-09-20 5:50-7:00 Visit timing constraint is +/-24 hours (about +/- 2 Jupiter rotations) from PJ time. Can be expanded if necessary for scheduling. (Tic-Visit :proposal-id 17275 :visit-id "08" :proposal-version -1 :trans-version "20240604" :date "07-Aug-2024 11:59:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 455632 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17275 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17275 :visit-id "08" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2413 :al-overhead-at-end 0 :internal-dur-at-end 534 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3005 :pcs-gap 0 ) true 1 0 Request BLADE=A for this exposure only Request BLADE=A for this exposure only