LATE CORRECTION - One of the Co-I's was originally omitted because he did not have a MyST account, and then after he created it, I forgot to add him. However, he was listed in the team expertise.
No changes have been made to this proposal other than adding Steven Hill as a Co-I.
This change is important because it could cause confusion for the TAC if there is a person described in the Team Expertise who is not listed as a Co-I.-1293283940Assigned ID: 6076
----- Attempting Submission 1 (Tue Apr 01 01:04:44 GMT 2025) -----
HST Phase I Proposal 6076 successfully submitted.
Receipt: # 6076-1
----- Attempting Submission 2 (Thu Apr 10 09:17:19 GMT 2025) -----
HST Phase I Proposal 6076 successfully submitted.
Receipt: # 6076-2
----- Attempting Submission 3 (Thu Apr 10 09:24:53 GMT 2025) -----
HST Phase I Proposal 6076 successfully submitted.
Receipt: # 6076-3
----- Attempting Submission 4 (Thu Apr 10 22:22:23 GMT 2025) -----
HST Phase I Proposal 6076 successfully submitted.
Receipt: # 6076-4
----- Attempting Submission 5 (Tue Apr 15 21:42:32 GMT 2025) -----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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Unschedulable Visit
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
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
FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser
Unschedulable Visit
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
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
FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser
Unschedulable Visit
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
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
FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browserWe were given permission to use BLADE=A on short (4 sec or less) exposures.
This resubmission includes a new ordering of exposures to limit the number of
extra shutter activations needed to accommodate BLADE=A commands.
For PJs 77 and 88 (1K subs, 15 actual exposures) this leads to an additional 4-5
shutter activations (depending on whether the orbit randomly starts on B or not).
For PJs 78 and 79 (2K subs, 9 exposures) the new sequence leads to only 1-2
extra shutter activations per visit.693456689----- Attempting Submission 1 (Sat Aug 02 01:38:06 GMT 2025) -----
----- Attempting Submission 2 (Wed Aug 13 22:32:56 GMT 2025) -----Error (Visit Planner): Unschedulable Visit --- For now, visits 10-12 do not schedule (Jupiter
visibility window opens 16-Oct-2026, but timing window ends
13-Oct-2026). PC has approved submitting this as-is and waiting to resolve this next
year, when both the Juno orbit may be better known, and you never know if a policy
change might enable a slightly smaller solar exclusion zone.
Warning (Form): FLASH level may be too low --- Light in the extended PSF wings effectively
flashes the detector for us. Please see Fig. 2 and the associated discussion in Wong et al. (2020),
DOI: 10.3847/1538-4365/ab775f
Warning (Form): POS TARG & PATTERN should be used carefully with WFC3 quad filters --- This is
done intentionally to minimize slew distance. Please see Fig. 1 and the associated discussion in
Wong et al. (2020).Simultaneous mapping of ammonia on Jupiter with Juno and HST/WFC3Recent publications have demonstrated that imaging filter ratios at visible wavelengths can measure the spatial variation of ammonia gas on Jupiter. The approach is validated using both small-aperture filtered observations and spectroscopic observations. WFC3/UVIS includes the F645N filter which can enable the same analysis but at state of the art spatial resolution. The method also requires continuum and weak methane-band filters to resolve the degeneracy between ammonia concentration and aerosol screening.
Measuring the spatial variation of ammonia has science value in three broad areas:
1. It traces vertical flows, because ammonia is depleted at high altitude by condensation. High-resolution maps reveal the vertical flows associated with discrete storms and vortices, measure sharp meridional gradients that are blurred in ground-based observations, and detect both causes and effects of moist convection.
2. By independently mapping cloud opacity and ammonia concentration, we can test the hypothesis (seemingly contradicted in recent retrievals) that the upper cloud deck is composed of ammonia ice particles.
3. The bulk abundance of ammonia is a key astrochemical constraint on planet formation, but the strong spatial variation of ammonia is a significant source of error. The proposed data would provide an independent constraint from radio (VLA, Juno) retrievals that include a degeneracy with temperature.
We propose a long-term study that would overlap with Juno passes, providing additional value as context for thermal profiles from radio occultations.Within +/-2 days of each available Juno perijove (PJ), three orbits will be used to target the PJ longitude, the radio occultation ingress longitude, and the egress longitude. When Jupiter's disk is smaller than 40 arcsec, we use 1K subarrays, otherwise 2K subarrays.
Longitude constraints are enforced in the target specs. Timing constraints are enforces in the visit specs.
POS-TARG values are used to move the target closer to detector center to minimize slew distance, while still avoiding quad-filter edge effects.
If orbits do not schedule, we can try several things:
* add POS-TARGs to 2K subs in addition to QUAD-SUBs
* increase POS-TARG offsets, driving the edge of the disk into unusuable regions of quad filters
* dropping some exposures (remove patterns first, then drop filters in order of Phase 1 proposal priority)
* expand date range to +/-3 days (absolute maximum usuable time-offset)The team is fully qualified for the proposed effort:
Mike Wong (PI) is an experienced HST/WFC3 user, and part of the OPAL team. He has mapped cloud properties with filter ratios, and used a UC Berkeley radiative transfer model to interpret the results (see Wong et al. 2023). He remains part of the Juno science team, as a former Participating Scientist. He has led multiple MAST HLSP contributions. He was awarded JWST time to observe Jupiter in Cycle 4, with the observations falling between the PJ 79 and 88 visits proposed here.
Pat Irwin developed the NEMESIS radiative transfer model and applied it to MUSE data (Figures 1 and 3). He has led many papers using HST/WFC3 data, including a recent series of Uranus/Neptune papers that led to his holistic cloud model for their atmospheres.
Steven Hill has been conducting ground-based imaging for several years, using filters very similar to the ones proposed here, to derive ammonia column density variations on Jupiter. He teamed with Pat Irwin on Irwin et al. (2025) to validate his filter ratio analysis published in Hill et al. (2024).
John Rogers has decades of experience interpreting the worldwide body of amateur/citizen astronomer observations of Jupiter and its atmospheric variability. He is a true pioneer of "Long-Term Monitoring." His book (Rogers 1995) remains a primary source for placing updated Jupiter measurements into historical context.
Amy Simon is PI of OPAL, the largest solar-system HST program (by orbit number) to date. She leads the MAST HLSP node for OPAL, and she publishes multiple planetary atmosphere papers every year using the OPAL dataset.
Victor Tejfel pioneered methods using ground-based visible-wavelength spectroscopy to analyze the spatial variation of ammonia in the 1960s, and has published papers including comparisons with other ground-based observations such as the VLA. He is the Head of the Laboratory of Physics of the Moon and Planets at the Fesenkov Astrophysical Institute in Kazakhstan, which does not have ESA membership. This proposal would represent his first participation in an HST observing program. His ongoing campaign provides a venue to disseminate results from the proposed study.
Gordon Bjoraker leads a ground-based mid-infrared spectroscopic campaign timed to coincide with Juno passes. His data are shown in Fig. 1c. His ongoing campaign provides a venue to disseminate results from the proposed study.
Imke de Pater leads a long-term program to map Jupiter's ammonia distribution in 3 dimensions using the VLA and ALMA. Her ongoing campaign provides a venue to disseminate results from the proposed study.Solar System Astronomy6falsefalsefalsefalsefalsefalseAVAILABLESOLAR SYSTEMYESTarget lon: 101.20PLANETJupiter, centered on PJ77 longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-77-PJ BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-PJ BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-PJ BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-PJ BY CALLISTO FROM EARTH,
SEP OF JUPITER-77-PJ IO FROM EARTH GT 0",
SEP OF JUPITER-77-PJ EUROPA FROM EARTH GT 0",
SEP OF JUPITER-77-PJ GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-77-PJ CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 56.2 146.2EARTHSOLAR SYSTEMYESTarget lon: 41.56PLANETJupiter, centered on Juno radio occultation ingress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-77-INGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-INGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-INGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-INGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-77-INGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-77-INGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-77-INGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-77-INGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN -3.4 86.6EARTHSOLAR SYSTEMYESTarget lon: 249.97PLANETJupiter, centered on Juno radio occultation ingress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-77-EGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-EGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-EGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-77-EGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-77-EGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-77-EGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-77-EGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-77-EGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 205.0 295.0EARTHSOLAR SYSTEMYESTarget lon: 118.45PLANETJupiter, centered on PJ78 longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-78-PJ BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-PJ BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-PJ BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-PJ BY CALLISTO FROM EARTH,
SEP OF JUPITER-78-PJ IO FROM EARTH GT 0",
SEP OF JUPITER-78-PJ EUROPA FROM EARTH GT 0",
SEP OF JUPITER-78-PJ GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-78-PJ CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 73.4 163.4EARTHSOLAR SYSTEMYESTarget lon: 59.05PLANETJupiter, centered on Juno radio occultation ingress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-78-INGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-INGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-INGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-INGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-78-INGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-78-INGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-78-INGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-78-INGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 14.1 104.1EARTHSOLAR SYSTEMYESTarget lon: 266.96PLANETJupiter, centered on Juno radio occultation egress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-78-EGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-EGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-EGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-78-EGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-78-EGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-78-EGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-78-EGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-78-EGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 222.0 312.0EARTHSOLAR SYSTEMYESTarget lon: 137.20PLANETJupiter, centered on PJ79 longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-79-PJ BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-PJ BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-PJ BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-PJ BY CALLISTO FROM EARTH,
SEP OF JUPITER-79-PJ IO FROM EARTH GT 0",
SEP OF JUPITER-79-PJ EUROPA FROM EARTH GT 0",
SEP OF JUPITER-79-PJ GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-79-PJ CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 92.2 182.2EARTHSOLAR SYSTEMYESTarget lon : 79.61PLANETJupiter, centered on Juno radio occultation ingress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-79-INGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-INGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-INGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-INGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-79-INGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-79-INGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-79-INGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-79-INGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 34.6 124.6EARTHSOLAR SYSTEMYESTarget lon: 292.95PLANETJupiter, centered on Juno radio occultation egress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-79-EGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-EGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-EGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-79-EGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-79-EGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-79-EGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-79-EGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-79-EGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 248.0 338.0EARTHSOLAR SYSTEMYESTarget lon: 325.49PLANETJupiter, centered on PJ88 longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-88-PJ BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-PJ BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-PJ BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-PJ BY CALLISTO FROM EARTH,
SEP OF JUPITER-88-PJ IO FROM EARTH GT 0",
SEP OF JUPITER-88-PJ EUROPA FROM EARTH GT 0",
SEP OF JUPITER-88-PJ GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-88-PJ CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 280.5 370.5EARTHSOLAR SYSTEMYESTarget lon: 62.80PLANETJupiter, centered on Juno radio occultation ingress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-88-INGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-INGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-INGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-INGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-88-INGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-88-INGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-88-INGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-88-INGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 17.8 107.8EARTHSOLAR SYSTEMYESTarget lon: 89.50PLANETJupiter, centered on Juno radio occultation egress longitudeSTD=JUPITERNOT ECL P PARTIAL OF JUPITER-88-EGRESS BY IO FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-EGRESS BY EUROPA FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-EGRESS BY GANYMEDE FROM EARTH,
NOT ECL P PARTIAL OF JUPITER-88-EGRESS BY CALLISTO FROM EARTH,
SEP OF JUPITER-88-EGRESS IO FROM EARTH GT 0",
SEP OF JUPITER-88-EGRESS EUROPA FROM EARTH GT 0",
SEP OF JUPITER-88-EGRESS GANYMEDE FROM EARTH GT 0",
SEP OF JUPITER-88-EGRESS CALLISTO FROM EARTH GT 0",
CML OF JUPITER FROM EARTH BETWEEN 44.5 134.5EARTHWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WWFC3/UVISImagingNoNoF645NWFC3/UVISImagingNoNoFQ619NWFC3/UVISImagingNoNoF631NWFC3/UVISImagingNoNoFQ889NWFC3/UVISImagingNoNoFQ727NWFC3/UVISImagingNoNoF673NWFC3/UVISImagingNoNoF395NWFC3/UVISImagingNoNoF502NWFC3/UVISImagingNoNoF275WPOS-TARGDITHER0.725Large dither for fringing artifactsLINEfalsefalse246.84WFC3-UVIS-DITHER-LINE1falseUsing ephemeris for target 18055-01-JUPITER-77-PJThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-10-17 16:46
Deq = 39.0 arcsec, so 1K subs1760587949000279.1533962235876(Tic-Visit
:proposal-id 18055
:visit-id "01"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:50.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "01"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2541
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-02-JUPITER-77-INGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-10-17 16:46
Deq = 39.0 arcsec, so 1K subs1760582269000279.1512854480302(Tic-Visit
:proposal-id 18055
:visit-id "02"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:53.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "02"
:obset-id "02"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "02"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2541
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-03-JUPITER-77-EGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-10-17 16:46
Deq = 39.0 arcsec, so 1K subs1760570964000279.1470700517026(Tic-Visit
:proposal-id 18055
:visit-id "03"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:53.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "03"
:obset-id "03"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "03"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2541
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-04-JUPITER-78-PJThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-11-19 09:16
Deq = 43.1 arcsec, so 2K subs1763629361000271.60861254135904(Tic-Visit
:proposal-id 18055
:visit-id "04"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:54.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "04"
:obset-id "04"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "04"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-05-JUPITER-78-INGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-11-19 09:16
Deq = 43.1 arcsec, so 2K subs1763657616000271.6049371806761(Tic-Visit
:proposal-id 18055
:visit-id "05"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:56.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "05"
:obset-id "05"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "05"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-06-JUPITER-78-EGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-11-19 09:16
Deq = 43.1 arcsec, so 2K subs1763646314000271.6064236966308(Tic-Visit
:proposal-id 18055
:visit-id "06"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:56.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "06"
:obset-id "06"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "06"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-07-JUPITER-79-PJThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-12-22 01:50
Deq = 46.1 arcsec, so 2K subs(Tic-Visit
:proposal-id 18055
:visit-id "07"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:57.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "07"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-08-JUPITER-79-INGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-12-22 01:50
Deq = 46.1 arcsec, so 2K subs(Tic-Visit
:proposal-id 18055
:visit-id "08"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:57.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "08"
:obset-id "08"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "08"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-09-JUPITER-79-EGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2025-12-22 01:50
Deq = 46.1 arcsec, so 2K subs(Tic-Visit
:proposal-id 18055
:visit-id "09"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:57.0"
: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 633488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "09"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2547
:al-overhead-at-end 0
:internal-dur-at-end 267
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-10-JUPITER-88-PJThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2026-10-11 22:14
Deq = 30.9 arcsec, so 1K subs(Tic-Visit
:proposal-id 18055
:visit-id "10"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:58.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "10"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2571
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-11-JUPITER-88-INGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2026-10-11 22:14
Deq = 30.9 arcsec, so 1K subs(Tic-Visit
:proposal-id 18055
:visit-id "11"
:proposal-version -1
:trans-version "20250624"
:date "13-Aug-2025 15:16:59.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "11"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2571
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)false10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625Using ephemeris for target 18055-12-JUPITER-88-EGRESSThe scheduling data was generated by CASM 33.1.CASM was run in Phase II mode.2026-10-11 22:14
Deq = 30.9 arcsec, so 1K subs(Tic-Visit
:proposal-id 18055
:visit-id "12"
:proposal-version -1
:trans-version "20250624"
:date "25-Sep-2025 13:13:58.0"
: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 526016
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18055
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18055
:visit-id "12"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2571
:al-overhead-at-end 0
:internal-dur-at-end 611
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2979
:pcs-gap 0
)true10New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021623New filter, ETC WFC3UVIS.im.2021627New filter, ETC WFC3UVIS.im.2021625