Second submission 1931607640 Assigned ID: 1872 ----- Attempting Submission 1 (Fri Apr 09 11:00:32 GMT 2021) ----- HST Phase I Proposal 1872 successfully submitted. Receipt: # 1872-1 ----- Attempting Submission 2 (Fri Apr 09 21:18:07 GMT 2021) ----- HST Phase I Proposal 1872 successfully submitted. Receipt: # 1872-2 Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. Sensitive exposures should have an ETC run number provided. 0 ----- Attempting Submission 1 (Mon Jul 26 16:10:05 GMT 2021) ----- ----- Attempting Submission 2 (Wed Jul 13 14:46:03 GMT 2022) ----- Jupiter has been successfully observed with this set up many times previously. In September 2021, the highly successful NASA Juno spacecraft will begin its Extended Mission (EM). During the EM, Juno will cross the equatorial region inside of Ganymede's orbit providing an opportunity to obtain HST auroral images simultaneously with high-resolution in situ observations in the crucial inner equatorial region of Jupiter's magnetosphere, where the key dynamics that drive and shape the magnetosphere originate. The STIS/FUV imaging observations proposed here over Cycles 29-31 will answer a large number of outstanding scientific questions, including: * Do magnetosphere-ionosphere coupling currents drive Jupiter's main auroral emission? * What radial forces govern the structure of Jupiter's magnetosphere? * What is the nature of the interaction between Jupiter and its satellites? * How do Jovian plasma populations relate to low latitude auroral emissions? * How does magnetospheric wave activity influence Jupiter's magnetosphere? * What processes give rise to pulsating high-latitude emissions? This program responds to the UV initiative and is only possible during the Juno EM. These observations cannot be made by Juno UVS and HST is the only observatory capable of making these FUV observations, which will yield high-impact results, and complement and extend the goals of the NASA Juno mission. The timescale of the observations required to address the science goals is governed by the orbit of Juno in the EM and covers HST Cycles 29-31; hence our proposal is for a Long Term program of observations. The EM begins in July 2021 and is scheduled nominally to last until August 2025. The availability of Jupiter from HST during Cycles 29-31 is 1 Oct 2021 - 25 Dec 2021; 18 May 2022 - 31 Jan 23; 25 Jun 2023 - 7 March 2024; and 2 Aug 2024 - 30 Sept 2024, where the last date is the assumed end of Cycle 31. Our observations will be clustered around the perijoves, when Juno is in the critical regions of the magnetosphere as described above. Orbit requests are 18 (Cycle 29), 12 (Cycle 30) and 10 (Cycle 31). The orbit request is governed as follows: the science lies in the temporal domain, i.e. variations in the auroral morphology are compared with changes in the in situ field and plasma observations. It is critical that such variation is captured in order to correlate the multiple data sets, and to determine the response to dynamical processes such as solar wind compression events and changing mass loading rates. We hence will use multiple observations for each science goal to capture the key variability that reveals the dynamics of the system. The timescales are: there are typically two ~3- day solar wind compressions per solar rotation (25 days), so the duty cycle for "disturbed" conditions is around 1/4. Thus observing 8 epochs will yield ~2 disturbed intervals, the minimum required to establish repeatable effects. Changes typically take place over a few days. We hence will observe for 2-4 orbits per interval to determine the short-timescale dynamics and to cover both north and south auroras in order to capture the important physics along the entire flux tube. The exact numbers for each interval have been determined by examination of the number of favourable viewing windows for each of the science goals during the 2-3-day intervals surrounding each perijove. We note that there are ~5 SAA-free orbits per day, such that it is possible to observe at least once per day, as has been done successfully previously. For the flybys we will observe as close as possible to the events within the limits of the SAA.These observations will be obtained using the STIS/FUV-MAMA instrument. Auroral images will be obtained using the F25SRF2 filter, in order to observe the H2 Lyman and Werner emission whilst removing contamination from the geocoronal Lyman-alpha. We will observe both northern and southern auroras; the priority will be observing whilst Juno is in the critical regions, rather than focusing on one hemisphere. Jupiter will be positioned using POS_ANGLE (i.e. RAD and ANG) such that only the auroral region and nearby disc will be in the 25x25" field of view, and thus <1/4 of the detector is filled with the planet. This limits the count rates to ~20,000 counts/s, well within the limit of 200,000 counts/s. Observations will be taken in ~3000 s time-tagged exposures, from which images integrated over smaller intervals (e.g. 10-100 s) will be extracted. This setup has been successfully used to observe Jupiter's auroras previously. In the event of STIS not being available, these observations will be obtained with the Solar Blind Channel of the Advanced Camera for Surveys, which in practice yields lower signal to noise than STIS owing to its red leak. In the past, Jupiter observations have been successfully obtained in both 2-gyro and 3-gyro mode. In 2-gyro mode we would remove any roll constraints and we would request our orbit during the interval when Jupiter is available. The investigators on this proposal have unparalleled depth of experience studying the auroras of the outer planets, through HST observations, modelling, and spacecraft data analysis. In particular the team possesses through investigators Nichols, Clarke, Grodent, Bonfond and Gladstone a significant history of HST/FUV observations, and the PI (Nichols) has previously successfully led as PI 7 HST programs of UV observations of Jupiter, Saturn, Ganymede and WASP-12b. The most recent program led by the PI (GO 16195 observing Saturn's FUV auroras) executed in November 2020, with a paper currently in preparation. The team has significant experience of the software and techniques required to reduce and analyse Jupiter HST images, and has an excellent track record of producing world-class, high-impact publications using HST data. In particular the PI has recently re-written the custom-made "Boston University" STIS/ACS auroral image reduction pipeline in Python. The PI will work with the PC to schedule these observations once the orbit is known, and has previously developed software and techniques to accomplish this efficiently. Recent relevant publications led by the PI are numbered 7, 8 and 21 in the bibliography. This proposal is fully supported by the Juno project, as evidenced by the Letter of Support. The PI is a Juno Science Team Member, as are Co-Is Grodent, Bonfond, Cowley, Gladstone, Bagenal and Orton, such that the proposers have the requisite access to the Juno data. Prof. Cowley will provide expertise on the jovian M-I coupling current system and mangetic field measurements, while Prof. Bagenal will provide expertise regarding Juno plasma measurments, Dr Gladstone, Prof. Grodent and Dr Bonfond will provide expertise on Jupiter's auroras, and Dr Orton will provide efficient coordination with the Juno Project. Prof. Lysak will provide expertise in modelling MHD waves. Solar System Astronomy 6 false false true false false false false false SUPPORTED SOLAR SYSTEM YES This target is nominally for imaging Jupiter's southern auroras. Observation criteria are, in order of priority: Time window Avoidance of repeller wire and blotch region For this and all other imaging targets here, the values of RAD and ANG that will centre the auroral region in the relevant half of the detector, away from the repeller wire if possible, will depend in principle on ORIENT (although this is specified in the visit) and the CML range of the observations. We will work with the PC to update these once the orbit of HST is known. If the south is not visible during the SAA free orbits on a given day, we will observe the north or move the visit to a different time window. For the north, the values of ANG will be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 120-220 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23,ANG=155,REF=NORTH NOT CML OF JUPITER FROM EARTH BETWEEN 100 310 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=24,ANG=340,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's southern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the north, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 120-220 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23.0,ANG=152,REF=NORTH NOT CML OF JUPITER FROM EARTH BETWEEN 100 310 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 120-220 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23,ANG=348,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's southern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23.0,ANG=154,REF=NORTH NOT CML OF JUPITER FROM EARTH BETWEEN 100 310 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23,ANG=340,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=355,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=24,ANG=340,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's southern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 120-220 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=25,ANG=160,REF=NORTH NOT CML OF JUPITER FROM EARTH BETWEEN 100 310 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23,ANG=350,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's southern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the north, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 120-220 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=21,ANG=360,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH SOLAR SYSTEM YES This target is for imaging Jupiter's northern auroras. The values of RAD and ANG are dependent on ORIENT and the date and time of the observations. We will work with our PC to update these once the orbit of HST is known. For the south, the values of ANG would be essentially these plus 180 degrees (with minor adjustements to avoid the repeller wire), and the CML range would be 310-100 deg. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=23,ANG=343,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220 EARTH STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 STIS/FUV-MAMA Imaging No No F25SRF2 1657722559533 Using ephemeris for target 16989-19-JUPITER-AURORA-JUNOEM-19 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. Inbound middle magnetopshere, south. We haven't specified an ORIENT range, since we can set RAD and ANG appropriately for any available ORIENT, but as outlined in Phase 1, ORIENT would ideally be as close to 60 as possible to put the disc in the corner of the FOV. 1667712525000 51.0 (Tic-Visit :proposal-id 16989 :visit-id "19" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:29:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "19" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2749 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1657722560277 Using ephemeris for target 16989-20-JUPITER-AURORA-JUNOEM-20 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. This visit is to cover the inner-middle magnetosphere. North. 1667689674000 46.322028671514204 (Tic-Visit :proposal-id 16989 :visit-id "20" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:29:20.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "20" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2749 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1657722562235 Using ephemeris for target 16989-21-JUPITER-AURORA-JUNOEM-21 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. High latitude outbound, south. 1667781083000 55.7423083601808 (Tic-Visit :proposal-id 16989 :visit-id "21" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:29:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "21" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2698 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3091 :pcs-gap 0 ) false 1 0 1657722562992 Using ephemeris for target 16989-22-JUPITER-AURORA-JUNOEM-22 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. This visit is to observe the northern auroras while Juno is inbound in the middle magnetosphere 1671008853000 52.099999999999994 (Tic-Visit :proposal-id 16989 :visit-id "22" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:29:22.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "22" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2698 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3091 :pcs-gap 0 ) false 1 0 1668533029285 Using ephemeris for target 16989-23-JUPITER-AURORA-JUNOEM-23 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. Io flyby, southern aurora. Priority is the southern aurora window near the flux tube crossing near 00h on 15 Dec. If not available due to the SAA, the later we will switch to high latitude south in the following rotation or expand the time interval by a day either side. 1671071552000 62.096359409221094 (Tic-Visit :proposal-id 16989 :visit-id "23" :proposal-version -1 :trans-version "20220630" :date "15-Nov-2022 12:23:49.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1530800 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "23" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2338 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2731 :pcs-gap 0 ) false 1 0 1668533047415 Using ephemeris for target 16989-24-JUPITER-AURORA-JUNOEM-24 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. North, inbound if possible prior to Io flyby in the window beginning ~19h on 14 Dec, otherwise Io flux tube following PJ in the window beginning ~05 h on 15 Dec (depending on SAA and visit 22 availability was) 1671082977000 66.4128082766629 (Tic-Visit :proposal-id 16989 :visit-id "24" :proposal-version -1 :trans-version "20220630" :date "15-Nov-2022 12:24:07.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1530800 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "24" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2338 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2731 :pcs-gap 0 ) false 1 0 1696256747826 Using ephemeris for target 16989-25-JUPITER-AURORA-JUNOEM-25 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. North, middle magnetosphere inbound. 1697310286000 229.16411600062997 (Tic-Visit :proposal-id 16989 :visit-id "25" :proposal-version -1 :trans-version "20230626" :date "02-Oct-2023 10:25:47.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1530800 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "25" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2270 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2713 :pcs-gap 0 ) false 1 0 1696256773110 Using ephemeris for target 16989-26-JUPITER-AURORA-JUNOEM-26 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. 2nd North, middle magnetosphere inbound. If no availaiblity, south in this interval. 1697315986000 229.1914098183462 (Tic-Visit :proposal-id 16989 :visit-id "26" :proposal-version -1 :trans-version "20230626" :date "02-Oct-2023 10:26:12.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1530800 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "26" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2270 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2713 :pcs-gap 0 ) false 1 0 1696256820607 Using ephemeris for target 16989-27-JUPITER-AURORA-JUNOEM-27 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. Ideally start of the northern interval on 22 Jan at 06:18, but if not available we'll shift to the south for the interval post-PJ 1697407155000 265.2371005796533 (Tic-Visit :proposal-id 16989 :visit-id "27" :proposal-version -1 :trans-version "20230626" :date "02-Oct-2023 10:27:00.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1530800 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "27" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2270 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2713 :pcs-gap 0 ) false 1 0 1657722760139 Using ephemeris for target 16989-28-JUPITER-AURORA-JUNOEM-28 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. This visit is to coincide with the Io flyby (north). Ideally within the 2023-07-31 02:51 - 05:37 window as possible. 1690701238000 250.16242782639728 (Tic-Visit :proposal-id 16989 :visit-id "28" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:32:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "28" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2698 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3091 :pcs-gap 0 ) false 1 0 1718989087597 Using ephemeris for target 16989-29-JUPITER-AURORA-JUNOEM-29 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. This visit is to coincide with the Io flyby (south). Ideally the windows starting 2023-07-30 22:10 or 2023-07-31 08:05, but if not available we will move to another window in the north during this window (or expand a day or so either side of necessary). (Tic-Visit :proposal-id 16989 :visit-id "29" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 12:58:07.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1739552 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "29" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2562 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3005 :pcs-gap 0 ) false 1 0 1657722761527 Using ephemeris for target 16989-30-JUPITER-AURORA-JUNOEM-30 The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. North inbound middle magnetosphere 1690632794000 247.5 (Tic-Visit :proposal-id 16989 :visit-id "30" :proposal-version -1 :trans-version "20220516" :date "13-Jul-2022 16:32:41.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 1809136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16989 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16989 :visit-id "30" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2698 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3091 :pcs-gap 0 ) false 1 0