The Japanese Aerospace Exploration Agency (JAXA) EUV spectroscopic mission, EXCEED, will be launched to low-Earth orbit in August 2013. EXCEED's primary mission goal is to simultaneously observe the Jovian aurora and Io plasma torus (IPT) with unprecedented temporal resolution, quasi-continuously (50 min per 100 min orbit) for at least two full months. We propose a multi-wavelength campaign of coordinated observations using HST and NOAO facilities that, together with the observations by EXCEED, provide a unique opportunity to discover how energy is transferred throughout Jupiter's vast, dynamic magnetosphere and its interaction with the solar wind. EXCEED spectral imaging of ion emission lines will reveal temporal and spatial variations in the IPT, to diagnose the dynamics in the inner magnetosphere, and relate the dynamics to Jupiter's auroral intensity and spectra. These novel observations will reveal plasma heating and electron precipitation driven by both local and global disturbances. Coordinated high spatial-resolution HST-STIS images of the UV aurora are essential to reveal the global morphology of the aurora, i.e. to pinpoint where the energy deposited in the upper atmosphere originates in the magnetosphere. Simultaneous visible wavelength observations of the IPT by WIYN will provide the low-energy component of the ion emission spectrum to identify heating and density fluctuations of the local plasma. Coordinated observations of the infrared (IR) aurora by Gemini will reveal the ionospheric heating and cooling in the corresponding auroral regions. These observations will provide a huge, novel science return for a small investment of HST and NOAO observation time. Observations of Jupiter's northern UV auroral emissions will be made over 14 days around Jupiter opposition (6 January 2014). 1 orbit per day over 14 days is required to capture the auroral signatures of solar wind activity and their time-development. During each orbit, two STIS images and one spectrum will be acquired using the STIS/FUV-MAMA detector operating in time-tag mode (in the order image-spectrum-image). The imaging observations are to be made with the SrF2 filter to reject geo-coronal contaminated Lyman-alpha. Spectra will be obtained using the 52x0.5" slit and the G140L grating to produce FUV spectra over the range 1150-1700 A at ~12 A resolution. The observations will focus on the northern auroral region. The field-of-view should be offset northwards to include the northern polar region and to limit the count rate from the planet's disk. The orientation values will be optimised within the available range for each orbit after the more precise orbit timings (and hence CML) are known so that the slit will lie across the auroral region. The STIS images will reveal the auroral morphology on short timescales, while the spectra will be used to measure the colour ratio and derive the auroral electron energy. Orbit requests are optimised for Jupiter CML and supporting Gemini observations, but other times are possible. These can be changed if necessary once HST orbit is better known (e.g. to avoid SAA orbits), through communication with the PC and CS. SOLAR SYSTEM 12 false false 0.0 4.2 false false false SUPPORTED SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 225, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 108 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 110 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 120 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH SOLAR SYSTEM FOV offset towards north pole so slit (centre of FOV) will be aligned on auroral region, and disk emission limited. PLANET PLANET JUPITER STD=JUPITER TYPE=POS_ANGLE,RAD=26,ANG=8,REF=NORTH CML OF JUPITER FROM EARTH BETWEEN 110 220, NOT OLG OF JUPITER FROM EARTH BETWEEN 15 345 EARTH STIS/FUV-MAMA Imaging No No F25LYA STIS/FUV-MAMA Spectroscopic No No G140L 1425 STIS/FUV-MAMA Imaging No No F25LYA Using ephemeris for target 13035-01-JUPITER-NORTH-1 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 filtered images and G140L, 52x0.5 spectra will be taken (image-spectrum-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled here. Final timing, position angle, and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "01" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 14:24:45.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-02-JUPITER-NORTH-2 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "02" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 14:24:47.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-03-JUPITER-NORTH-3 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "03" :proposal-version -1 :trans-version "20131031" :date "26-Nov-2013 12:09:36.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-04-JUPITER-NORTH-4 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "04" :proposal-version -1 :trans-version "20131031" :date "29-Nov-2013 09:36:42.0" :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 1130624 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2665 :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 3000.0 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-05-JUPITER-NORTH-5 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "05" :proposal-version -1 :trans-version "20131031" :date "26-Nov-2013 12:11:59.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-06-JUPITER-NORTH-6 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "06" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:46.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-07-JUPITER-NORTH-7 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "07" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:49.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-08-JUPITER-NORTH-8 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "08" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:52.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-09-JUPITER-NORTH-9 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "09" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:54.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-10-JUPITER-NORTH-10 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "10" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:56.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-11-JUPITER-NORTH-11 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "11" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:58:58.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-12-JUPITER-NORTH-12 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "12" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:59:00.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-13-JUPITER-NORTH-13 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "13" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:59:02.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED. Using ephemeris for target 13035-14-JUPITER-NORTH-14 The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. Observations of Jupiter's northern UV aurora. On each orbit timetag SrF2 images and G140L, 52x0.5 spectra will be taken (image-spectra-image). Timings are restricted by Jupiter CML and optimised for simultaneous GEMINI observations. Other timings are possible if HST orbits cannot be scheduled. Final timing and orientation to be determined with PC/CS once HST orbit is known. (Tic-Visit :proposal-id 13035 :visit-id "14" :proposal-version -1 :trans-version "20120604" :date "09-Jul-2012 13:59:04.0" :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 1269792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13035 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13035 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2721 :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 3229 :pcs-gap 0 ) false 1 0 Activation of the HST observations requires a successful launch and acquisition of data from the JAXA mission EXCEED.