8108( 22) - 12/28/00 11:25 - [ 1] PROPOSAL FOR HUBBLE SPACE TELESCOPE OBSERVATIONS ST ScI Use Only ID: 8108 Version: 22 Check-in Date: 28-Dec-2000 11:24:03 1.Proposal Title: Search for Origin of Supersonic Turbulence Observed in the Upper Equatorial Atmosphere of Jupiter ------------------------------------------------------------------------------------ 2. Proposal For 3. Cycle GO 8 ------------------------------------------------------------------------------------ 4. Investigators Contact? PI: Claude Emerich Universite Paris XI CoI: Dr. Lotfi Ben Jaffel CNRS-Institut d'Astrophysique N CoI: Dr. John Clarke T. University of Michigan N CoI: Dr. Renee Prange CNRS-Institut d'Astrophysique Spatiale N CoI: Dr. Gilda Ballester University of Michigan N CoI: Dr. Randal Gladstone Southwest Research Institute N CoI: Dr. Joel Sommeria Ecole Normale Superieure-Lyon N ------------------------------------------------------------------------------------ 5. Abstract It is now clear that Jupiter, like the Sun, sustains a coronal region at the top of its atmosphere. H-Ly-alpha\ spectra measured by GHRS in the Jovian Ly-alpha\ bulge region, evidenced a non thermal line broadening, implying supersonic atomic motions and variability on a time scale of about one minute. Such an atmospheric turbulence was suggested by Ben Jaffel et al. 1993 to explain the Jovian Ly-alpha\ bulge by an enhancement of the H-Ly-alpha\ resonance cross-section rather than by a local increase of t he H density. Sommeria et al. 1995 proposed then a model of thermospheric circulation reproducing the main characteristics of the bulge and explaining the heating excess observed in the Jovian upper atmosphere. This temperature excess was also explained b y Yelle (1996) invoking heating from gravitational waves dissipation. To put new constraints on these models, and to find out potential alternative explanations, we propose to use STIS to make high- resolution H-Ly-alpha li ne profile maps in four cruci al regions of the planet. Recent cycle 7 STIS auroral observations of J. Clarke et al., demonstrated its capability to provide a wealth of new information on spatial, spectral and scale height distributions, allowing to refine our understanding of the phy si cal processes that drive this highly perturbed region of the Jovian atmosphere, using only a few HST orbits. ------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 2] Observations Description ------------------------ sectionSky-Background Measurements and Proposed Targets: The most complete spatial scan being essential to search for variations of both the line profiles and their relative Doppler shifts, the use of a long slit is greatly preferred. The echelle grating E140H, associated with the long slit 52"* 0.5", should be used to obtain the maximum spatial exploration, combined with a maximum signal to noise ratio and a maximum resolving power (spatially and spectrally). The 25 " * 25 " square field of view of the M AMA detector limits the effective FOV to 25 " times0.5 ". Therefore, using the long slit will finally allow us to split the corresponding FOV into ~eq\ 12 spatial resolution elements of 2"\ * 0.5" providing a spatial coverage ~eq\ 12 times the FOV that w a s obtained with the Large Scientific Aperture of GHRS. It has to be noted that our targets being essentially outside the auroral zones, the usual drawbacks associated with a long aperture (overlap between orders, scattere d light) will generally not conc er n our observations. The longest slit is also desirable to optimize the accuracy of sky-background corrections for observations made near the limb since it allows to simultaneously make measurements inside and just outside the Jovian disc, providing th e exact sky-background emission needed to deduce the genuine Jovian spectra. For these particular observation conditions, the requirement of Shadow Time Measurements conditions to minimize the sky- background pollution is no more necessary. Specific sky- b ackground measurements remain however necessary for the observations made at CML, the slit being then not long enough to simultaneously observe the Jupiter's disc and the sky- background. To get the maximum scientific return, using a minimum of orbits, we propose to observe Ly-alpha\ spectra in 4 crucial regions of the Jovian disk which appear to be the most significant to describe the physics at work in the upper Jovian atmosphere. The 6 f ol lowing science exposures are then requested: o first visit: core of the bulge at CML, within 15-20 degrees of N-S and E-W directions: the CML viewing geometry allows most direct interpretation and will serve as a reference for comparison with similar measurements made with GHRS. o second visit: sky-background o third visit: bulge at limb within 15-20 degrees of N-S and E-W directions: such observations will allow to analyze the supersonic turbulence observed with GHRS as a function of the altitude, to obtain the altitude distribution of the H-Ly- alpha\ emissio n, and then to deduce the H scale height and the corresponding temperatures through radiative transfer calculations. o fourth visit: anti- bulge at limb (same directions and same objectives) o fifth visit: ~eq 20 degrees\ North Latitude near limb (~eq Nor th direction): this observation will be made at longitudes System III corresponding to the the active Northern auroral region, in order to analyze the H-Ly-alpha li ne profiles in these active regions where particular features were detected with our pr ev ious GHRS observations, but only marginally due to the insufficient spatial exploration allowed by the shorter GHRS slit. o sixth visit: ~eq 10 degrees\ South Latitude near limb (~eq North direction): same directions, same objectives as previous targe t (mutatis mutandis) The exposure times will be ~eq20 minutes for CML observations and ~eq50 minutes for observations made near the limb. It has to be emphasised that we do not ask for particular scheduling (near opposition) since the alignments (~eqN-S an d ~eqE-W) are required only within 15-20 degrees of those directions. sectionExpected Signals and Feasibility: The best proof of feasibility for the proposed observations is obviously offered by the nice Jupiter spectra obtained by J.T. Clarke et al. u si ng the STIS instrument during cycle 7 (Figure 3). The exposure times can however be estimated as follows: considering a resolution el ement of 2"\ * 0.5" 1 kR at 1216 Angstrom\ roughly corresponds to 7.5* 10^-14 \ ergs\ cm^- 2 \ s^-1. For a Jovian H Ly-al pha\ line width of the order of 0.15 Angstrom this gives a peak level of about 5.0times10^-13 \ ergs\ cm^-2 \ s^-1 \ ang^-1. The sensitivity of the echelle E140H gratings given in the STIS Handbook is roughly 2.4*10^8 \ counts \ s^-1 pix _lambda^-1 \ pix_ s^-1 for an incident flux of 1 erg cm^-2\ s^-1\ rmang^-1\ arcsec^-2. This leads to an instrumental response of (square)uig\ 7.5times10^-2 counts s^-1 \ kR^-1 per resolution element. The consequent signal to noise ratio corresp onding to an exposure time o f 50 minutes is then S/N (square)uig \ 15 \ kR^-1 per resolution element. A typical bulge intensity of 10 kR will be measured with a S/N (square)uig \ 47, equivalent to the results obtained with GHRS-EchA. Consequently, tak ing into account of the acquisi tions and overheads times, one orbit will be sufficient for each target observed near the limb. Tw o orbits are necessary for the observations made at CML (only 25 minutes being available for dark time observations). The tota l number of orbits necessary t o realize our program is then 8 orbits, including the sky measurements. \input epsf beginfigure 4truecm \epsfxsize=9cm epsfbox/users1/emerich/cycle8_prop/e140h1.ps captionJupiter Spectrum measured by Clarke et al. using STI S (6*0.2 slit, cycle 7). The ex posure time was (square)uig 13 minutes. The spatial integration was made over 0.75" *0.2 ". endfigure Real Time Justification ----------------------- The long slit of 25 "\ is required to optimize the sky corrections (see detailed justification in the paragraph concerning the sky-background measurements). , To minimize the geocoronal background for CML measurements, the observations should be scheduled during shadow time, near Jupiter's opposition. , The bulge observations at CML and the related sky-background measurements should be made consecutively in order to obtain the most similar conditions of observations. HST imagery and/or spectral measuremen ts in the auroral zones would also bring a more global view of the region that is supposed to be the origin of the observed 'bulge' phenomena. If such measurements could be made very close in time to our CML bulge measurements, this would give insight on the expected correlation between auroral and bulge activity., Our study should also benefit from additional data from the D/H investigation program proposed by L. Ben Jaffel et al., and also from comparison with the auroral o bservations proposed by J. Cl a rke et al., R. Gladstone et al., and R. Prange et al. , Comparison of our data with the Lyman series obtained from LYMAN-FUSE (Feldman et al.) will help determining potential contributions of collisional processes to the lines formation. Calibration Justification ------------------------- Additional Comments ------------------- ------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 3] Data Distribution Paper Products: YES Media: 8MM Blocking Factor: 10 Ship To: PI_Address Ship Via: Email: ------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 4] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 1 | TARGET NAME: JUPITER-BULGE-CML ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: PLANET JUPITER LY-ALPHA BULGE AT CENTRAL MERIDIEN ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=0,LAT=0,RAD=71400,POLE_L | AT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | CML OF JUPITER FROM EARTH BETWEEN 70 110 | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on the Central W-LINE(1216.0)=0.15+/-0.1 | Meridian and on the Equator SURF-LINE(1216.0)=2+/-1e-11 | | Ephemeris Uncertainty: 10 KM | Acquisition Uncertainty: 0.1 " | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 5] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 2 | TARGET NAME: GEOCORONAL-BACKGROUND ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: OFFSET GEOCORONAL BACKGROUND MEASUREMENT ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=POS_ANGLE,RAD=24,ANG=70,REF=NORTH | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | W-LINE(1216)=0.030+/-.005 | This observation is aimed at F(1216)=6+/-1e-12 | measuring the H Lyman Alpha line SURF(V) = 5.4+/-.5 | profile of the Sky-Background | emissions (Geocoronal plus | Interplanetary). The scientific | return of this observation could be | improved significantly if the slit | were tangent to the Jovian limb, | enhancing considerably the S/N | measurement of the H Lyman alpha | Jovian limb emission. The planet | being oblate, the offset radius | depends on latitude which in turn | depends on the roll angle of the | spacecraft and then on the date of | observation. As soon as this date is | known, the exact offset coordinates | (RAD and ANG) can be determined. | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 6] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 3 | TARGET NAME: JUP-BULGE-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=270,LAT=0,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(1216.0)=2+/-1e-11 | corresponds to the Jovian Lyman | alpha bulge longitude (~90 D) | Ephemeris Uncertainty: 10 KM | Acquisition Uncertainty: 0.1 " | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 4 | TARGET NAME: JUP-ANTIBLG-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER(LYMAN ALPHA ANTI BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=270,LAT=0,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(V) = 5.3 | corresponds to the Lyman alpha | antibulge longitude(~210 D) | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 7] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 5 | TARGET NAME: JUP-NORTH-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=286,LAT=20,RAD=67500,POL | E_LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(V) = 5.3 | corresponds to active region of | Northern upper atmosphere(~120 D) | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 6 | TARGET NAME: JUP-SOUTH-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=275,LAT=- | 10,RAD=67500,POLE_LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(V) = 5.3 | corresponds to Southern active | region (~100 D) | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 8] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 7 | TARGET NAME: JUP-BULGE-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=90,LAT=0,RAD=67500,POLE_ | LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(V) = 5.3 | corresponds to the Jovian Lyman | alpha bulge longitude(~90 D) | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 8 | TARGET NAME: JUP-ANTIBLG-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA ANTI BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=90,LAT=0,RAD=67500,POLE_ | LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that the target SURF(V) = 5.3 | corresponds to the Jovian Lyman | alpha antibulge longitude(~210 D) | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 9] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 9 | TARGET NAME: JUP-NORTH-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=85,LAT=20,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that target SURF(1216.0)=2+/-1e-11 | corresponds to active region of | Northern upper atmosphere (~120 D). | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 10 | TARGET NAME: JUP-SOUTH-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=85,LAT=- | 10,RAD=67500,POLE_LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML such that target SURF(1216.0)=2+/-1e-11 | corresponds to Southern active | region (~100 D) | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 10] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 11 | TARGET NAME: IO-ACQUISITION ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: PLANET SATELITE IO ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | STD=IO | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | SEP OF IO JUPITER FROM EARTH GT 30" | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.8+/-0.5 | Io acquisition for an onboard SURF(1216.0)=1+/-0.2 | acquisition of Jupiter with 0.1 | arcsec accuracy (spectroscopy with | 0.5 arcsec aperture)- The target may | be changed for any other Galilean | satellites if more convenient. In | that case please check exposure time | and CHECK-BOX size. | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 12 | TARGET NAME: CP1-JUP-BULGE-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=90,LAT=0,RAD=67500,POLE_ | LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~ 180 D such that SURF(V) = 5.3 | the target corresponds to the Jovian | Lyman alpha bulge longitude | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 11] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 13 | TARGET NAME: CP1-JUP-ANTIBLG-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA ANTI BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=90,LAT=0,RAD=67500,POLE_ | LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~ 300 D such that SURF(V) = 5.3 | the target corresponds to the Jovian | Lyman alpha antibulge longitude. | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 14 | TARGET NAME: CP1-JUP-NORTH-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=85,LAT=20,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~205 D such that SURF(1216.0)=2+/-1e-11 | target corresponds to active region | of Northern upper atmosphere. | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 12] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 15 | TARGET NAME: CP1-JUP-SOUTH-LIMB-A ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=85,LAT=- | 10,RAD=67500,POLE_LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on West limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~ 190 D such that SURF(1216.0)=2+/-1e-11 | target corresponds to Southern | active region. | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 16 | TARGET NAME: CP1-JUP-BULGE-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER (LYMAN ALPHA BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=270,LAT=0,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~ 0 D such that the SURF(1216.0)=2+/-1e-11 | target corresponds to the Jovian | Lyman alpha bulge longitude. | Ephemeris Uncertainty: 10 KM | Acquisition Uncertainty: 0.1 " | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 13] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 17 | TARGET NAME: CP1-JUP-ANTIBLG-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: FEATURE OF JUPITER(LYMAN ALPHA ANTI BULGE AT LIMB) ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=270,LAT=0,RAD=67500,POLE | _LAT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(1216.0)=2+/-1e-11 | Aperture centered on East limb of W-LINE(1216.0)=0.15+/-0.1 | Jupiter. CML at ~ 120 D such that SURF(V) = 5.3 | the target corresponds to the Lyman | alpha antibulge longitude. | ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 18 | TARGET NAME: IO-ACQUISITION-BIS ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: PLANET SATELITE IO ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | STD=IO | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | SEP OF IO JUPITER FROM EARTH GT 30" | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.8+/-0.5 | Io acquisition for an onboard SURF(1216.0)=1+/-0.2 | acquisition of Jupiter with 0.1 | arcsec accuracy (spectroscopy with | 0.5 arcsec aperture)- The target may | be changed for any other Galilean | satellites if more convenient. In | that case please check exposure time | and CHECK-BOX size. | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 14] TARGET LIST Solar System Targets ------------------------------------------------------------------------------------------------------------------------------------ TARGET NUMBER: 19 | TARGET NAME: CP1-JUPITER-BULGE-CML ------------------------------------------------------------------------------------------------------------------------------------ TARGET DESCRIPTION: PLANET JUPITER LY-ALPHA BULGE AT CENTRAL MERIDIEN ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 1 | TARGET POSITION LEVEL 2 | STD=JUPITER | TYPE=TORUS,LONG=0,LAT=0,RAD=71400,POLE_L | AT=+90 | ------------------------------------------------------------------------------------------------------------------------------------ TARGET POSITION LEVEL 3 | WINDOWS | | CML OF JUPITER FROM EARTH BETWEEN 70 110 | ------------------------------------------------------------------------------------------------------------------------------------ DATA | COMMENTS | SURF(V) = 5.3 | Aperture centered on the Central W-LINE(1216.0)=0.15+/-0.1 | Meridian and on the Equator SURF-LINE(1216.0)=2+/-1e-11 | | Ephemeris Uncertainty: 10 KM | Acquisition Uncertainty: 0.1 " | ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 15] Visit: 01 Visit Priority: Visit Requirements: BETWEEN 23-Sep-1999 AND 23-Oct-1999 SEQ 01, 02 WITHIN 130 H ON HOLD On Hold Comments: Visit 01 has to be executed only if scheduled before or at opposition (23 Oct 1999), when the brightest Jupiter's limb is on the East side. Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1 month around opposition. Before opposition the brightest limb is the East limb. 2. Exposures 111-112, 121-122, 131-132, 141-142, 151-152 should be made in five consecutive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 111 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 111-112 NON-INT SEQ ION CD P DIFFUSE-CENTER=GEOMETRIC-CENTER 121-122 NON-INT SEQ 131-132 NON-INT SEQ 141-142 NON-INT SEQ 151-152 NON-INT Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 112 JUPITER-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000,WAVECAL=NO 1 31 M GE-CML UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being provided by the H-Lyman alpha geocoronal emission measured in special sky exposures (151, 152). ------------------------------------------------------------------------------------------------------------------------------------ 121 JUP-BULGE-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-B UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 122 JUP-BULGE-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-B UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 131 JUP-NORTH-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M IMB-B UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being given by the H-Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 132 JUP-NORTH-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M IMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 141 JUP-ANTIBLG STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M -LIMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 16] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 142 JUP-ANTIBLG STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M -LIMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 151 GEOCORONAL- STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M BACKGROUND UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 152 GEOCORONAL- STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M BACKGROUND UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 17] Visit: 02 Visit Priority: Visit Requirements: BETWEEN 23-Sep-1999 AND 23-Oct-1999 ON HOLD On Hold Comments: Visit 02 has to be executed only if scheduled before or at opposition (23 Oct 1999) Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1.5 months around opposition. Before opposition the brightest Jovian limb is on the East side. 2. Exposures 211-212, 221-222, 231-232 should be made in three successive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 211 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 211-212 NON-INT SEQ ION CD P DIFFUSE-CENTER=GEOMETRIC-CENTER 221-222 NON-INT SEQ 231-232 NON-INT Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 212 JUPITER-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 31 M SEQ 211-212 NON-INT GE-CML UV-MAM G A Comments: These observations do not need internal wavelength calibration because the slit is positionned in such a way that one part of it is illuminated by the sky, providing a direct and simultaneous wavelength calibration by the H Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 221 JUP-BULGE-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000,WAVECAL=NO 1 19 M IMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 222 JUP-BULGE-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 231 JUP-SOUTH-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 232 JUP-SOUTH-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 18] Visit: 03 Visit Priority: Visit Requirements: BETWEEN 24-Oct-1999 AND 23-Nov-1999 SEQ 03, 04 WITHIN 130 H ON HOLD On Hold Comments: Visit 03 has to be executed only if scheduled after opposition (23 Oct 1999), when the brightest Jupiter's limb is on the West side. Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1 month around opposition. After opposition the brightest limb is the West limb. 2. Exposures 311-312, 321-322, 331-332, 341-342, 351-352 should be made in five consecutive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 311 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 311-312 NON-INT SEQ ION CD P DIFFUSE-CENTER=GEOMETRIC-CENTER 321-322 NON-INT SEQ 331-332 NON-INT SEQ 341-342 NON-INT SEQ 351-352 NON-INT Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 312 JUP-BULGE-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000,WAVECAL=NO 1 31 M IMB-A UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being provided by the H-Lyman alpha geocoronal emission measured in special sky exposures (151, 152). ------------------------------------------------------------------------------------------------------------------------------------ 321 JUP-NORTH-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 322 JUP-NORTH-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 331 JUPITER-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M GE-CML UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being given by the H-Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 332 JUPITER-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M GE-CML UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 341 JUP-ANTIBLG STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M -LIMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 19] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 342 JUP-ANTIBLG STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M -LIMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 351 GEOCORONAL- STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M BACKGROUND UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 352 GEOCORONAL- STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1000000 1 19 M BACKGROUND UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 20] Visit: 04 Visit Priority: Visit Requirements: BETWEEN 24-Oct-1999 AND 23-Nov-1999 ON HOLD On Hold Comments: Visit 04 has to be executed only if scheduled after opposition (23 Oct 1999) Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1.5 months around opposition. After opposition the brightest Jovian limb is on the West side. 2. Exposures 411-412, 421-422, 431-432 should be made in three successive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 411 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 411-412 NON-INT SEQ ION CD P DIFFUSE-CENTER=GEOMETRIC-CENTER 421-422 NON-INT SEQ 431-432 NON-INT Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 412 JUP-BULGE-L STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=200000 1 31 M SEQ 411-412 NON-INT IMB-A UV-MAM G A Comments: These observations do not need internal wavelength calibration because the slit is positionned in such a way that one part of it is illuminated by the sky, providing a direct and simultaneous wavelength calibration by the H Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 421 JUP-SOUTH-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000,WAVECAL=NO 1 19 M IMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 422 JUP-SOUTH-L STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M IMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 431 JUPITER-BUL STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M GE-CML UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 432 JUPITER-BUL STIS/F TIME-TA 52X0.05 E140H 1234 BUFFER-TIME=200000 1 19 M GE-CML UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 21] Visit: 05 Visit Priority: Visit Requirements: Between 22-Jan-2001 and 29-Jan-2001 GROUP 05, 06, 07 WITHIN 130 H On Hold Comments: Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1 month around opposition. After opposition the brightest limb is the West limb. 2. Exposures 511-512, 521-522, 531-532 should be made in three consecutive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 511 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 511-512 NON-INT ION-BIS CD P DIFFUSE-CENTER=GEOMETRIC-CENTER Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 512 CP1-JUPITER STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1860,wavecal=no 1 29 M -BULGE-CML UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being given by the H-Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 521 CP1-JUP-ANT STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 19 M seq 521-522 non-int IBLG-LIMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 522 CP1-JUP-ANT STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 18 M IBLG-LIMB-B UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 531 CP1-JUP-SOU STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 19 M seq 531-532 non-int TH-LIMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 532 CP1-JUP-SOU STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 18 M TH-LIMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 22] Visit: 06 Visit Priority: Visit Requirements: Between 22-Jan-2001 and 29-Jan-2001 On Hold Comments: Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1 month around opposition. After opposition the brightest limb is the West limb. 2. Exposures 611-612, 621-622, 631-632 should be made in three consecutive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 611 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 611-612 NON-INT ION-BIS CD P DIFFUSE-CENTER=GEOMETRIC-CENTER Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 612 CP1-JUP-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1860 1 29 M GE-LIMB-A UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being given by the H-Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 621 CP1-JUP-NOR STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140,wavecal=no 1 19 M seq 621-622 non-int TH-LIMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 622 CP1-JUP-NOR STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 18 M TH-LIMB-A UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 631 CP1-JUP-ANT STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 19 M seq 631-632 non-int IBLG-LIMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 632 CP1-JUP-ANT STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 18 M IBLG-LIMB-A UV-MAM G A Comments: No wave internal calibration is necessary. ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 23] Visit: 07 Visit Priority: Visit Requirements: Between 22-Jan-2001 and 29-Jan-2001 On Hold Comments: Additional Comments: 1. To minimize the geocoronal contribution to the measured signal we require to make all the observations within +/- 1 month around opposition. After opposition the brightest limb is the West limb. 2. Exposures 711-712, 721-722 should be made in three consecutive orbits Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exposure| Target |Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Number | Name |Config| Mode |or FOV |Element |Waveln.| Parameters |Exp| | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 711 IO-ACQUISIT STIS/C ACQ F28X50L MIRROR ACQTYPE=DIFFUSE,CHECKBOX=25, 1 0.2 S SEQ 711-712 NON-INT ION-BIS CD P DIFFUSE-CENTER=GEOMETRIC-CENTER Comments: 1. If the acquisition is done with another Galilean satellite, the exposure time and the CHECK-BOX size should have to be modified. ------------------------------------------------------------------------------------------------------------------------------------ 712 CP1-JUP-BUL STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1860,wavecal=no 1 29 M GE-LIMB-B UV-MAM G A Comments: No wave internal calibration is necessary, the wavelength calibration being given by the H-Lyman alpha geocoronal emission. ------------------------------------------------------------------------------------------------------------------------------------ 721 CP1-JUPITER STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 19 M seq 721-722 non-int -BULGE-CML UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 722 CP1-JUPITER STIS/F TIME-TA 52X0.5 E140H 1234 BUFFER-TIME=1140 1 18 M -BULGE-CML UV-MAM G A ------------------------------------------------------------------------------------------------------------------------------------ 8108( 22) - 12/28/00 11:25 - [ 24] Summary Form for Proposal 8108 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures F28X50LP 52X0.5 52X0.05 ------------------------------------------------------------------------------------------------------------------------------------ Configurations STIS/CCD STIS/FUV-MAMA ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACQ TIME-TAG ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters ACQTYPE=DIFFUSE CHECKBOX=25 DIFFUSE-CENTER=GEOMETRIC-CENTER WAVECAL=NO BUFFER-TIME=200000 BUFFER-TIME=1000000 wavecal=no BUFFER-TIME=1140 BUFFER-TIME=1860 ------------------------------------------------------------------------------------------------------------------------------------ Proposal Category GO ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements BETWEEN 23-Sep-1999 AND 23-Oct-1999 SEQ 01, 02 WITHIN 130 H ON HOLD SEQ 111-112 NON-INT SEQ 121-122 NON-INT SEQ 131-132 NON-INT SEQ 141-142 NON-INT SEQ 151-152 NON-INT BETWEEN 23-Sep-1999 AND 23-Oct-1999 ON HOLD SEQ 211-212 NON-INT SEQ 221-222 NON-INT SEQ 231-232 NON-INT SEQ 211-212 NON-INT BETWEEN 24-Oct-1999 AND 23-Nov-1999 SEQ 03, 04 WITHIN 130 H ON HOLD SEQ 311-312 NON-INT SEQ 321-322 NON-INT SEQ 331-332 NON-INT SEQ 341-342 NON-INT SEQ 351-352 NON-INT BETWEEN 24-Oct-1999 AND 23-Nov-1999 ON HOLD SEQ 411-412 NON-INT SEQ 421-422 NON-INT SEQ 431-432 NON-INT SEQ 411-412 NON-INT Between 22-Jan-2001 and 29-Jan-2001 GROUP 05, 06, 07 WITHIN 130 H SEQ 511-512 NON-INT seq 521-522 non-int seq 531-532 non-int Between 22-Jan-2001 and 29-Jan-2001 SEQ 611-612 NON-INT seq 621-622 non-int seq 631-632 non-int SEQ 711-712 NON-INT seq 721-722 non-int ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements MIRROR E140H ------------------------------------------------------------------------------------------------------------------------------------ Target Names IO-ACQUISITION JUPITER-BULGE-CML JUP-BULGE-LIMB-B JUP-NORTH-LIMB-B JUP-ANTIBLG-LIMB-B GEOCORONAL-BACKGROUND JUP-SOUTH-LIMB-B JUP-BULGE-LIMB-A JUP-NORTH-LIMB-A JUP-ANTIBLG-LIMB-A JUP-SOUTH-LIMB-A IO-ACQUISITION-BIS CP1-JUPITER-BULGE-CML CP1-JUP-ANTIBLG-LIMB-B CP1-JUP-SOUTH-LIMB-A CP1-JUP-BULGE-LIMB-A CP1-JUP-NORTH-LIMB-A CP1-JUP-ANTIBLG-LIMB-A CP1-JUP-BULGE-LIMB-B ------------------------------------------------------------------------------------------------------------------------------------ Wavelengths 1234 ------------------------------------------------------------------------------------------------------------------------------------