! File: 3937C.PROP ! Database: PEPDB ! Date: 20-FEB-1994:00:46:04 coverpage: title_1: LY-ALPHA AND H2 SURVEY -- CYCLES 2,3 sci_cat: SOLAR SYSTEM proposal_for: GTO/HRS cont_id: 1202 pi_fname: LAURENCE pi_mi: M. pi_lname: TRAFTON pi_inst: TEXAS, UNIVERSITY OF pi_country: USA pi_phone: (512) 471-1476 keywords_1: LY-ALPHA, UV SPECTRA, UV EMISSION, PLANETARY keywords_2: ATMOSPHERES hours_pri: 13.40 hours_par: 4.00 num_pri: 12 num_par: 1 realtime: X time_crit: X pi_position: RESEARCH SCIENTIST ! end of coverpage abstract: line_1: Measure the Ly-alpha emission and the Lyman and Werner H2 emission for Jupiter, line_2: Saturn, Titan, Uranus and Neptune for a low - and medium - resolution survey line_3: and comparative study. Calibrate the superposed geocoronal Ly-alpha background line_4: emission in parallel HRS observations. Search for emissions for line_5: aeronomical species generated by ion chemistry in the intense line_6: auroral emissions (such as species recently detected in the 2 - 4 micron line_7: aurora of Jupiter). Search for HD emission in order to evaluate the line_8: D/H ratio with the aid of the H2 bands. Perform an overall comparative line_9: study of the aurorae in reducing atmospheres, including a comparative line_10: study of their magnetospheric excitation processes. ! ! end of abstract general_form_proposers: lname: TRAFTON fname: LAURENCE mi: M. inst: TEXAS, UNIVERSITY OF country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Observe Titan, Uranus and Neptune at 1456 - 1774A and 1072 - 1360A with the HRS line_2: low/medium resolution modes and large science aperture within 3 months of line_3: opposition. Make similar observations of line_4: Saturn's disk center (excluding Rings and its shadow) and Northern aurora. line_5: Make similar observations of line_6: Jupiter's equatorial region at LambdaIII (1965) = 100d and 280d and Jupiters's line_7: northern aurora near LambdaIII (1965) = 180d. The FOC will be needed to locate line_8: auroral "hot spot" and for HRS acquisition of it. Parallel observations, line_9: including the use of the HRS when another instrument is prime and looking near line_10: one of these planets are needed to calibrate the background geocoronal line_11: Ly-alpha emission. line_15: PRIORITY = 1. ! question: 4 section: 1 line_1: 1100 - 1360A required line_2: spatial resolution required ! question: 5 section: 1 line_1: FOC or WF/PC image at Ly-alpha needed to locate auroral emission on Jupiter line_2: and Uranus and to point HRS to it. line_3: Obs. between quad. and opp. needed to min. geocoranal background emission line_4: (dark time). line_5: Certain central meridian longitudes of Jupiter and Saturn are needed. line_6: Tracking of auroral features need (planetary rotation). line_7: Geocoronal calibrations should match Sun-Earth-Planet observing geometry as line_8: much as possible (dayglow not equal to night emission) line_9: [automatic if observation is made close in time to planet observtion]. ! question: 6 section: 1 line_1: see (5) for geocoronal- calibration parallel observations and dark-time line_2: requirements. The geocorona is bright and superposes the planetary Ly-alpha line_3: emissions at low spectral resolution. It needs to be known in order to subtract line_4: it. It is dimmer at night and so dark time observations have weaker geocoronal line_5: contamination; better accuracy is achieved. It varies with Sun-Earth-Planet line_6: angle so each planet observations requires a geocoronal spectrum. line_7: Max. Doppler shift of geocorona occurs at quadrature. ! question: 7 section: 1 line_1: Initial reductions at STScI; line_2: Final reductions and analysis at Univ. Texas at Austin using our VAX 11/780 and line_3: Sun 4 Sparcstation ! question: 8 section: 1 line_1: Request geocoronal calibrations to be parallel-mode observations at no charge line_2: when another instrument is prime and looking at planets [or a big vicinity line_3: (~10d) around a planet we observed] within a month of my planet observation. line_5: Need FOC to acquire and locate emissions in auroral regions of Jupiter and line_6: Saturn. ! question: 10 section: 1 line_1: Cluster of VAX 11/780's and 6410. line_2: Sun 4 Sparcstation ! question: 13 section: 1 line_1: A low and medium resolution Ly-alpha and H2 emission survey for Jupiter, Saturn line_2: Titan, Uranus and Neptune, will be attempted using the HRS for comparative line_3: auroral studies. ! !end of general form text general_form_address: lname: TRAFTON fname: LAURENCE mi: M. category: PI inst: TEXAS, UNIVERSITY OF addr_1: ASTRONOMY DEPT. addr_2: RLM 16.326 city: AUSTIN state: TX zip: 78712 country: USA phone: (512) 471-1476 ! ! end of general_form_address records ! No fixed target records found solar_system_targets: targnum: 1 name_1: URANUS descr_1: FEATURE URANUS lev1_1: STD = URANUS, ACQ = 0.1 lev2_1: TYPE = CARTO, lev2_2: LONG = 62, lev2_3: LAT = +31 comment_1: OBSERVE AURORAL EMISSION NEAR MAGNET comment_2: IC POLE. LONGITUDE SYSTEM IS THAT OF comment_3: NESS ET AL 1986(SCIENCE 233, 85-89). comment_4: SEE CONNERNEY ET AL 1987, JGR 92 comment_5: (A13), 15329-36. fluxnum_1: 1 fluxval_1: V=5.7,TYPE=G2V fluxnum_2: 2 fluxval_2: SURF(1216)=3.1E-12 fluxnum_3: 3 fluxval_3: W-LINE(1216)=0.01 fluxnum_4: 4 fluxval_4: SURF-BKG(1216)=7.6E-12 fluxnum_5: 5 fluxval_5: SURF(1600)=2.3E-14 ! targnum: 2 name_1: NEPTUNE descr_1: PLANET NEPTUNE lev1_1: STD = NEPTUNE, ACQ = 0.1 comment_1: OBSERVE AURORAL EMMISION NEAR POLE. fluxnum_1: 1 fluxval_1: V=7.7,TYPE=G2V fluxnum_2: 2 fluxval_2: SURF(1216)=1.6E-12 fluxnum_3: 3 fluxval_3: W-LINE(1216)=0.01 fluxnum_4: 4 fluxval_4: SURF-BKG(1216)=7.6E-12 fluxnum_5: 5 fluxval_5: SURF(1600)=2.2E-14 fluxnum_6: 6 fluxval_6: F(1800) = 1.3E-15 ! targnum: 3 name_1: TITAN descr_1: SATELLITE TITAN lev1_1: STD = SATURN lev2_1: STD = TITAN wind_1: SEP OF SATURN TITAN FROM EARTH GT 40" comment_1: OBSERVE TITAN'S AIRGLOW. fluxnum_1: 1 fluxval_1: V=8 fluxnum_2: 2 fluxval_2: SURF(1216)=6.1E-13 fluxnum_3: 3 fluxval_3: W-LINE(1216)=0.01 fluxnum_4: 4 fluxval_4: SURF-BKG(1216)=7.6E-12 ! targnum: 4 name_1: SATURN-CENTER descr_1: PLANET SATURN lev1_1: STD = SATURN comment_1: OBSERVE CENTER OF SATURN (EXCLUDING comment_2: THE RINGS) fluxnum_1: 1 fluxval_1: V=-0.4 fluxnum_2: 2 fluxval_2: SURF(1216)=9+/-3E-12 fluxnum_3: 3 fluxval_3: W-LINE(1216)=0.01 fluxnum_4: 4 fluxval_4: SURF-BKG(1216)=7.6E-12 fluxnum_5: 5 fluxval_5: SURF(1600)=2.6E-15 ! targnum: 5 name_1: SATURN-NPR descr_1: FEATURE SATURN lev1_1: STD = SATURN lev2_1: TYPE = TORUS, lev2_2: LONG = 0, lev2_3: POLE_LAT = +90, lev2_4: LAT = +90, lev2_5: RAD = 54460 comment_1: OBSERVE SATURN'S NORTHERN AURORA. comment_2: ANY LONGITUDE IS ACCEPTABLE SINCE THE comment_3: MAGNETIC POLE NEARLY comment_4: COINCIDES WITH THE SPIN POLE. fluxnum_1: 1 fluxval_1: V=-0.4 fluxnum_2: 2 fluxval_2: SURF(1216)=12E-12 fluxnum_3: 3 fluxval_3: W-LINE(1216)=0.01 fluxnum_4: 4 fluxval_4: SURF-BKG(1216)=7.6E-12 fluxnum_5: 5 fluxval_5: SURF(1600)=5E-15 ! targnum: 10 name_1: TITAN-ACQ descr_1: SATELLITE TITAN lev1_1: STD = SATURN lev2_1: STD = TITAN wind_1: SEP OF SATURN TITAN FROM EARTH LT 135", wind_2: SEP OF SATURN TITAN FROM EARTH GT 20" comment_1: ACQUIRE TITAN AND COMPARE PREDICTED comment_2: VS ACTUAL COORDINATES(ONBOARD). comment_3: USE DIFFERENCE TO ACQUIRE SATURN. fluxnum_1: 1 fluxval_1: V=8 ! targnum: 11 name_1: GEOCORONA-3 descr_1: OFFSET URANUS lev1_1: STD = URANUS, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF URANUS' ORBIT. THIS IS A comment_4: CALIBRATION OF THE GEOCORONA FOR THE comment_5: URANUS OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! targnum: 12 name_1: GEOCORONA-5 descr_1: OFFSET URANUS lev1_1: STD = URANUS, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF URANUS' ORBIT. THIS IS A comment_4: CALIBRATION OF THE GEOCORONA FOR THE comment_5: 2ND URANUS OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! targnum: 13 name_1: GEOCORONA-9 descr_1: OFFSET NEPTUNE lev1_1: STD = NEPTUNE, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF NEPTUNE'S ORBIT. THIS IS comment_4: A CALIBRATION OF THE GEOCORONA FOR comment_5: THE NEPTUNE OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! targnum: 14 name_1: GEOCORONA-11 descr_1: OFFSET SATURN lev1_1: STD = SATURN, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF SATURN'S ORBIT. THIS IS comment_4: A CALIBRATION OF THE GEOCORONA FOR comment_5: A SATURN OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! targnum: 16 name_1: GEOCORONA-21 descr_1: OFFSET TITAN lev1_1: STD = SATURN, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF SATURN'S ORBIT. THIS IS comment_4: A CALIBRATION OF THE GEOCORONA FOR comment_5: A TITAN OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! targnum: 17 name_1: GEOCORONA-53 descr_1: OFFSET SATURN lev1_1: STD = SATURN, ACQ = 3600 comment_1: OBSERVE SUCCESSIVE SEGMENTS OF THE comment_2: NIGHT GEOCORONA PROJECTED ALONG THE comment_3: VICINITY OF SATURN'S ORBIT. THIS IS comment_4: A CALIBRATION OF THE GEOCORONA FOR comment_5: A SATURN OBSERVATION. comment_6: THIS IS A PARALLEL TARGET. fluxnum_1: 1 fluxval_1: SURF(1216)=1.6E-6 fluxnum_2: 2 fluxval_2: W-LINE(1216)=0.01 ! ! end of solar system targets ! No generic target records found exposure_logsheet: linenum: 1.000 targname: URANUS config: PC opmode: IMAGE aperture: P6 sp_element: F439W wavelength: 4353 num_exp: 1 time_per_exp: 20S s_to_n: 70 fluxnum_1: 1 priority: 1 req_1: CYCLE 2 /1-9; req_2: SEQ 1-5 NO GAP; req_3: INT ACQ FOR 2-5; req_4: AT 5-OCT-92 +/- 25D; req_5: GUID TOL 0.025" ! linenum: 2.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 30S priority: ^ req_1: CALIB FOR 3; req_2: DARK TIME / 1,3,3.1,5,5.1,9,9.1; req_3: SEQ 2,3 NON-INT ! linenum: 3.000 targname: URANUS config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: ^ param_1: FP-SPLIT=STD, param_2: STEP-TIME=1.0 ! linenum: 3.100 targname: URANUS config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 5 time_per_exp: 10M fluxnum_1: 2 priority: ^ param_1: FP-SPLIT=STD, param_2: STEP-TIME=1.0 req_1: SEQ 3,3.1 NO GAP; req_2: COND IF TAC ! linenum: 4.000 targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 30S priority: ^ req_1: CALIB FOR 5; req_2: SEQ 4,5 NON-INT ! linenum: 5.000 targname: URANUS config: ^ opmode: ^ aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: ^ param_1: STEP-TIME=1,FP-SPLIT=STD ! linenum: 5.100 targname: URANUS config: ^ opmode: ^ aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 6 time_per_exp: 10M fluxnum_1: 2 priority: ^ param_1: STEP-TIME=1,FP-SPLIT=STD req_1: SEQ 5,5.1 NO GAP; req_2: COND IF TAC ! linenum: 7.000 targname: INTFLAT config: HRS opmode: ACCUM aperture: 2.0 sp_element: SAFE2 wavelength: ^ num_exp: 1 time_per_exp: 7S priority: ^ req_1: CALIB FOR 5 ! linenum: 7.500 targname: NEPTUNE config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S fluxnum_1: 1 priority: 1 param_1: LOCATE=NO, param_2: FAINT=400, param_3: BRIGHT=8600, param_4: SEARCH-SIZE=5 req_1: ONBOARD ACQ FOR 7.6; req_2: DARK TIME / 7.5-7.7,9 ! linenum: 7.600 targname: NEPTUNE config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 74S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 7.7,8,9 comment_1: STEP-TIME= 1.6 SEC ! linenum: 7.700 targname: NEPTUNE config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 194S fluxnum_1: 1 priority: 1 comment_1: STEP-TIME= 0.4 SEC ! linenum: 8.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC1 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 30S priority: 1 req_1: CALIB FOR 9; req_2: SEQ 8,9 NON-INT ! linenum: 9.000 targname: NEPTUNE config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 20M fluxnum_1: 2 priority: 1 param_1: STEP-TIME=1,FP-SPLIT=STD req_1: SEQ 7.5-9 NO GAP; req_2: AT 9-OCT-92 +/- 25D; ! linenum: 9.100 targname: NEPTUNE config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 8 time_per_exp: 20M fluxnum_1: 2 priority: 1 param_1: STEP-TIME=1,FP-SPLIT=STD req_1: SEQ 9,9.1 NO GAP; req_2: COND IF TAC ; req_3: CYCLE 2 ! linenum: 10.000 targname: TITAN-ACQ config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S fluxnum_1: 1 priority: 2 param_1: BRIGHT=3300, param_2: FAINT=280, param_4: SEARCH-SIZE=5 req_1: ONBOARD ACQ FOR 10.1; req_2: CYCLE 2/10-13 comment_1: OFFSET TO SATURN AFTER TITAN comment_2: ACQUISITION USING comment_3: ADJUSTED COORDINATES. ! linenum: 10.100 targname: TITAN config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 74S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 10.2,11,13 comment_1: STEP-TIME= 1.6 SEC ! linenum: 10.200 targname: TITAN config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 194S fluxnum_1: 1 priority: 1 comment_1: STEP-TIME= 0.4 SEC comment_2: TAKE MAP AFTER CENTERING ! linenum: 11.000 targname: SATURN-CENTER config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 2 time_per_exp: 5M fluxnum_1: 2 priority: 2 req_1: GROUP 10-13,52-56 NO GAP; req_2: AT 30-OCT-91 +/- 25D ! linenum: 11.100 targname: SATURN-CENTER config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 2 time_per_exp: 5M fluxnum_1: 2 priority: 2 req_1: SEQ 11,11.1 NO GAP; req_2: COND IF TAC ! linenum: 12.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 30S priority: 2 req_1: CALIB FOR 13; req_2: SEQ 12,13 NON-INT ! linenum: 13.000 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD req_1: DARK TIME / 10-11,13.1 ! linenum: 13.100 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD req_1: SEQ 13,13.1 NO GAP; req_2: COND IF TAC; req_3: CYCLE 2 ! linenum: 19.000 targname: TITAN config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S fluxnum_1: 1 priority: 1 param_1: BRIGHT=3300, param_2: FAINT=280, param_4: SEARCH-SIZE=5 req_1: CYCLE 3 /19-21; req_2: ONBOARD ACQ FOR 19.1; req_3: SEQ 19-21 NO GAP; req_4: AT 5-SEP-92 +/- 25D ! linenum: 19.100 targname: TITAN config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 74S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 19.2,21 comment_1: STEP-TIME= 1.6 SEC ! linenum: 19.200 targname: TITAN config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 194S fluxnum_1: 1 priority: 1 comment_1: STEP-TIME= 0.4 SEC comment_2: TAKE MAP AFTER CENTERING ! linenum: 20.000 targname: WAVE config: ^ opmode: ACCUM aperture: SC2 sp_element: G140L wavelength: 1150-1435 num_exp: ^ time_per_exp: 30S priority: ^ req_1: CALIB FOR 21; req_2: SEQ 20,21 NON-INT; ! linenum: 21.000 targname: TITAN config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: 3 param_1: STEP-TIME=1.0,FP-SPLIT=STD req_1: DARK TIME / 19-21.1 ! linenum: 21.100 targname: TITAN config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 5 time_per_exp: 10M fluxnum_1: 2 priority: 3 param_1: STEP-TIME=1.0,FP-SPLIT=STD req_1: COND IF TAC; req_2: SEQ 21, 21.1 NO GAP; req_3: CYCLE 3 ! linenum: 22.000 targname: GEOCORONA-3 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: STEP-TIME = 1,FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 3; req_3: CYCLE 2 /22-24; req_4: DARK TIME / 22-27 comment_1: ALL PARALLEL GEOCORONA OBSERVATIONS comment_2: REQUIRE LINE-OF-SIGHT DOPPLER comment_3: CORECTION FOR HST'S ORBITAL MOTION. ! linenum: 23.000 targname: GEOCORONA-5 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 3 time_per_exp: 20M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 5; req_2: CALIB FOR 5 ! linenum: 23.100 targname: GEOCORONA-5 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: STEP-TIME=1,FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 5 ! linenum: 24.000 targname: GEOCORONA-9 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 9 time_per_exp: 20M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 9; req_2: CALIB FOR 9 ! linenum: 24.100 targname: GEOCORONA-9 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: STEP-TIME=1, FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 9; req_3: CYCLE 2 ! linenum: 25.000 targname: GEOCORONA-11 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 4 time_per_exp: 5M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 11; req_2: CALIB FOR 11; req_3: CYCLE 2 ! linenum: 25.100 targname: GEOCORONA-11 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: STEP-TIME=1, FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 11,13; req_3: CYCLE 2 ! linenum: 27.000 targname: GEOCORONA-21 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 3 time_per_exp: 20M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 21; req_2: CALIB FOR 21; req_3: CYCLE 3 ! linenum: 27.050 targname: GEOCORONA-11 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 1 time_per_exp: 20M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 13; req_2: CALIB FOR 13; req_3: CYCLE 2 ! linenum: 27.100 targname: GEOCORONA-21 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1150-1435 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 1 param_1: STEP-TIME=1, FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 21; req_3: CYCLE 3 ! linenum: 37.000 targname: TITAN-ACQ config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5S fluxnum_1: 1 priority: 1 param_1: BRIGHT=3300, param_2: FAINT=280, param_4: SEARCH-SIZE=5 req_1: ONBOARD ACQ FOR 37.1; req_2: CYCLE 2 /37-41; req_3: AT 8-AUG-92 +/- 60D comment_1: OFFSET TO SATURN AFTER TITAN comment_2: ACQUISITION USING comment_3: ADJUSTED COORDINATES. ! linenum: 37.100 targname: TITAN config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 74S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 37.2,39,41; comment_1: STEP-TIME= 1.6 SEC ! linenum: 37.200 targname: TITAN config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 194S fluxnum_1: 1 priority: 1 comment_1: STEP-TIME= 0.4 SEC comment_2: TAKE MAP AFTER CENTERING ! linenum: 38.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G140L wavelength: 1600 num_exp: 1 time_per_exp: 30S priority: 1 req_1: CALIB FOR 39; req_2: SEQ 38,39 NON-INT; ! linenum: 39.000 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1600 num_exp: 1 time_per_exp: 10M fluxnum_1: 5 priority: 1 param_1: FP-SPLIT=STD req_1: SEQ 37-41 NO GAP ! linenum: 39.100 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G140L wavelength: 1600 num_exp: 5 time_per_exp: 10M fluxnum_1: 5 priority: 1 param_1: FP-SPLIT=STD req_1: SEQ 39,39.1 NO GAP; req_2: COND IF TAC ! linenum: 40.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G160M wavelength: 1608 num_exp: 1 time_per_exp: 30S priority: 1 req_1: CALIB FOR 41; req_2: SEQ 40,41 NON-INT ! linenum: 41.000 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1608 num_exp: 1 time_per_exp: 10M fluxnum_1: 5 priority: 1 param_1: FP-SPLIT=STD ! linenum: 41.100 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1608 num_exp: 5 time_per_exp: 10M fluxnum_1: 5 priority: 1 param_1: FP-SPLIT=STD req_1: COND IF TAC; req_2: SEQ 41,41.1 NO GAP; req_3: CYCLE 2 ! linenum: 52.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 30S priority: 2 req_1: CALIB FOR 53; req_2: SEQ 52,53 NON-INT ! linenum: 53.000 targname: SATURN-CENTER config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD req_1: SEQ 11,52-56 NO GAP; req_2: AT 30-OCT-91 +/- 20D; req_3: DARK TIME / 52-57; req_4: CYCLE 2/ 52-57 ! linenum: 53.100 targname: SATURN-CENTER config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 3 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD req_1: SEQ 53, 53.1 NO GAP; req_2: COND IF TAC ! linenum: 53.200 targname: GEOCORONA-53 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 53; req_2: CALIB FOR 53 ! linenum: 54.000 targname: SATURN-NPR config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F120M,F140W num_exp: 1 time_per_exp: 20M fluxnum_1: 2 priority: 2 req_1: GUID TOL 0.025"; req_2: COND IF TAC comment_1: 'POST-CHECK' FOR SATURN FOR comment_2: AURORA LOCATION. ! linenum: 55.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 30S priority: 2 req_1: CALIB FOR 56; req_2: SEQ 55,56 NON-INT ! linenum: 56.000 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 1 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD ! linenum: 56.100 targname: SATURN-NPR config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 2 time_per_exp: 10M fluxnum_1: 2 priority: 2 param_1: FP-SPLIT=STD req_1: COND IF TAC; req_2: SEQ 56,56.1 NO GAP ! linenum: 57.000 targname: GEOCORONA-53 config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1350 num_exp: 4 time_per_exp: 10M fluxnum_1: 1 fluxnum_2: 2 priority: 2 req_1: PAR WITH 56; req_2: CALIB FOR 56 ! linenum: 57.100 targname: GEOCORONA-53 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1208 num_exp: 8 time_per_exp: 5M fluxnum_1: 1 fluxnum_2: 2 priority: 2 param_1: STEP-TIME = 1, FP-SPLIT=STD req_1: EXT PAR WITH 9999 OF 9999; req_2: CALIB FOR 53,56; req_3: CYCLE 2 ! ! end of exposure logsheet ! No scan data records found