! $Id: 5313,v 35.1 1995/01/31 16:52:26 pepsa Exp $ coverpage: title_1: CHARACTERIZATION OF JUPITER'S VERTICAL CLOUD STRUCTURE AND ATMOSPHERIC title_2: MOTIONS: CYCLE4 HIGH sci_cat: SOLAR SYSTEM sci_subcat: GIANT PLANTS proposal_for: GO pi_fname: RETA pi_mi: F pi_lname: BEEBE pi_inst: NEW MEXICO STATE UNIVERSITY pi_country: USA pi_phone: 505-646-1938 hours_pri: 10.00 num_pri: 12 wf_pc: Y time_crit: Y off_fname: CAROL off_lname: WALKER off_title: DIR. A&S RES. CENT. off_inst: 2960 off_addr_1: ARTS AND SCIENCES RESEARCH CENTER off_addr_2: BOX 30001/DEPT RC off_city: LAS CRUCES off_state: NM off_zip: 88003 off_country: USA off_phone: 505-646-2611 ! end of coverpage abstract: line_1: The primary scientific objective of this proposal is to continue the line_2: investigation to determine the state and long-term evolution of the dynamical line_3: and cloud regimes in Jupiter's atmosphere, with special emphasis on the region line_4: between +/- 15 degrees planetocentric latitude. This objective is an essential line_5: part of a larger research effort which includes the acquisition and analysis of line_6: data from the Galileo orbiter and probe, and the analysis of ground-based and line_7: Voyager data. The goal of this effort is to understand the general meteorology line_8: of Jupiter's visible atmosphere and the nature of the transport processes that line_9: occur within it. Filters and observing sequences have been chosen to allow us line_10: to evaluate the extent to which the WFPC2 can be utilized to characterize the line_11: spatial and temporal variations in horizontal motions and to discriminate line_12: vertical structure. An observing sequence consisting of multicolor observations line_13: for two rotations of the planet is requested in March-May 1995 for the post-come line_14: t impact era. Due to the red-blindness of the Voyager and the limited data rate line_15: from Galileo, HST/WFPC2 is the prime instrument to characterize the state of the line_16: Jovian atmosphere before and during the Galileo probe entry epoch. The observat line_17: ions in this proposal will help to define whether the probe data are typical of line_18: the latitude of entry (6.57 +/-0.5 deg.planetocentric latitude) and the extent t line_19: o which they can be extrapolated to other latitudes. ! ! end of abstract general_form_proposers: lname: BEEBE fname: RETA inst: 2960 country: USA ! lname: BELTON fname: MICHAEL inst: 2902 country: USA ! lname: CUNNINGHAM fname: CINDY inst: 4678 country: CANADA ! lname: GIERASCH fname: PETER inst: 1810 country: USA ! lname: INGERSOLL fname: ANDREW inst: 1590 country: USA ! lname: ORTON fname: GLENN inst: 2370 country: USA ! lname: POLLACK fname: JAMES inst: 2852 country: USA ! lname: RAGES fname: KATHY inst: 2852 country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: line_2: We propose to use the PC1 chip of WFPC2 with filters F953N, FQCH4P15 line_3: (893nm), F814W, F673N, FQCH4N15 (619 nm), F555M, F439W, F336W and F218W to line_4: obtain multicolor images of Jupiter and to derive cloud displacements and line_5: color ratios as a function of viewing geometry for selected regions of the line_6: planet. line_7: Because the PC1 chip has a field-of-view of 35 X 35 arcseconds and the line_8: diameter of Jupiter is 44 X 42 arcsec. at opposition, we are proposing to line_9: target the planet at the equator but to offset the PC1 chip in longitude line_10: toward the limbward side of the planet and rotate the telescope in order to line_11: get as much of both poles as possible and to keep the equatorial limb of the line_12: planet away from the edge of the chip. Because Jupiter rotates 0.605 degrees line_13: per minute or about 58 degrees per HST orbit, selected regions can be viewed line_14: at high and low incident and emergent angles in two consecutive orbits. From line_15: this data we can: line_16: 1. obtain zonal wind speeds in near-IR, green and methane (892 nm) and line_17: obtain reliable error estimates and line_18: 2. derive color ratio measurements of equatorial emission angles of 84, line_19: 72, 55, 26 and 14 deg. (a cloud parcel that is 84 degrees from the CM at the line_20: beginning of imaging in an orbit will be at 72 deg 20min later, at 55 deg 13 line_21: HST orbits later, and at 26 and 14 deg in the next HST orbit. This yields a line_22: cosine of the emergent angle sampling of 0.11, 0.31, 0.57, 0.90, 0.97.) line_23: We are requesting two 6-orbit sequences separated by 20.8 (13 HST ! question: 3 section: 2 line_1: orbits) late in Cycle 4 (March-May 1995) to define the state of the line_2: atmosphere before the arrival of the Galileo probe in December 1995. ! question: 4 section: 1 line_1: line_2: The pixel scale of the planetary mode of the WFPC2 is 46 milliarcseconds. line_3: Using the 1993 opposition as a typical case, the range from earth to Jupiter line_4: was 4.454 AU on March 31, 1993. At this range a PC1 pixel will subtend 149 km line_5: at the subearth point on the planet. Figure 5.2 of the WFPC2 Instrument line_6: handbook indicates that more than 50% of the light from a point source will line_7: fall within a 2 X 2 pixel area. Although this will smear small clouds over line_8: several pixels, if the noise within the images is low enough that we can line_9: navigate and map our images and obtain cross-correlations between the two sets line_10: (separated by 19.26 hours) that are accurate to 3 pixels, we can detect line_11: changes in the zonal jets on the order of 6.5 meters/sec. There are few line_12: clouds in Jupiter's atmosphere that move in the high speed jets that have high line_13: enough local contrast to be visible at groundbased resolutions and still line_14: remain unchanged for long enough periods of time. It is necessary to obtain line_15: subarcsecond seeing for sequential viewing at 8 day intervals to match line_16: accuracy of zonal wind measurements attainable with the advertised line_17: resolution of the WFPC2. line_18: The Voyager data provided us with zonal wind measurements more than a line_19: Jovian year ago. Although HST/WFPC1 data were obtained late in Cycle 1 and 2, line_20: data nearer to the time of the Galileo probe entry, our first in situ line_21: sampling line_22: of the planet in December 1995, are needed to characterize the state of the line_23: equatorial region and establish the zonal wind profile as a function of ! question: 4 section: 2 line_1: latitude during the Galileo epoch. line_2: The current state of the Galileo high gain antenna is such that very line_3: little dynamical information will be obtained. Current data management plans line_4: for imaging during the Galileo mission reveal that it will be very heavily line_5: weighted toward characterization of satellite surfaces. A small amount of line_6: imaging of the daylight side of Jovian atmosphere will be done at very close line_7: range, where the narrow angle camera spans less than 15 degrees of latitude on line_8: the planet. These opportunities will be used to obtain cloud brightness as a line_9: function of incident and emergent angles in an effort to understand the line_10: vertical structure of the atmosphere, especially the probe entry site. The line_11: observations that we propose here are highly complementary to the Galileo data. line_12: The data rate and onboard data storage of the Galileo orbiter preclude line_13: acquisition of a inbound global movie. WFPC2 can provide the highest line_14: resolution global maps of the planet that will be available before and line_15: spanning the time of the Galileo probe entry. line_16: b. Justify the amount of exposure and estimated spacecraft time requested. line_17: Computed exposures are less than 2 minutes for any of the filters. The line_18: requirement of continuous longitudinal coverage to optimize derivation of zonal line_19: winds and the need to obtain a range of incident and emission angles recommends line_20: that we plan a sequence that uses contiguous orbits. For an object as bright line_21: as Jupiter the readout time of the chip dominates the spacecraft time. ! question: 5 section: 1 line_1: We are requesting time-critical observations to the extent that we want to line_2: acquire the observations near opposition when it is possible to rotate th line_3: e telescope to optimize the polar coverage. line_4: We will request a waiver to retrieve only the PC1 data. Our plans call for line_5: more than 7 exposures per orbit. The WF chips will be underexposed by a factor line_6: of 5 for objects with surface brightness similar to that of Jupiter (the line_7: Galilean satellites) and are so short that serendipitous discoveries are line_8: unlikely. A waiver will allow us to reach our goals and relieve the load on line_9: the data downlink. line_11: We reserve the option of changing filters after preliminary analysis of line_12: the WFPC2 data. Quality of flat fields, noise level versus line_13: rotational smear, etc. will be considered in an effort to select the best line_14: filter set and exposures to optimize the March-May 1995 data set. ! question: 6 section: 1 line_1: We have no special calibration requirements ! ! ! question: 8 section: 1 line_1: No comments. ! question: 9 section: 1 line_1: a. List the HST program numbers, titles, and present authors involved in each. line_2: Cycle 0: DD-3090 Saturn Target of Opportunity - R.Beebe and A. Ingersoll. line_3: Cycle 1: GO-2560 Integrated Dynamical and Spectroscopic Observations of line_4: Jupiter and Saturn - R. Beebe, M. Belton, P. Gierasch, line_5: A. Ingersoll. line_6: Cycle 2: GO-3887 Integrated Dynamical and Spectroscopic Observations of line_7: Jupiter and Saturn - R. Beebe, M. Belton, P. Gierasch, line_8: A. Ingersoll. line_9: Cycle 3: AR-4596 Temporal Variations of Jupiter's Atmosphere - Reta Beebe line_10: b. Specify which of the above programs are related to this proposal and line_11: summarize the scientific relationship, completion status, and main results of line_12: each. line_13: The Cycle 1 dynamical data set for Jupiter was not obtained until December line_14: 1992 and is currently being analysed by the team. Pointing difficulties line_15: have forced the postponement of the Cycle 2 observations of Jupiter to line_16: June 1993. The Cycle 3 archival data set was delivered in late April 1993 line_17: and funding has not yet arrived at NMSU. line_18: Deconvolution optimization studies have progressed during Jan-May 1993 and line_19: systematic reduction of Cycles 0-2 will be carried out during the summer of line_20: 1993. line_21: The Cycle 0 and Saturn part of Cycle 1 and 2 are related to this proposal in line_22: that they have allowed direct comparison of temporal variability of the two line_23: giant planets. These data have been reduced and published. From a comparative ! question: 9 section: 2 line_1: point-of-view the most significant result from these data is the derivation of line_2: zonal winds from broad-band green and 889 CH4 images which shows variation of line_3: zonal winds with height at low latitudes. These results are consistent with line_4: midlatitude values derived from the Voyager infrared data using the thermal line_5: wind equation which is not valid at low latitudes. line_6: c. List publications resulting from previous HST data (Format: Title, line_7: Authors,Journal, Volume, Page, and Year.) line_8: The Onset and Growth of the 1990 Equatorial Disturbance on Saturn, line_9: Beebe, R.F., C. Barnet, P.V. Sada, and A.S. Murrell, Icarus, 95, line_10: 163-172, 1992. line_11: Hubble Space Telescope Observations of the 1990 Equatorial Disturbance line_12: on Saturn: Zonal Winds and Central Meridian Albedos, Barnet, C.D., J.A. line_13: Westphal,R.F. Beebe, and L.F. Huber, Icarus, 100, 499-511, 1992. ! question: 10 section: 1 line_1: Access to Sun Work Stations, equipped with IRAF-STSDAS and software that is line_2: analogous to the JPL-MIPL AMOS is available at NMSU and York University. line_3: M. Belton will have direct access to JPL-Galileo reduction software through a line_4: homebased work station. Orton, Pollack and Rages have computing facilities line_5: and current software for data reduction and interpretation of the data. line_6: Ingersoll and Gierasch have their own systems and will use reduced data line_7: provided by the rest of the team ! !end of general form text general_form_address: lname: BEEBE fname: RETA mi: F category: PI inst: 2960 addr_1: DEPT. OF ASTRONOMY addr_2: NEW MEXICO STATE UNIVERSITY addr_3: P.O. BOX 30001/ DEPT 4500 city: LAS CRUCES state: NM zip: 88003 country: USA phone: 505-646-1938 telex: RBEEBE@NMSU.EDU ! lname: category: CON ! ! end of general_form_address records ! No fixed target records found solar_system_targets: targnum: 1 name_1: JUPITER-PC-ROT0-LONG1 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER lev2_1: TYPE = POS_ANGLE, RAD = 7.8, lev2_2: ANG = 21, REF = SUN comment_1: FLUX VALUES ARE FOR PLANET CENTER comment_2: PC OFFSET TOWARD THE LIMB fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(9530) = 1.0 +/-0.3E-12 fluxnum_3: 3 fluxval_3: SURF(8930) = 1.6 +/-0.3E-12 fluxnum_4: 4 fluxval_4: SURF(8140) = 1.5 +/-0.3E-11 fluxnum_5: 5 fluxval_5: SURF(6730) = 4.5 +/-0.3E-11 fluxnum_6: 6 fluxval_6: SURF(6190) = 4.5 +/-0.3E-11 fluxnum_7: 7 fluxval_7: SURF(5550) = 3.7 +/-0.6E-11 fluxnum_8: 8 fluxval_8: SURF(4390) = 3.5 +/-0.6E-11 fluxnum_9: 9 fluxval_9: SURF(3360) = 9.6 +/-2.0E-12 fluxnum_10: 10 fluxval_10: SURF(2180) = 5.1 +/-2.0E-13 ! targnum: 12 name_1: JUPITER-WF-ROT2-LONG6 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER lev2_1: TYPE = POS_ANGLE, RAD = 3.2, lev2_2: ANG = 0, REF = SUN comment_1: FLUX VALUES ARE FOR PLANET CENTER comment_2: WF OFFSET TO AVOID VIGNETTING fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(9530) = 1.0 +/-0.3E-12 fluxnum_3: 3 fluxval_3: SURF(8930) = 1.6 +/-0.3E-12 fluxnum_4: 4 fluxval_4: SURF(8140) = 1.5 +/-0.3E-11 fluxnum_5: 5 fluxval_5: SURF(6730) = 4.5 +/-0.3E-11 fluxnum_6: 6 fluxval_6: SURF(6190) = 4.5 +/-0.3E-11 fluxnum_7: 7 fluxval_7: SURF(5550) = 3.7 +/-0.6E-11 fluxnum_8: 8 fluxval_8: SURF(4390) = 3.5 +/-0.6E-11 fluxnum_9: 9 fluxval_9: SURF(3360) = 9.6 +/-2.0E-12 fluxnum_10: 10 fluxval_10: SURF(2180) = 5.1 +/-2.0E-13 ! ! end of solar system targets ! No generic target records found exposure_logsheet: linenum: 1.010 sequence_1: DEFINE sequence_2: EXPOSURE1 targname: # config: WFPC2 opmode: IMAGE aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; req_4: SEQ 1.01-1.09 NON-INT; comment_1: LONGITUDE IN TORUS COORDINATE SYSTEM comment_2: SHOULD BE ADJUSTED FOR DISTANCE comment_3: QUALITY AND EXPOSURE OF FILTER WILL BE comment_4: CHECKED ! linenum: 1.020 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.030 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.040 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F673N num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.050 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 0.2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.060 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F410M num_exp: 1 time_per_exp: 9.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 8 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.070 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.080 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 1.090 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED comment_3: 1.09 COULD BE DROPPED IF NECESSARY ! linenum: 2.010 sequence_1: DEFINE sequence_2: EXPOSURE2 targname: # config: WFPC2 opmode: IMAGE aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; req_5: seq 2.01-2.09 non-int; comment_1: LONGITUDE IN TORUS COORDINATE SYSTEM comment_2: SHOULD BE ADJUSTED FOR DISTANCE comment_3: QUALITY AND EXPOSURE OF FILTER WILL BE comment_4: CHECKED ! linenum: 2.020 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.030 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.040 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F255W num_exp: 1 time_per_exp: 300S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.050 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: 1 time_per_exp: 15.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 9 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.060 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F410M num_exp: 1 time_per_exp: 9S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 8 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.070 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 0.2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.080 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 2.090 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.010 sequence_1: DEFINE sequence_2: EXPOSURE3 targname: # config: WFPC2 opmode: IMAGE aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7, param_2: read=1+3+4 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; req_4: SEQ 3.01-3.11 non-int; comment_1: LONGITUDE IN TORUS COORDINATE SYSTEM comment_2: SHOULD BE ADJUSTED FOR DISTANCE comment_3: QUALITY AND EXPOSURE OF FILTER WILL BE comment_4: CHECKED ! linenum: 3.020 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16S s_to_n: 30 param_1: ATD-GAIN=7, param_2: read=1+3+4 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.030 sequence_1: DEFINE sequence_2: EXPOSURE3 targname: # config: WFPC2 opmode: IMAGE aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! ! linenum: 3.040 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F673N num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.050 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 0.2S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.060 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F410M num_exp: 1 time_per_exp: 9S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 8 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.070 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: 1 time_per_exp: 15.0S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 9 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.080 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7, param_2: read=1+3+4 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.090 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16S s_to_n: 30 param_1: ATD-GAIN=7, param_2: read=1+3+4 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.100 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 3.110 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F814W num_exp: 1 time_per_exp: 0.2S s_to_n: 30 param_1: ATD-GAIN=15, param_2: read=1+3+4 fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED comment_3: DROP 3.10 IF NECESSARY ! linenum: 4.010 sequence_1: DEFINE sequence_2: EXPOSURE4 targname: # config: WFPC2 opmode: IMAGE aperture: PC1-FIX sp_element: FQCH4N15 wavelength: 6211 num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; req_5: SEQ 4.01-4.10 non-int; comment_1: LONGITUDE IN TORUS COORDINATE SYSTEM comment_2: SHOULD BE ADJUSTED FOR DISTANCE comment_3: QUALITY AND EXPOSURE OF FILTER WILL BE comment_4: CHECKED ! linenum: 4.020 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.030 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.040 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F255W num_exp: 1 time_per_exp: 300S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.050 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: 1 time_per_exp: 15.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 9 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.060 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F410M num_exp: 1 time_per_exp: 9S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 8 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.070 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 0.2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.080 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F673N num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.090 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: PC1-FIX sp_element: FQCH4P15 wavelength: 8922 num_exp: 1 time_per_exp: 50.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 4.100 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 16.0S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED comment_3: DROP 4.08 IF NECESSARY ! linenum: 5.010 sequence_1: DEFINE sequence_2: EXPOSURE5 targname: # config: WFPC2 opmode: IMAGE aperture: fqch4w3 sp_element: FQCH4N33 wavelength: 6211 num_exp: 1 time_per_exp: 0.14S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; req_5: SEQ 5.01-5.10 non-int; comment_1: LONGITUDE IN TORUS COORDINATE SYSTEM comment_2: SHOULD BE ADJUSTED FOR DISTANCE comment_3: QUALITY AND EXPOSURE OF FILTER WILL BE comment_4: CHECKED ! linenum: 5.020 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: fqch4w3 sp_element: F953N num_exp: 1 time_per_exp: 7.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.030 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: FQCH4N wavelength: 8922 num_exp: 1 time_per_exp: 20.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.040 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F255W num_exp: 1 time_per_exp: 60S s_to_n: 30 param_1: ATD-GAIN=7 fluxnum_1: 10 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.050 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: 1 time_per_exp: 3.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 9 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.060 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F410M num_exp: 1 time_per_exp: 2.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 8 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.070 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F547M num_exp: 1 time_per_exp: 0.11S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.080 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F673N num_exp: 1 time_per_exp: 2S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.090 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: FQCH4N wavelength: 8922 num_exp: 1 time_per_exp: 20.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED ! linenum: 5.100 sequence_1: ^ sequence_2: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F953N num_exp: 1 time_per_exp: 7.0S s_to_n: 30 param_1: ATD-GAIN=15 fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.103"; comment_1: QUALITY AND EXPOSURE OF FILTER WILL BE comment_2: CHECKED THIS EXPOSURE CAN BE DROPPED. comment_3: THE F673N CAN ACT AS A CONTINUUM AND comment_4: IN R-G-B SET IF WILLIAMS DOES NOT comment_5: GRANT SL-9 TIME ! linenum: 10.100 sequence_1: USE sequence_2: EXPOSURE1 targname: JUPITER-PC-ROT0-LONG1 req_1: CYCLE 4 / 10.1-12.6; req_2: SEQ 10.1-11.5 WITHIN 10H; ! req_3: AT 9-FEB-95:12:00 +/- 3.5D ! linenum: 11.100 sequence_1: USE sequence_2: EXPOSURE1 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 11.200 sequence_1: USE sequence_2: EXPOSURE3 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 11.300 sequence_1: USE sequence_2: EXPOSURE3 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 11.400 sequence_1: USE sequence_2: EXPOSURE3 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 11.500 sequence_1: USE sequence_2: EXPOSURE3 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 12.100 sequence_1: USE sequence_2: EXPOSURE2 targname: JUPITER-PC-ROT0-LONG1 req_1: SEQ 12.1-12.5 WITHIN 10H; ! req_2: AT 9-FEB-95:12:00 +/- 3.5D ! linenum: 12.200 sequence_1: USE sequence_2: EXPOSURE4 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 12.300 sequence_1: USE sequence_2: EXPOSURE4 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 12.400 sequence_1: USE sequence_2: EXPOSURE4 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 12.500 sequence_1: USE sequence_2: EXPOSURE4 targname: JUPITER-PC-ROT0-LONG1 ! linenum: 12.600 sequence_1: USE sequence_2: EXPOSURE5 targname: JUPITER-WF-ROT2-LONG6 req_1: AFTER 12.1 BY 20H+/-3H comment_1: AFTER 12.1 BY 30H+/-3H is comment_2: also acceptable ! ! end of exposure logsheet ! No scan data records found