! File: 3887C.PROP ! Database: PEPDB ! Date: 19-FEB-1994:22:57:40 coverpage: title_1: INTEGRATED DYNAMICAL AND SPECTROSCOPIC OBSERVATIONS OF JUPITER AND SAT title_2: URN sci_cat: SOLAR SYSTEM sci_subcat: GIANT PLANETS proposal_for: GO longterm: 3 cont_id: 2560 pi_title: DR 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: 20.00 num_pri: 402 wf_pc: Y fos: Y funds_amount: 300000 funds_length: 12 off_fname: CAROL off_mi: _ off_lname: QUINTANA off_title: ACTING DIRECTOR___ off_inst: NEW MEXICO STATE UNIVERSITY off_addr_1: BOX 30001, DEPT. 3699 off_city: LAS CRUCES off_state: NM off_zip: 88003 off_country: USA off_phone: 505-646-2611 ! end of coverpage abstract: line_1: An integrated set of multispectral images and ultraviolet spectra provides the line_2: basis for comparative analysis of the atmospheres of Jupiter and Saturn. The line_3: spatial resolution and the spectral range of the Hubble Space Telescope, line_4: combined with the ability to continue similar observations for at least 17 line_5: years, assure that these data will contribute to a valuable database for line_6: interpreting the high resolution data from Voyager, Galileo and Cassini. The line_7: basic problems that are addressed with these data are: temporal variations of line_8: the ammonia clouds, characterization of convection in the upper tropospheres, line_9: meridional stratospheric circulation, variation in the troposphere-stratosphere line_10: dynamic coupling and seasonal variability. ! ! end of abstract general_form_proposers: lname: ATREYA fname: SUSHIL inst: MICHIGAN, UNIVERSITY OF country: USA ! lname: BEEBE fname: RETA title: PI mi: F. inst: NEW MEXICO STATE UNIVERSITY country: USA ! lname: BELTON fname: MICHAEL inst: NATIONAL OPTICAL ASTR OBS country: USA ! lname: DANIELSON fname: G. mi: E. inst: CALTECH country: USA ! lname: GIERASCH fname: PETER inst: CORNELL UNIVERSITY country: USA ! lname: INGERSOLL fname: ANDREW inst: CALTECH country: USA ! lname: LIMAY fname: SANJAY inst: WISCONSIN, UNIVERSITY OF country: USA ! lname: OWEN fname: TOBIAS inst: HAWAII, UNIVERSITY OF country: USA ! lname: ROSSOW fname: WILLIAM inst: NASA, GISS country: USA ! lname: TRAFTON fname: LAURENCE inst: TEXAS, UNIVERSITY OF country: USA ! lname: WEST fname: ROBERT inst: JET PROPULSION LABORATORY country: USA ! lname: ENCRENAZ fname: THERESE inst: PARIS OBSERVATORY country: FRANCE esa: Y ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: This investigation is based on the acquisition of an integrated set of line_2: observations that utilize the Planetary Camera and the Faint Object line_3: Spectrograph to accumulate a data set that will provide near simultaneous line_4: multi-colored imaging and UV spectra of selected regions. The more line_5: contiguous the data, the higher will be the scientific yield. Our line_6: approach is to identify specific observing sequences and to systematically line_7: apply them during selected intervals of time. Because the Cycle 2 TAC altered line_8: our program by reducing requested observing time in cycle 2 and eliminating line_9: cycle 3, our spectroscipic investigation is mainly limited to central meridian line_10: observations of Jupiter and Saturn in Cycle 2 and our PC multicolored. line_11: imaging is curtailed. Our planned PC observations are as follows: line_12: Jupiter-- Multi-colored imaging with the Planetary Camera that will span orbits line_13: 1-6 (0 to 7.9 hours) and orbits 13 to 16 (19.3 to 24.6 hr), respectively, will line_14: yield a global comparision with Cycle 1 cloud morphology and partial maps for line_15: deriving changes in global winds. Multicolor PC observations of Saturn include line_16: two sets separated by 4.8hr +/-0.5hr which will give near global coverage line_17: and allow us to characterize how Saturn's atmosphere has recovered from line_18: the 1990 disturbance and to measure the location of the polar storm. line_19: NOTE: SATURN will be SEP by 21 H as per logsheet - PRR 8/92. ! question: 3 section: 2 line_1: For long-term projects,list the breakdown of exposure time requested/granted for line_2: each cycle. (Cycle 1= first year of HST observing; Cycle 2= second year; etc.) line_4: Cycle 1 22 hours primary, 0 hours parallel line_5: Cycle 2 33.5 (20) hours primary, 0 hours parallel line_6: Cycle 3 33.5 ( 0) hours primary, 0 hours parallel ! question: 4 section: 1 line_1: Imaging and spectral observations in the UV will provide information line_2: concerning the response of the stratosphere to variations in solar energy line_3: input. Unlike the IUE, the Faint Object Spectrograph, with a resolution line_4: of one arc second, will allow us to resolve the belt-zone structure and line_5: the planetary camera will yield increased sampling near the limb, line_6: providing information relating to vertical structure. Despite the line_7: Voyager, Galileo and Cassini missions, there will be a lack of coherent line_8: long-term mapping of Jupiter and Saturn. The long baseline of date that line_9: can be obtained with the Hubble Space Telescope will enhance the line_10: usefulness of the high resolution data and characterize the seasonal line_11: response of the polar regions. The nominal lifetime for HST is 17 years, line_12: less than a Saturnian year, however, coverage of both hemispheres of the line_13: two planets through this interval will generate a unique data set that line_14: will provide strong constraints on the models for seasonal atmospheric line_15: effects. ! question: 5 section: 1 line_1: Calculations for the FOS have been carried out by L. Trafton. The line_2: exposures have been set to achieve signal-to-noise ratios from 10 to 50. line_3: The exposures for the PC have been derived from WF/PC team results. line_4: For most of the filters, the exposures are less than a minute and do not line_5: impact the scheduling of multi-filter sequences as much as the read-out line_6: times. Throughout the proposal we have indicated that we desire an line_7: update of the PC exposures to optimize the amount of data acquired line_8: while maximizing the signal-to-noise ratios. ! question: 6 section: 1 line_1: We have not requested any real-time observations nor Peak-ups. line_2: We have assumed that the Peak-up mode will not be available in line_3: Cycle 2 and have attempted to select exposures and sequences line_4: to optimize longitudinal and latitudinal coverage. We have line_5: requested an update to identify the location of typical longitudinal line_6: regions. Using ground-based observations the location of cloud systems line_7: in System III longitude can be specified, as we did with Voyager, line_8: several months in advance. Like all other observers who are line_9: observing solar system objects, we will need information concerning line_10: the variation of the solar UV and standard instrument calibrations. ! question: 7 section: 1 line_1: The team will be organized in two categories; area of investigation and line_2: data set of primary interest. Reta Beebe and Laurence Trafton will have line_3: the chief responsibility for ascertaining that the imaging and spectral line_4: data undergoes preliminary reduction and calibration at the STScI and line_5: those components that are desired by the individual investigators are line_6: delivered for analysis. Efforts will be made to verify and archive line_7: secondary products, such as map projected data or I/F as a function of line_8: latitude, longitude, and incident and emergent angles. A line_9: three-day working meeting of the team will be held during the first line_10: 6 months that the investigators have the data within a given cycle. The line_11: goal of these sessions is to encourage collaboration, divide the data line_12: reduction effort and avoid duplication of effort. In addition, subgroup line_13: meetings, consisting of disciplines or geographical regions will be line_14: utilized. The investigators who are participating in this proposal line_15: are experienced in reduction of spacecraft data and have access line_16: to established data reduction facilities at their institutions. Costs line_17: associated with the use of these facilities are reflected in their line_18: individual budgets. ! question: 8 section: 1 line_1: This data is complementary to the GTO request by Westfall's group. If line_2: it is separated in time by a month or more, the two data sets will be more line_3: valuable as a dynamics pair that will allow investigation of the evolution line_4: of active storm centers in Jupiter's atmosphere. Spectroscopic observations line_5: by other GTO observers will enhance the long-term yield from this data line_6: set. It is our request for near simultaneous PC and FOS observations that line_7: make this proposal unique. ! question: 9 section: 1 line_1: L. Trafton, E. Danielson, and R. West are involved in other current HST line_2: proposals within this observing cycle. ! question: 10 section: 1 line_1: New Mexico State University supports the academic year salary of the line_2: PI, Reta Beebe, as is the case for all co-investigators who are not line_3: requesting personal salaries within their budgets. Computor facilities line_4: and software for data reduction and analysis have been developed and are line_5: in position to receive this data at the individual institutions. In line_6: addition, NMSU will provide facilities and support personnel to host line_7: the annual working meetings. ! !end of general form text general_form_address: lname: BEEBE fname: RETA mi: F category: PI inst: NEW MEXICO STATE UNIVERSITY addr_1: DEPT. OF ASTRONOMY addr_2: BOX 30001/DEPT.4500 city: LAS CRUCES state: NM zip: 88003 country: USA phone: 505-646-1938 ! lname: BEEBE fname: RETA title: DR. category: PI inst: NEW MEXICO STATE UNIVERSITY addr_1: DEPT. OF ASTRONOMY addr_2: BOX 30001, DEPT. 4500 city: LAS CRUCES state: NM zip: 88003 country: USA phone: 505-646-1938 telex: 505-646-6096 ! ! end of general_form_address records ! No fixed target records found solar_system_targets: targnum: 1 name_1: RD-JUP-65DEGN-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, LAT = +61.93, lev2_2: LONG = 200 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 65 DEG NLAT comment_2: ON CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 2 name_1: RD-JUP-48DEGN-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD = 67802.0, lev2_2: LAT = +44.17, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 48 DEG N LAT comment_2: ON CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 3 name_1: RD-JUP-6DEGN-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, lev2_2: LAT = +5.25, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 6 DEG N LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 4 name_1: RD-JUP-EQU-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD = 71490.0, lev2_2: LAT = +0.00, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT EQUATOR ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 5 name_1: RD-JUP-6DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD = 71449.0, lev2_2: LAT = -5.25, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 6 DEGS LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 6 name_1: RD-JUP-12DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, lev2_2: LAT = -10.53, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 12 DEG S LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 7 name_1: RD-JUP-25DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, lev2_2: LAT = -22.19, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 25 DEG S LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 8 name_1: RD-JUP-33DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, lev2_2: LAT = -29.59, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 33 DEG S LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 9 name_1: RD-JUP-48DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD = 69125.0, lev2_2: LAT = -44.17, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 48 DEG S ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 10 name_1: RD-JUP-65DEGS-CM-FOS-CYC2 descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD = 66900.0, lev2_2: LAT = -61.93, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: OBSERVE JUPITER AT 65 DEG S ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=1.4+/-0.7E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 11 name_1: JUPITER-PC-CYC2 descr_1: PLANET JUPITER lev1_1: STD = JUPITER wind_1: OLG OF JUPITER BETWEEN 330 30 comment_1: IMAGE JUPITER IN MULTIPLE FILTERS FOR 2 comment_2: SETS OF CONTIGUOUS ORBITS TO OBTAIN TWO comment_3: COMPLETE MULTICOLOR MAPS OF THE PLANET comment_4: OMIT FILTERS AT THE END OF A SEQUENCE comment_5: DURING A GIVEN ORBIT WHEN GUIDE STAR comment_6: ACQUISITION IS NECESSARY comment_7: FLUX VALUES ARE FOR PLANET CENTER fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(8890)=1.6+/-0.3E-12 fluxnum_3: 3 fluxval_3: SURF(7180)=1.5+/-0.3E-11 fluxnum_4: 4 fluxval_4: SURF(4130)=3.5+/-0.6E-11 fluxnum_5: 5 fluxval_5: SURF(3360)=9.6+/-2.0E-12 fluxnum_6: 6 fluxval_6: SURF(2300)=5.1+/-2.0E-13 fluxnum_7: 7 fluxval_7: SURF(6310)=4.5+/-0.9E-11 ! targnum: 12 name_1: RD-SAT-79DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 54640.0, lev2_2: LAT = +76.56, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +79 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 13 name_1: RD-SAT-60DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 56144.0, lev2_2: LAT = +54.64, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +60 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V = 0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 14 name_1: RD-SAT-48DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 57703.0, lev2_2: LAT = +42.73, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +48 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 15 name_1: RD-SAT-40DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 58187.0, lev2_2: LAT = +34.32, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +40 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 16 name_1: RD-SAT-90DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 54364.0, lev2_2: LAT = +90.00, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +90 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 17 name_1: RD-SAT-20DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 59719.0, lev2_2: LAT = +16.50, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +20 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 18 name_1: RD-SAT-12DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 60146.0, lev2_2: LAT = +10.03, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +12 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 19 name_1: RD-SAT-4DEGN-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 60246.0, lev2_2: LAT = +3.26, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT +4 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 21 name_1: RD-SAT-4DEGS-CM-FOS-CYC2 descr_1: FEATURE SATURN lev1_1: STD = SATURN, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 60246.0, lev2_2: LAT = -3.26, LONG = 0 wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: OBSERVE SATURN AT -4 DEG LAT ON comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(2700)=4.2+/-1.0E-13 fluxnum_3: 3 fluxval_3: SURF(1900)=9.2+/-4.0E-15 ! targnum: 22 name_1: SATURN-PC-CYC2 descr_1: PLANET SATURN lev1_1: STD = SATURN wind_1: OLG OF SATURN BETWEEN 330 30 comment_1: IMAGE SATURN IN MULTIPLE FILTERS comment_2: FLUX VALUES ARE FOR PLANET CENTER fluxnum_1: 1 fluxval_1: V=0.7 fluxnum_2: 2 fluxval_2: SURF(7180)=3.6+/-0.3E-12 fluxnum_3: 3 fluxval_3: SURF(4130)=3.9+/-0.6E-12 fluxnum_4: 4 fluxval_4: SURF(3360)=1.7+/-0.2E-12 fluxnum_5: 5 fluxval_5: SURF(2300)=1.1+/-1.0E-13 fluxnum_6: 6 fluxval_6: SURF(6310)=7.9+/-0.2E-12 fluxnum_7: 7 fluxval_7: SURF(8890)=2.4+/-0.5E-13 fluxnum_8: 8 fluxval_8: SURF(10420)=8.7+/-1.7E-13 ! ! end of solar system targets ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: PCJUP-C2-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: SEQ 1-5 NON-INT; req_2: REQ UPDATE; req_3: GUID TOL 0.025"; req_4: CYCLE 2 / 1-123 ! linenum: 2.000 sequence_1: DEFINE sequence_2: PCJUP-C2-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 14.0S fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.025" ! linenum: 3.000 sequence_1: DEFINE sequence_2: PCJUP-C2-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F718M num_exp: 1 time_per_exp: 0.5S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025" ! linenum: 4.000 sequence_1: DEFINE sequence_2: PCJUP-C2-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F889N num_exp: 1 time_per_exp: 40S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 5.000 sequence_1: DEFINE sequence_2: PCJUP-C2-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F631N num_exp: 1 time_per_exp: 8.0S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025" comment_1: THIS GENERATES A COMPLETE MAP comment_2: OF THE PLANET WHEN IT IS comment_3: REPEATED 5 MORE TIMES comment_4: COMBINED WITH 11-15, IT ALLOWS comment_5: PARTIAL MAPPING OF HORIZONTAL WINDS ! linenum: 11.000 sequence_1: DEFINE sequence_2: PCJUP-C2-2 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.4S fluxnum_1: 7 priority: 1 req_1: SEQ 11-15 NON-INT; req_2: REQ UPDATE; req_3: GUID TOL 0.025"; ! linenum: 12.000 sequence_1: DEFINE sequence_2: PCJUP-C2-2 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F1042M num_exp: 1 time_per_exp: 40S fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.025" ! linenum: 13.000 sequence_1: DEFINE sequence_2: PCJUP-C2-2 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F718M num_exp: 1 time_per_exp: 0.5S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025" ! linenum: 14.000 sequence_1: DEFINE sequence_2: PCJUP-C2-2 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 2.3S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 15.000 sequence_1: DEFINE sequence_2: PCJUP-C2-2 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 14.0S fluxnum_1: 5 priority: 1 req_1: GUID TOL 0.025" comment_1: COMBINED WITH 1-5 THIS ALLOWS comment_2: COLOR RATIOS AND MAPPING OF THE comment_3: HORIZONTAL WINDS ! linenum: 20.000 sequence_1: DEFINE sequence_2: FOSRG190H targname: # config: FOS/RD opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 13M fluxnum_1: 3 priority: 1 comment_1: MAXIMUM ALLOWED EXPOSURE TO comment_2: ALLOW 2 EXP PER ORBIT ! linenum: 21.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-65DEGN-CM-FOS-CYC2 req_1: SEQ 21-22 NO GAP; req_2: REQ UPDATE comment_1: SELECT DESIRED LONGITUDE AT comment_2: CM AT 65 DEG N LATITUDE ! linenum: 22.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-48DEGN-CM-FOS-CYC2 comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 48 DEG N LATITUDE ! linenum: 23.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-6DEGN-CM-FOS-CYC2 req_1: REQ UPDATE; comment_1: PLACE APERTURE NEAR CENTRAL comment_2: MERIDIAN AT 6 DEG N LATITUDE comment_3: AT SELECTED LONGITUDE ! linenum: 24.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-EQU-CM-FOS-CYC2 comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT EQUATOR ! linenum: 25.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-6DEGS-CM-FOS-CYC2 comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 7 DEG S LATITUDE ! linenum: 26.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-12DEGS-CM-FOS-CYC2 req_1: REQ UPDATE; comment_1: PLACE APERTURE NEAR CENTRAL comment_2: MERIDIAN AT 12 DEG S LATITUDE comment_3: AT A TYPICAL LONGITUDE ! linenum: 27.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-25DEGS-CM-FOS-CYC2 req_1: SEQ 27-28 NO GAP; req_2: REQ UPDATE comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 25 DEG S LATITUDE comment_3: AT A TYPICAL LONGITUDE ! linenum: 28.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-33DEGS-CM-FOS-CYC2 req_1: REQ UPDATE; comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 33 DEG S LATITUDE comment_3: AT A TYPICAL LONGITUDE ! linenum: 29.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-48DEGS-CM-FOS-CYC2 req_1: SEQ 29-30 NO GAP; comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 48 DEG S LATITUDE ! linenum: 30.000 sequence_1: USE sequence_2: FOSRG190H targname: RD-JUP-65DEGS-CM-FOS-CYC2 comment_1: PLACE APERTURE ON CENTRAL comment_2: MERIDIAN AT 65 DEG S LATITUDE ! linenum: 40.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 req_1: SEQ 40-45 NO GAP; comment_1: 40-45 GENERATES A COMPLETE MAP comment_2: OF THE PLANET. WITH 50-53 IT comment_3: ALLOWS MAPPING OF HORIZONTAL WINDS ! linenum: 41.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 ! linenum: 42.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 ! linenum: 43.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 ! linenum: 44.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 ! linenum: 45.000 sequence_1: USE sequence_2: PCJUP-C2-1 targname: JUPITER-PC-CYC2 ! linenum: 50.000 sequence_1: USE sequence_2: PCJUP-C2-2 targname: JUPITER-PC-CYC2 req_1: SEQ 50-53 NO GAP; req_2: AFTER 40 BY 19.3H +/-0.5H comment_1: 40-45 GENERATES A COMPLETE MAP comment_2: OF THE PLANET. WITH 50-53 IT comment_3: ALLOWS MAPPING OF HORIZONTAL WINDS ! linenum: 51.000 sequence_1: USE sequence_2: PCJUP-C2-2 targname: JUPITER-PC-CYC2 ! linenum: 52.000 sequence_1: USE sequence_2: PCJUP-C2-2 targname: JUPITER-PC-CYC2 ! linenum: 53.000 sequence_1: USE sequence_2: PCJUP-C2-2 targname: JUPITER-PC-CYC2 ! linenum: 100.000 sequence_1: DEFINE sequence_2: PCSAT-C2-1 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F718M num_exp: 1 time_per_exp: 0.8S fluxnum_1: 2 priority: 1 req_1: SEQ 100-102 NON-INT; req_2: REQ UPDATE; req_3: GUID TOL 0.025" ! linenum: 100.500 sequence_1: DEFINE sequence_2: PCSAT-C2-1 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F547M num_exp: 2 time_per_exp: 1S fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 101.000 sequence_1: DEFINE sequence_2: PCSAT-C2-1 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F631N num_exp: 1 time_per_exp: 17S fluxnum_1: 8 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 101.500 sequence_1: DEFINE sequence_2: PCSAT-C2-1 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F889N num_exp: 1 time_per_exp: 2M fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 102.000 sequence_1: DEFINE sequence_2: PCSAT-C2-1 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F230W num_exp: 1 time_per_exp: 3.0M fluxnum_1: 5 priority: 2 req_1: REQ UPDATE; req_2: GUID TOL 0.025" ! linenum: 103.000 sequence_1: DEFINE sequence_2: PCSAT-C2-2 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F718M num_exp: 1 time_per_exp: 0.8S fluxnum_1: 2 priority: 1 req_1: SEQ 103-106 NON-INT; req_2: REQ UPDATE; req_3: GUID TOL 0.025"; ! linenum: 104.000 sequence_1: DEFINE sequence_2: PCSAT-C2-2 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F439W num_exp: 1 time_per_exp: 4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 105.000 sequence_1: DEFINE sequence_2: PCSAT-C2-2 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F336W num_exp: 1 time_per_exp: 20S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 106.000 sequence_1: DEFINE sequence_2: PCSAT-C2-2 targname: # config: PC opmode: IMAGE aperture: P6 sp_element: F547M num_exp: 2 time_per_exp: 1S fluxnum_1: 6 priority: 1 req_1: GUID TOL 0.025" ! linenum: 107.000 sequence_1: DEFINE sequence_2: FOSRS190H targname: # config: FOS/RD opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 13M fluxnum_1: 3 priority: # ! linenum: 108.000 sequence_1: DEFINE sequence_2: FOSRS190H2 targname: # config: FOS/RD opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 30M fluxnum_1: 3 priority: # ! linenum: 110.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-79DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 79 DEG NORTH LATITUDE ! linenum: 111.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-60DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 60 DEG NORTH LATITUDE ! linenum: 112.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-48DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 48 DEG NORTH LATITUDE ! linenum: 113.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-40DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 40 DEG NORTH LATITUDE ! linenum: 114.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-90DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 90 DEG NORTH LATITUDE ! linenum: 115.000 sequence_1: USE sequence_2: FOSRS190H2 targname: RD-SAT-20DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 20 DEG NORTH LATITUDE ! linenum: 116.000 sequence_1: USE sequence_2: FOSRS190H targname: RD-SAT-12DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 12 DEG NORTH LATITUDE ! linenum: 117.000 sequence_1: USE sequence_2: FOSRS190H targname: RD-SAT-4DEGN-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 4 DEG NORTH LATITUDE ! linenum: 119.000 sequence_1: USE sequence_2: FOSRS190H targname: RD-SAT-4DEGS-CM-FOS-CYC2 priority: 1 comment_1: LOCATE APERTURE ON CENTRAL MERIDIAN comment_2: AT 4 DEG SOUTH LATITUDE ! linenum: 120.000 sequence_1: USE sequence_2: PCSAT-C2-1 targname: SATURN-PC-CYC2 ! linenum: 121.000 sequence_1: USE sequence_2: PCSAT-C2-1 targname: SATURN-PC-CYC2 req_1: SEQ 120-121 NO GAP; req_2: REQ UPDATE comment_1: LONGITUDE OF POLAR STORM SHOULD comment_2: BE CONSIDERED ! linenum: 122.000 sequence_1: USE sequence_2: PCSAT-C2-2 targname: SATURN-PC-CYC2 req_1: AFTER 120 BY 21H+/-0.5H ! linenum: 123.000 sequence_1: USE sequence_2: PCSAT-C2-2 targname: SATURN-PC-CYC2 req_1: SEQ 122-123 NO GAP ! ! end of exposure logsheet ! No scan data records found