! File: 2560C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:08:04:39 coverpage: title_1: INTEGRATED DYNAMICAL AND SPECTROSCOPIC OBSERVATIONS OF JUPITER AND title_2: SATURN sci_cat: SOLAR SYSTEM sci_subcat: GIANT PLANETS proposal_for: GO longterm: 3 pi_title: DR. pi_fname: RETA pi_lname: BEEBE pi_inst: NEW MEXICO STATE UNIVERSITY pi_country: USA pi_phone: 505-646-1938 keywords_1: SOLAR SYSTEM-PLANETS, JUPITER AND SATURN, BELTS, ZONES, keywords_2: WIND, ATMOSPHERE, PLUMES, RED SPOT, OVALS, BARGES, ACTIVE CONVECTION SITES hours_pri: 22.00 num_pri: 29 wf_pc: Y fos: Y funds_amount: 301000 funds_length: 12 funds_date: JAN-92 pi_position: PROF. OF ASTRONOMY off_fname: CAROL off_lname: QUINTANA off_title: ACTING DIRECTOR off_inst: THE REGENTS OF NEW MEXICO STATE UNIVERSITY 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 off_telex: 505-646-6096 ! end of coverpage abstract: line_1: An integrated set of multispectral images and ultraviolet spectra line_2: provides the basis for comparative analysis of the atmospheres of line_3: Jupiter and Saturn. The spatial resolution and the spectral range line_4: of the Hubble Space Telescope, combined with the ability to continue line_5: similar observations for at least 17 years, assure that this data line_6: will contribute to a valuable database for interpreting the high line_7: resolution data from Voyager, Galileo and Cassini. The basic problems line_8: that are addressed with these data are: temporal variations of the line_9: ammonia clouds, characterization of convection in the upper line_10: tropospheres, meridional stratospheric circulation, variation in the line_11: troposphere-stratosphere dynamic coupling and seasonal variability. ! ! end of abstract general_form_proposers: lname: ATREYA fname: SUSHIL title: DR. inst: MICHIGAN, UNIVERSITY OF country: USA ! lname: BEEBE fname: RETA title: P.I. inst: NEW MEXICO STATE UNIVERSITY country: USA ! lname: BELTON fname: MICHAEL title: DR. inst: NATIONAL OPTICAL ASTR OBS country: USA ! lname: DANIELSON fname: G. title: MR. mi: E. inst: CALTECH country: USA ! lname: GIERASCH fname: PETER title: DR. inst: CORNELL UNIVERSITY country: USA ! lname: INGERSOLL fname: ANDREW title: DR. inst: CALTECH country: USA ! lname: LAMAYE fname: SANJAY title: DR. inst: WISCONSIN, UNIVERSITY OF country: USA ! lname: OWEN fname: TOBIAS title: DR. inst: HAWAII, UNIVERSITY OF country: USA ! lname: ROSSOW fname: WILLIAM title: DR. inst: NASA, GODDARD country: USA ! lname: TRAFTON fname: LAURENCE title: DR. inst: TEXAS, UNIVERSITY OF country: USA ! lname: WEST fname: ROBERT title: DR. mi: A. inst: JET PROPULSION LABORATORY country: USA ! lname: ENCRENAZ fname: THERESE title: DR. inst: PARIS OBSERVATORY country: FRANCE esa: X ! ! 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-color 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. Features, including the Red line_8: Spot, and active equatorial plume, a brown barge and a White Oval, will be line_9: observed as well. The northern hemisphere of Saturn will be mapped in the line_10: second cycle and the southern hemisphere in the third cycle. We have sub- line_11: mitted a detailed schedule for the first cycle only. We plan to use a line_12: highly similar approach for th following two cycles. Because of our desire line_13: for contiguous data, we have assigned priorities to specific sets of line_14: observations and would to prefer to omit certain data when it interferes line_15: with acquisition of guide stars, etc. rather than to suffer larger temporal line_16: gaps in the data. line_18: Our planned observations are as follows: line_20: Jupiter-- Multi-color imaging with the Planetary Camera that will span orbits line_21: 1-6 (0 to 7.9 hours) and orbits 14 to 19 (19.0 to 26.9), respectively, will line_22: yield two multi-color maps of the planet. The two sequences will look at the line_23: center of the planet and the longitude of the central meridian will be 0, 57, ! question: 3 section: 2 line_1: 115, 172, 230 and 286 degrees for sequence 1 and 25, 82, 140, 197, 255 and 312 line_2: deg for seq 2, relative to the initial starting position. Sequence 1 Filters line_3: are F718M, F889N, F413M, F336W and F230W and sequence 2 filters are F413M, line_4: F718M, F631N, F336W and F284W. The indicated order of the filters minimizes line_5: the difference in viewing angle for F718M and F889N (optimizing a color-ratio line_6: map) in the first sequence and assures that we obtain the F413M pair for line_7: measuring wind field in two colors with the least smeared images. The F336W line_8: pair will be lower spatial resolution; however, they will provide information line_9: on vertical wind shear. The F631N filter places additional constraints on line_10: the spectral dependence on limb- darkening. We have considered the possible line_11: loss of the last image in some of the sequences and assumed that we could read line_12: out the last image during earth occultation. This 20.6 hour time difference line_13: between the two imaging sets corresponds to a minimum detectable velocity of line_14: 2 m/sec. During orbits preceding and between this line_15: mapping sequence spectra will be obtained of the line_16: same atmospheric region with different gratings of the Faint Object Spectro- line_17: graph: Three observing sequences have been formulated to obtain spectra line_18: ranging in wavelength from 1600 to 3300A. Using the FOS/RD and the FOS/BL line_19: configuration with gratings G190H and G270H, signal to noise ranging from 10 to line_20: 50 can be obtained for the wavelength interval from 1700 to 3300A. In order to line_21: obtain observations at selected latitudes, as well as observations of specific line_22: features, we are proposing that sequences be repeated in a systematic manner. line_23: This will allow us to characterize the Rayleigh H2 and particulate scattering, ! question: 3 section: 3 line_1: obtain visible, near IR and UV imaging, and obtain spectra of NH3, PH3, C2H2, line_2: and H2S at selected latitudes (a preliminary choice is 65, 48, 25, 20, 15, 6, line_3: and -20 degrees planetographic latitude for cycles 1 and 3, with a similar line_4: selection mapping the southern hemisphere in cycle 2). This approach to line_5: observing the planet defines the scope of data that can be obtained within 22 line_6: hours of observing time. ! question: 3 section: 4 line_1: For long-term projects, list the breakdown of exposure time requested 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 hours primary, 0 hours parallel line_6: Cycle 3 33.5 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 calculated by E. Danielson and R. West. 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 and FOS 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, however in order line_2: to use a peak-up mode of acquisition on Io in an efficient manner it line_3: is necessary to sequence the data for several orbits to utilize a single line_4: guide star acquisition. We have requested an update to identify the line_5: longitude of the Red Spot and an active plume. Using ground-based line_6: observations the location of these cloud systems in System III longitude line_7: can be specified, as we did with Voyager, several months in advance. line_8: We will also need to specify the longitude of the sun-lit limb in the line_9: TORUS mode after we know whether our observations will be pre- or post- line_10: opposition. Like all other observers who are observing solar system line_11: objects, we will need information concerning the variation of the solar line_12: 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. Other investi- line_9: gators plan to be present during the observing period to familiarize line_10: themselves with the data acquisition procedures and the preliminary data line_11: reduction. A three-day working meeting of the team will be held during line_12: the first 6 months that the investigators have the data for a given line_13: cycle. The goal of these sessions is to encourage collaboration, divide line_14: the data reduction effort and avoid duplication of effort. In addition, line_15: sub-group meetings, consisting of disciplines or geographical regions line_16: will be utilized. The investigators who are participating in this pro- line_17: posal are experienced in reduction of spacecraft data and have access line_18: to established data reduction facilities at their institutions. Costs line_19: associated with the use of these facilities are reflected in their line_20: 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 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: 2 name_1: BL-JUPITER-6DEGN-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD=71449.0, lev2_2: LAT = +5.25, LONG = 77 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER ON SUNLIT LIMB AT comment_2: AT +6 DEG LATITUDE fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 3 name_1: BL-JUPITER-6DEGN-CM-FOS 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 90 comment_1: OBSERVE A PLUME NEAR THE CENTRAL comment_2: MERIDIAN. LONGITUDE TBD AT LAST comment_3: POSSIBLE DATE FROM GROUND-BASED comment_4: INFORMATION, REQUIRE UPDATE fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 4 name_1: BL-JUPITER-48DEGN-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD=69125.0, lev2_2: LAT = +44.16, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +48 DEG LAT ON THE comment_2: CENTRAL MERIDIAN fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 5 name_1: BL-JUPITER-48DEGN-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 69125.0, lev2_2: LAT = +44.16, LONG = 74 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +48 DEG LAT ON THE comment_2: SUNLIT LIMB fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 6 name_1: BL-JUPITER-HILAT-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD=67802.0, lev2_2: LAT = +56.57, LONG = 70 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT HIGH LAT ON THE comment_2: SUNLITLIMB. LAT WILL BE SUPPLIED TO comment_3: COINCIDE WITH AURORAE fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 7 name_1: BL-JUPITER-HILAT-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, LAT = +56.57, LONG = 200 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT HIGH LAT ON THE comment_2: CENTRAL MERIDIAN. LAT WILL BE CHOSEN comment_3: TO COINCIDE WITH AURORA comment_4: REQUIRE UPDATE fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(1900)=2.1+/-1.0E-14 ! targnum: 8 name_1: RD-JUPITER-6DEGN-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 71449.0, lev2_2: LAT = +5.25, LONG = 90 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +6 DEG ON THE comment_2: SUNLIT LIMB 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-JUPITER-6DEGN-LIMB-FOSB descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 71449.0, lev2_2: LAT = +5.25, LONG = 77 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +6 DEG ON THE comment_2: SUNLIT LIMB 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-JUPITER-6DEGN-CM-FOS 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 90 comment_1: OBSERVE CM +6 DEG LAT comment_2: LONGITUDE TBD, REQUIRE UPDATE fluxnum_1: 1 fluxval_1: V=-2.5 fluxnum_2: 2 fluxval_2: SURF(2700)=2.1+/-1.0E-12 fluxnum_3: 3 fluxval_3: SURF(1900)=2.1+/-1.0E-14 ! targnum: 11 name_1: RD-JUPITER-25DEGN-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 70774.0, lev2_2: LAT = +22.18, LONG = 80 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +25 DEG LAT ON THE comment_2: SUNLIT LIMB 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: 12 name_1: RD-JUPITER-25DEGN-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 70774.0, lev2_2: LAT = +22.18, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +25 DEG LAT ON THE 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: 13 name_1: RD-JUPITER-48DEGN-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 69125.0, lev2_2: LAT = +44.16, LONG = 90 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +48 DEG LAT ON THE comment_2: SUNLIT LIMB 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: 14 name_1: RD-JUPITER-48DEGN-LIMB-FOSB descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 69125.0, lev2_2: LAT = +44.16, LONG = 74 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +48 DEG LAT ON THE comment_2: SUNLIT LIMB 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: 15 name_1: RD-JUPITER-48DEGN-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 69125.0, lev2_2: LAT = +44.16, LONG =0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +48 DEG LAT ON THE 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: 16 name_1: RD-JUPITER-HILAT-LIMB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 67802.0, lev2_2: LAT =+56.57, LONG = 90 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT A HIGH LATITUDE comment_2: ON THE SUNLIT LIMB 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: 17 name_1: RD-JUPITER-HILAT-LIMB-FOSB descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 67802.0, lev2_2: LAT =+56.57, LONG = 70 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT A HIGH LATITUDE comment_2: ON THE SUNLIT LIMB. 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: 18 name_1: RD-JUPITER-HILAT-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 67802.0, lev2_2: LAT = +56.57, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT A HIGH LATITUDE ON comment_2: THE 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: 19 name_1: RD-JUPITER-SEB-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, LAT = -15.86, LONG = 229 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE THE SEB 25 DEG EAST OF THE comment_2: THE RED SPOT. 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: 21 name_1: RD-JUPITER-RED-SPOT-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, LAT = -17.65, LONG = 254 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE THE CENTER OF THE RES comment_2: SPOT. LONG TBD 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: 23 name_1: RD-JUPITER-15DEGN-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD= 771225.0, lev2_2: LAT = +13.19, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +15 LAT ON THE 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: 25 name_1: RD-JUPITER-PLUME-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = CARTO, LAT = +5.25, LONG = 289 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE A PLUME AT +6 DEG LAT. 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: 27 name_1: RD-JUPITER-20DEGN-CM-FOS descr_1: FEATURE JUPITER lev1_1: STD = JUPITER, ACQ = 0.1 lev2_1: TYPE = TORUS, RAD=71024.0, lev2_2: LAT = +17.65, LONG = 0 wind_1: OLG OF JUPITER BETWEEN 330 90 comment_1: OBSERVE JUPITER AT +20 DEG LAT ON THE 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: 28 name_1: JUPITER-PC-CYCL1 descr_1: PLANET JUPITER lev1_1: STD = JUPITER wind_1: OLG OF JUPITER BETWEEN 330 90 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 ! ! end of solar system targets ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: SEQ 1-10.5; req_2: GROUP 1-5 WITHIN 60M; req_3: GUID TOL 0.025"; req_4: CYCLE 1 / 1-140 comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 2.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 3.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 4.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 5.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F230W num_exp: ^ time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; comment_1: THIS GENERATES A COMPLETE MAP comment_2: OF THE PLANET, COUPLED WITH comment_3: 11-15, IT ALLOWS MAPPING comment_4: OF HORIZONTAL WINDS ! linenum: 6.100 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: GROUP 6.1-6.5 WITHIN 60M; req_2: GUID TOL 0.025"; ! linenum: 6.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 6.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 6.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 6.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F230W num_exp: 1 time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 7.100 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: GROUP 7.1-7.5 WITHIN 60M; req_2: GUID TOL 0.025"; ! linenum: 7.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 7.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 7.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 7.500 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F230W num_exp: ^ time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 8.100 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: GROUP 8.1-8.5 WITHIN 60M; req_2: GUID TOL 0.025"; ! linenum: 8.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 8.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 8.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 8.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F230W num_exp: 1 time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 9.100 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: GROUP 9.1-9.5 WITHIN 60M; req_2: GUID TOL 0.025"; ! linenum: 9.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 9.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 9.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 9.500 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F230W num_exp: ^ time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 10.100 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F413M num_exp: 1 time_per_exp: 1.2S fluxnum_1: 3 priority: 1 req_1: GROUP 10.1-10.5 WITHIN 60M; req_2: GUID TOL 0.025"; ! linenum: 10.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F336W num_exp: ^ time_per_exp: 5.0S fluxnum_1: 2 priority: 1 req_1: GUID TOL 0.025" ! linenum: 10.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025" ! linenum: 10.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F889N num_exp: ^ time_per_exp: 30S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025" ! linenum: 10.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F230W num_exp: 1 time_per_exp: 40S fluxnum_1: 6 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 11.000 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: SEQ 11-20.500; req_2: GROUP 11-15 WITHIN 60M; req_3: GUID TOL 0.025"; req_4: AFTER 1 BY 19.3H+/-.5H comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 12.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 13.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 14.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 15.000 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; comment_1: 11-15 GENERATES A COMPLETE MAP comment_2: OF THE PLANET. WITH 1-5 IT comment_3: ALLOWS MAPPING OF HORIZONTAL WINDS ! linenum: 16.100 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025"; req_2: GROUP 16.1-16.5 WITHIN 60M; comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 16.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 16.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 16.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 16.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 17.100 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025"; req_2: GROUP 17.1-17.5 WITHIN 60M; comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 17.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 17.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 17.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 17.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 18.100 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025"; req_2: GROUP 18.1-18.5 WITHIN 60M; comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 18.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 18.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 18.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 18.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 19.100 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025"; req_2: GROUP 19.1-19.5 WITHIN 60M; comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 19.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 19.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 19.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 19.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 20.100 sequence_1: ^ targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 0.26S fluxnum_1: 4 priority: 1 req_1: GUID TOL 0.025"; req_2: GROUP 20.1-20.5 WITHIN 60M; comment_1: EXPOSURES SHOULD BE VALIDATED ! linenum: 20.200 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F631N num_exp: ^ time_per_exp: 4.2S fluxnum_1: 7 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 20.300 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F718M num_exp: ^ time_per_exp: 0.4S fluxnum_1: 3 priority: 1 req_1: GUID TOL 0.025"; ! linenum: 20.400 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F413M num_exp: ^ time_per_exp: 1.2S fluxnum_1: 5 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 20.500 sequence_1: DEFINE sequence_2: PCJUP-1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 5.0S fluxnum_1: 4 priority: 2 req_1: GUID TOL 0.025"; ! linenum: 30.000 sequence_1: DEFINE sequence_2: FOSRDG270H targname: # config: FOS/RD opmode: ACCUM aperture: 0.5 sp_element: G270H num_exp: 1 time_per_exp: 2M fluxnum_1: 2 priority: # ! linenum: 31.000 sequence_1: DEFINE sequence_2: FOSBLG270H targname: # config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G270H num_exp: 1 time_per_exp: 1M fluxnum_1: 2 priority: # ! linenum: 32.000 sequence_1: DEFINE sequence_2: FOSRDG190H targname: # config: FOS/RD opmode: ACCUM aperture: 0.5 sp_element: G190H num_exp: 1 time_per_exp: 24M fluxnum_1: 3 priority: 1 comment_1: THIS SEQUENCE COMBINES WITH 1 CALL comment_2: TO FOSRDG207H TO PROVIDE NEAR comment_3: SIMULTANEOUS SPECTRAL COVERAGE ! linenum: 32.500 sequence_1: DEFINE sequence_2: FOSB2G190H targname: # config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 24M fluxnum_1: 2 priority: 1 comment_1: THIS SEQUENCE COMBINES WITH 1 CALL comment_2: TO FOSBLG207H TO PROVIDE NEAR comment_3: SIMULTANEOUS SPECTRAL COVERAGE ! linenum: 33.000 sequence_1: DEFINE sequence_2: FOSBLG190H targname: # config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G190H num_exp: 1 time_per_exp: 30M fluxnum_1: 2 priority: 1 comment_1: THIS SEQUENCE YIELDS DATA AT THE 1700A ! linenum: 36.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-6DEGN-LIMB-FOS comment_1: LOCATE APERTURE ON SUNLIT LIMB comment_2: AT 6 DEG NORTH LATITUDE ! linenum: 37.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-6DEGN-CM-FOS comment_1: LOCATE APERTURE ON CM comment_2: NEAR 6 DEG NORTH LATITUDE comment_3: NEED TO CONSIDER PLUMES ! linenum: 38.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-48DEGN-CM-FOS comment_1: LOCATE APERTURE ON CM comment_2: AT 48 DEG NORTH LATITUDE ! linenum: 41.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-48DEGN-LIMB-FOS comment_1: LOCATE APERTURE ON LIMB comment_2: AT 48 DEG NORTH LATITUDE ! linenum: 42.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-HILAT-LIMB-FOS comment_1: LOCATE APERTURE ON SUNLIT LIMB comment_2: AT HIGH LATITUDE ! linenum: 43.000 sequence_1: USE sequence_2: FOSBLG190H targname: BL-JUPITER-HILAT-CM-FOS comment_1: LOCATE APERTURE AT CM comment_2: AT HIGH LATITUDE ! linenum: 84.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-25DEGN-LIMB-FOS priority: 1 req_1: SEQ 84-85 NO GAP; comment_1: PLACE THE APERTURE ON THE SUNLIT LIMB comment_2: AT 25 DEG N LATITUDE. ! linenum: 85.000 sequence_1: USE sequence_2: FOSRDG190H targname: RD-JUPITER-25DEGN-LIMB-FOS ! linenum: 87.000 sequence_1: USE sequence_2: FOSBLG270H targname: RD-JUPITER-25DEGN-CM-FOS priority: 1 req_1: SEQ 87-88 NO GAP comment_1: THE APERTURE IS PLACED ON THE CENTRAL comment_2: MERIDIAN AT 25 DEG N LATITUDE ! linenum: 88.000 sequence_1: USE sequence_2: FOSB2G190H targname: RD-JUPITER-25DEGN-CM-FOS ! linenum: 90.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-6DEGN-LIMB-FOS priority: 1 req_1: SEQ 90-91 NO GAP comment_1: PLACE THE APERTURE ON THE SUNLIT LIMB comment_2: AT 6 DEG N LATITUDE. ! linenum: 90.500 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-6DEGN-LIMB-FOSB priority: 1 comment_1: PLACE APERTURE NEAR SUNLIT LIMB comment_2: AT 6 DEG N LATITUDE. ! linenum: 91.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-6DEGN-CM-FOS priority: 1 comment_1: NEED TO CONSIDER PLUME HEAD ! linenum: 92.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-48DEGN-LIMB-FOS priority: 1 req_1: SEQ 92-93 NO GAP comment_1: PLACE APERTURE ON SUNLIT LIMB comment_2: AT 48 DEG N LATITUDE. ! linenum: 92.500 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-48DEGN-LIMB-FOSB priority: 1 comment_1: PLACE APERTURE NEAR SUNLIT LIMB comment_2: AT 48 DEG N LATITUDE. ! linenum: 93.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-48DEGN-CM-FOS priority: 1 ! linenum: 94.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-HILAT-LIMB-FOS priority: 1 req_1: SEQ 94-95 NO GAP comment_1: PLACE APERTURE ON SUNLIT LIMB comment_2: AT HIGH LATITUDE. ! linenum: 94.500 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-HILAT-LIMB-FOSB priority: 1 comment_1: PLACE APERTURE NEAR THE SUNLIT LIMB comment_2: AT HIGH LATITUDE. ! linenum: 95.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-HILAT-CM-FOS priority: 1 comment_1: PLACE APERTURE ON THE CENTRAL MREIDIAN comment_2: AT 65 DEG N LATITUDE. ! linenum: 100.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-SEB-FOS priority: 1 req_1: SEQ 100-101 NO GAP comment_1: THE APERTURE SHOULD BE PLACED 25 DEG comment_2: EAST OF THE RED SPOT AT 20 DEG S LAT. comment_3: THE PI WILL SUPPLY THE LONGITUDE. ! linenum: 101.000 sequence_1: USE sequence_2: FOSRDG190H targname: RD-JUPITER-SEB-FOS ! linenum: 103.000 sequence_1: USE sequence_2: FOSRDG270H targname: RD-JUPITER-RED-SPOT-FOS priority: 1 req_1: SEQ 103-104 NO GAP comment_1: THE APERTURE SHOULD BE PLACED IN THE comment_2: CENTER OF THE RED SPOT AT 20DEG S LAT. comment_3: THE PI WILL SUPPLY THE LONGITUDE. ! linenum: 104.000 sequence_1: USE sequence_2: FOSRDG190H targname: RD-JUPITER-RED-SPOT-FOS ! linenum: 106.000 sequence_1: USE sequence_2: FOSBLG270H targname: RD-JUPITER-15DEGN-CM-FOS priority: 1 req_1: SEQ 106-107 NO GAP comment_1: PLACE APERTURE ON THE CENTRAL MERIDIAN comment_2: AT 15 DEG N LATITUDE ! linenum: 107.000 sequence_1: USE sequence_2: FOSB2G190H targname: RD-JUPITER-15DEGN-CM-FOS ! linenum: 112.000 sequence_1: USE sequence_2: FOSBLG270H targname: RD-JUPITER-PLUME-FOS priority: 1 req_1: SEQ 112-113 NO GAP comment_1: THE APERTURE SHOULD BE PLACED IN AN comment_2: ACTIVE PLUME HEAD NEAR 6 DEG N comment_3: LATITUDE. THE PI WILL SUPPLY THE comment_4: LONGITUDE. ! linenum: 113.000 sequence_1: USE sequence_2: FOSB2G190H targname: RD-JUPITER-PLUME-FOS ! linenum: 115.000 sequence_1: USE sequence_2: FOSBLG270H targname: RD-JUPITER-20DEGN-CM-FOS priority: 1 req_1: SEQ 115-116 NO GAP comment_1: PLACE APERTURE ON CM AT 20 DEG N ! linenum: 116.000 sequence_1: USE sequence_2: FOSB2G190H targname: RD-JUPITER-20DEGN-CM-FOS comment_1: THE LOCATION OF APERTURE FOR THIS comment_2: EXPOSURE COINCIDES WITH EXPOSURE comment_3: 115 ! linenum: 140.000 sequence_1: USE sequence_2: PCJUP-1 targname: JUPITER-PC-CYCL1 ! ! end of exposure logsheet ! No scan data records found