COVERPAGE: TITLE_1: THE NATURE OF THE VARIABLE INFALLING MATERIAL ON THE STAR TITLE_2: BETA PICTORIS: GHRS OBSERVATIONS SCI_CAT: Interstellar medium SCI_SUBCAT: Circumstellar matter PROPOSAL_FOR: GO TIME_CRIT:Y LONGTERM:3 PI_FNAME: Anne-Marie PI_MI: PI_LNAME: LAGRANGE PI_INST: 5428 PI_COUNTRY: FRANCE PI_PHONE: (33)76-51-42-03 HOURS_PRI:11.00 NUM_PRI:1 HRS: Y OFF_FNAME: Claude OFF_LNAME: BERTOUT OFF_TITLE: Director OFF_INST: 5428 OFF_ADDR_1: Groupe d'Astrophysique de Grenoble OFF_ADDR_2: Universite J. Fourier OFF_ADDR_3: BP-53X OFF_CITY: GRENOBLE-Cedex OFF_STATE: OFF_ZIP: F-38041 OFF_COUNTRY:FRANCE OFF_PHONE: (33)76-51-47-90 ABSTRACT: LINE_1:We propose to obtain spectroscopic diagnostics of the gaseous LINE_2:disk observed around the star Beta Pictoris. The high quality data LINE_3:obtained at the unprecedented resolution and sensitivity of the GHRS LINE_4:during our Cycle 2 observations under ID 3482, allowed us to clearly LINE_5:strengthen the idea that both the changes in spectral line shapes as LINE_6:well as the very presence of CI, CIV and CO simultaneously observed in LINE_7:the gaseous environment of the star may be explained by the evaporation LINE_8:of many kilometer sized bodies when approaching the star. LINE_9:In effect, bodies evaporating at larger distances produce an important LINE_10:gaseous disk responsible for the observed stable narrow absorption LINE_11:features in mainly neutral species (CI,FeI,MgI,CO) but also in more LINE_12:ionised species (CaII,MgII,FeII,even AlIII), while other bodies, LINE_13:falling almost directly onto the star, produce highly time variable LINE_14:absorption features only seen in the ionised species (CaII,MgII,FeII, LINE_15:AlIII,CIV). The purpose of this proposal is to study in detail the LINE_16:precise nature of these two different gaseous components. LINE_17:To link all our observations together and with previous studies, we LINE_18:will organise simultaneous, multisites ground based observations. LINE_19: LINE_20: GENERAL_FORM_PROPOSERS: LNAME:LAGRANGE FNAME:ANNE-MARIE MI: INST:5428 COUNTRY:FRANCE ESA: Y LNAME:BEUST FNAME:Herve INST: 5414 COUNTRY:FRANCE ESA:Y LNAME:DELEUIL FNAME:Magali INST: 5420 COUNTRY:FRANCE ESA:Y LNAME:FELDMAN FNAME:Paul INST: 2380 COUNTRY:USA ESA: LNAME:FERLET FNAME:Roger INST: 5436 COUNTRY:FRANCE ESA:Y LNAME:GRY FNAME:Cecile INST: 5420 COUNTRY:FRANCE ESA:Y LNAME:HOBBS FNAME:Lew INST: 1716 COUNTRY:USA ESA: LNAME:LISSAUER FNAME:Jack INST: 2988 COUNTRY:USA ESA: LNAME:McGRATH FNAME:Melissa INST: 3470 COUNTRY:USA ESA: LNAME:MOOS FNAME:Warren INST: 2380 COUNTRY:USA ESA: LNAME:VIDAL-MADJAR FNAME:Alfred INST: 5436 COUNTRY:FRANCE ESA:Y GENERAL_FORM_ADDRESS: ! The PI's address: LNAME:LAGRANGE FNAME:Anne-Marie MI: CATEGORY: PI INST:5428 ADDR_1: Groupe d'Astrophysique de Grenoble ADDR_2:Universite J. Fourier ADDR_3:BP-53X CITY:GRENOBLE-Cedex STATE: ZIP:F-38041 COUNTRY:FRANCE PHONE: (33)76-51-42-03 TELEX: LAGRANGE@GAG.OBSERV-GR.FR (INTERNET) ! FAX:(33)76-44-88-21 (FAX) ! The address of the primary contact for this proposal (if not PI): LNAME:LAGRANGE FNAME:Anne-Marie MI: CATEGORY: CON INST:5428 ADDR_1:Groupe d'Astrophysique de Grenoble ADDR_2:Universite J. Fourier ADDR_3:BP-53X CITY:GRENOBLE-Cedex STATE: ZIP:F-38041 COUNTRY:FRANCE PHONE:33-76-51-42-03 TELEX:LAGRANGE@GAG.OBSERV-GR.FR (INTERNET);33-76-44-88-21 (FAX) GENERAL_FORM_TEXT: QUESTION: 3 ! Description of proposed observations. SECTION: 1 ! Provide a detailed description of the proposed observing plan. ! This description is used during scheduling to ensure that the ! observations are implemented properly, so please answer with care. LINE_1:Our aim is to investigate the chemical composition and physical LINE_2:conditions in the beta Pictoris disk. Long exposures in the range LINE_3:1500-1650 A will be performed with G160M and SSA to investigate the LINE_4:CS lines of CO, CIV, CI and AlII. Two additionnal ECH-A spectra LINE_5:at 1544 and 1660 A will be taken if Side1 is available to LINE_6:investigate in more details the CIV and AlII lines. LINE_7:ECH-B spectra of MgII, AlIII, ZnII, SiII, MnII, NiII, and FeII LINE_8:(ground and metastable levels) will be performed. As already LINE_9:mentionned, these ECH-B spectra will be performed with LSA. LINE_10:Our experience with the HRS data is that it is mandatory for LINE_11:our scientific purpose to have better calibrations than the LINE_12:standard ones. We manage then to perform calibrations before each LINE_13:science exposure. LINE_14:Our experience with last data is that they can be interpreted LINE_15:into much more details if they have been taken at the same time. LINE_16:Indeed, days and sometimes hours time scale variability LINE_17:occur in those lines. As we manage to compare abondances of LINE_18:different elements and in the case of FeII, abundances of LINE_19:different levels, we need to have the data taken as close as LINE_20:possible in time. Also, the observing order is important. LINE_21:Note: this observing plan slightly differs from the one in phase1, LINE_22:according to the recommendations of TAC panel (no repeated LINE_23:exposures) QUESTION: 3 SECTION: 2 ! This is an example of how to append another section to a particular question. ! No more than 23 lines can be included in any one section, and no more than 2 ! sections per question are allowed. Delete any unused LINE_ keywords. QUESTION: 4 ! Justification of need for HST observations. SECTION: 1 LINE_1:Although a lot could be done from the ground, as we have demonstrated,it is LINE_2:clear that having access to essentially only the CaII H and K lines is a LINE_3:strong limitation. Having also used IUE to complement our observational LINE_4:approach we know exactly what line should be observed. It is clear however LINE_5:that IUE presents too severe limitations in both resolution and S/N to allow LINE_6:further progress. The number of diagnostic lines in the UV and the presence LINE_7:of line pairs with large differences in oscillator strength will give us a LINE_8:detailed view of the density, temperature, composition, and distribution of LINE_9:the circumstellar material, particularly during the variable events. It is LINE_10:clear that any ground-based or IUE observing plan could never give us such LINE_11:informations and our recent observations with GHRS prooved to be very LINE_12:efficient. QUESTION: 5 ! Description of special scheduling requirements. SECTION: 1 ! Describe any special scheduling requirements such as real-time, time-critical, ! dark time, uninterrupted, Target of Opportunity, or Continuous Viewing Zone ! observations. LINE_1:Scheduled observations with the GHRS should be made several months in LINE_2:advance in order to organize the simultaneous ground-based, multisites LINE_3:observations from various observatories: first in Chile, Australia, LINE_4:New Zealand and South Africa. LINE_5:For that reason the observations should be scheduled when the LINE_6:ground-based observations are more favorable (the period 1st--20st LINE_7:of December 1994 is then the most favorable). LINE_8:Because of rapid changes (days time scales) in the lines, the LINE_9:observations should be performed as a time-sequence. QUESTION: 6 ! Description of special calibration exposures. SECTION: 1 LINE_1:Our dec 92 observations with HST showed that we really need a LINE_2:calibration better than the routine calibrations. LINE_3:Calibrations will then be performed before each science exposure. QUESTION: 7 ! Data reduction and analysis plans. SECTION: 1 LINE_1:Our plan is to obtain from the STScI the calibrated science data which is LINE_2:provided as the output of the Routine Science Data Processing (RSDP) and LINE_3:Calibration Data Base Software (CDBS) software at the Institute. We have LINE_4:excellent computational facilities at our home institutions. The numerical LINE_5:analysis needed to analyse and interpret our data is straightforward and LINE_6:relatively simple, and the total amount of data to be processed is also very LINE_7:modest. QUESTION: 8 ! Additional comments or special requests. SECTION: 1 LINE_1:Simultaneous ground-based observations will be done during the HST LINE_2:ones. Our December 1992 experience showed that it is feasible to LINE_3:reserve the ground based telescope time ahead of time in the LINE_4:December period, and then try to schedule the ST at the proper time. LINE_5:Because we succeeded once, it is reasonable to think that for the LINE_6:next observations we will proceed in a similar manner provided the LINE_7:fact that scheduling is prepared well ahead in time. December 1994 LINE_8:will be the most convenient period. LINE_9:The US administrative PI is J. Lissauer. We require 90000$ funding LINE_10:for the Cycle 4. QUESTION: 9 ! Description of previous HST work. SECTION: 1 LINE_1:ID 1269: Far UV observations of the giant planets. LINE_2: Interplanetary/IS gas connection: search for the local cloud. LINE_3:ID 2251: The properties of Single Interstellar Clouds. LINE_4:ID 2442: Cometary Parent Molecules. LINE_5:ID 2481: HST Observations of Periodic Comets. LINE_6:ID 2536: Deuterium in the local interstellar gas. LINE_7:ID 2537: Physical conditions of interstellar gas within 50 pc. LINE_8:ID 2625: Excitation Processes for the Outer Planet UV Emissions. LINE_9:ID 2627: Io's Atmosphere and its Interaction with the Plasma Torus. LINE_10:ID 3064: HST Observation of Comet Levy (1990c) LINE_11:ID 3472: The Properties of Single Interstellar Clouds. LINE_12:ID 3616: The Upper Atmospheres of Uranus and Neptune. LINE_13:ID 3617: The Ultraviolet Emissions of Titan. LINE_14:ID 3618: Excitation Processes for the Outer Planet UV Emissions. LINE_15:ID 3707: HST Observations of Periodic Comets. LINE_16:ID 3993: The Properties of Single Interstellar Clouds. LINE_17:ID 4274: The interplanetary interstellar connexion. LINE_18:ID 4353: Hubble Space Telescope Imaging of Io. LINE_19:ID 4513: The volatile composition of new comets. LINE_20:ID 4545: Outgassing from Ceres. LINE_21:ID 4600: FUV Spectrscopy of Io's SO2 Atmosphere and Surface. LINE_22:ID 4798: The Properties of Single Interstellar Clouds. LINE_23:The present project is a continuation of the program ID 3482. QUESTION: 10 ! Resources to be supplied by investigator's institution(s). SECTION: 1 LINE_1:As indicated in item 7, extensive data analysis capabilities exist at all LINE_2:our home institutions. All proposers are appointed by CNRS or Universities, LINE_3:in France and in the USA. ! This is the end of the General Form FIXED_TARGETS: ! Replicate this section as needed for each Fixed Target. ! Delete this entire section if none of your targets are fixed targets. ! See Section 5.1 of the Proposal Instructions for detailed instructions. TARGNUM:1 NAME_1:HD39060 NAME_2:BETA-PICTORIS NAME_3:HR2020 DESCR_1:A,124,146,904,912,917 DESCR_2: DESCR_3: POS_1:RA = 05H 47M 16.97S +/- 0.1", POS_2:DEC = -51D 3' 58.6" +/- 0.1" POS_3: POS_4: EQUINOX:2000 PM_OR_PAR:Y POS_EPOCH_BJ:J POS_EPOCH_YR:2000.00 ! RA_PM_VAL: ! RA proper motion (arc-sec/yr), F4.4 ! RA_PM_UNCT: ! RA proper motion uncertainty, F4.4 ! DEC_PM_VAL: ! DEC proper motion value (arc-sec/yr), F4.4 ! DEC_PM_UNCT: ! DEC proper motion uncertainty, F4.4 AN_PRLX_VAL:0.060 AN_PRLX_UNCT:0.008 RV_OR_Z:V = +20 ACQPR_1: ACQPR_2: ACQPR_3: FLUXNUM_1: 1 FLUXVAL_1: V = 3.85 +/- 0.05 FLUXNUM_2: 2 FLUXVAL_2: B-V = 0.17 +/- 0.01 FLUXNUM_3: 3 FLUXVAL_3: F(1550) = 15 +/- 5 E-13 FLUXNUM_4: 4 FLUXVAL_4: F(1660) = 124 +/- 20 E-13 FLUXNUM_5: 5 FLUXVAL_5: F(1720) = 190 +/- 30 E-13 FLUXNUM_6: 6 FLUXVAL_6: F(1812) = 69 +/- 10 E-12 FLUXNUM_7: 7 FLUXVAL_7: F(1858) = 70 +/- 10 E-12 FLUXNUM_8: 8 FLUXVAL_8: F(2025) = 70 +/- 10 E-12 FLUXNUM_9: 9 FLUXVAL_9: F(2360) = 50 +/- 5 E-12 FLUXNUM_10: 10 FLUXVAL_10: F(2260) = 60 +/- 5 E-12 COMMENT_1:CONTINUUM FLUXES AND LINE COMMENT_2:DEPTHS ESTIMATED FROM HST COMMENT_3:OR IUE DATA COMMENT_4: F(1510) = 10 +/- 5 E-13 COMMENT_5: F(2580) = 40 +/- 5 E-12 COMMENT_6: F(2613) = 70 +/- 5 E-12 COMMENT_7: F(2730) = 80 +/- 5 E-12 COMMENT_8: F(2800) = 40 +/- 10 E-12 COMMENT_9: F(2625) = 80 +/- 10 E-12 COMMENT_10: F(2139) = 70 +/- 10 E-12 EXPOSURE_LOGSHEET: ! Replicate this section as needed for each exposure. ! See Section 6 for detailed instructions. LINENUM: 1.000 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ APERTURE: 2.0 SP_ELEMENT: MIRROR-A2 WAVELENGTH: PARAM_1: SEARCH-SIZE = 3, PARAM_2: BRIGHT=RETURN, PARAM_3: LOCATE = YES, NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_1: CYCLE 4 / 1-3.036; REQ_2: ONBOARD ACQ FOR 1.001; REQ_3: AT 24-NOV-1994 +/- 1D; REQ_4: SEQ 1-1.028; COMMENT_1: COUNT RATE FOR MIRROR A2 COMMENT_2: 16000 CNTS/S. STEP TIME IS COMMENT_3: 0.2S TO GIVE 3500 CNTS/STEP ! LINENUM: 1.001 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ/PEAKUP APERTURE: 0.25 SP_ELEMENT: MIRROR-A2 NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_1: ONBOARD ACQ FOR 1.010-1.015.; COMMENT_1: STEP TIME IS 0.2S ! LINENUM: 1.010 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: G160M WAVELENGTH: 1493.6 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_2: CALIB FOR 1.011 NO SLEW; ! LINENUM: 1.011 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 0.25 SP_ELEMENT: G160M WAVELENGTH: 1493.6 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 1000.0S S_TO_N: 40. S_TO_N_TIME: 6200.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 1.012 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: G160M WAVELENGTH: 1518.0 PARAM_1: FP-SPLIT=STD PARAM_2: COMB=FOUR PARAM_3: STEP-PATT=DEF NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 1.013 NO SLEW; ! LINENUM: 1.013 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 0.25 SP_ELEMENT: G160M WAVELENGTH: 1518.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 1000.0S S_TO_N: 40. S_TO_N_TIME: 6200.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 1.014 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: G160M WAVELENGTH: 1551.67 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 1.015 NO SLEW; ! LINENUM: 1.015 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 0.25 SP_ELEMENT: G160M WAVELENGTH: 1551.67 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: 40. S_TO_N_TIME: 6200.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 1.020 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-A WAVELENGTH: 1547.35 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: DEF PRIORITY: 1 REQ_2: CALIB FOR 1.021 NO SLEW; ! LINENUM: 1.021 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1547.35 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 3 TIME_PER_EXP: 1000.0S S_TO_N: 25. S_TO_N_TIME: 5600.0S FLUXNUM_1: 3 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 1.022 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-A WAVELENGTH: 1562.75 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: DEF PRIORITY: 1 REQ_1: CALIB FOR 1.023 NO SLEW; ! LINENUM: 1.023 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1562.75 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 3 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 1.024 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-A WAVELENGTH: 1612.2 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: DEF PRIORITY: 1 REQ_1: CALIB FOR 1.025 NO SLEW; ! LINENUM: 1.025 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1612.2 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: 15. S_TO_N_TIME: 1500.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE ! LINENUM: 1.026 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1547.35 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 1000.0S S_TO_N: 25. S_TO_N_TIME: 5600.0S FLUXNUM_1: 3 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 1.027 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1562.75 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 3 PRIORITY: 1 COMMENT_1: S/N PER DIODE ! LINENUM: 1.028 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1612.2 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: 15. S_TO_N_TIME: 1500.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 2.000 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ APERTURE: 2.0 SP_ELEMENT: MIRROR-A2 WAVELENGTH: PARAM_1: SEARCH-SIZE = 3, PARAM_2: BRIGHT=RETURN, PARAM_3: LOCATE = YES, NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_1: SEQ 2-2.062; REQ_2: ONBOARD ACQ FOR 2.01; REQ_3: AT 24-NOV-1994 +/- 1D; COMMENT_1: COUNT RATE FOR MIRROR A2 COMMENT_2: 16000 CNTS/S. STEP TIME IS COMMENT_3: 0.2S TO GIVE 3500 CNTS/STEP ! LINENUM: 2.010 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 1808.0 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 2.011 NO SLEW; REQ_2: AT 24-NOV-1994 +/- 1D; ! LINENUM: 2.011 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 1808.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 360S S_TO_N: 60 S_TO_N_TIME: 1040S FLUXNUM_1: 6 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 2.013 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 1821.8 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 2.014 NO SLEW; ! LINENUM: 2.014 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 1821.8 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 360.0S S_TO_N: 60 S_TO_N_TIME: 1040.0S FLUXNUM_1: 6 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 2.020 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2139.0 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 2 REQ_1: CALIB FOR 2.021 NO SLEW; ! LINENUM: 2.021 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2139.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 720.0S S_TO_N: 60. S_TO_N_TIME: 926.0S FLUXNUM_1: 10 PRIORITY: 2 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 2.030 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2061.2 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 2.0310 NO SLEW; ! LINENUM: 2.0310 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2061.2 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 600.0S S_TO_N: 60. S_TO_N_TIME: 387.0S FLUXNUM_1: 8 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 2.039 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ APERTURE: 2.0 SP_ELEMENT: MIRROR-A2 WAVELENGTH: PARAM_1: SEARCH-SIZE = 3, PARAM_2: BRIGHT=RETURN, PARAM_3: LOCATE = YES, NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_2: ONBOARD ACQ FOR 2.04; REQ_3: AT 24-NOV-1994 +/- 1D; COMMENT_1: COUNT RATE FOR MIRROR A2 COMMENT_2: 16000 CNTS/S. STEP TIME IS COMMENT_3: 0.2S TO GIVE 3500 CNTS/STEP ! LINENUM: 2.040 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2265.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 2.041 NO SLEW; ! LINENUM: 2.041 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2265.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 160.0S PRIORITY: 1 FLUXNUM_1: 10 ! LINENUM: 2.050 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 1859.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 2.051 NO SLEW; ! LINENUM: 2.051 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 1859.7 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 2 TIME_PER_EXP: 240.0S S_TO_N: 40. S_TO_N_TIME: 600.0S FLUXNUM_1: 7 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 2.060 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-A WAVELENGTH: 1670.65 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: DEF PRIORITY: 1 REQ_1: CALIB FOR 2.061 NO SLEW; ! LINENUM: 2.061 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1670.65 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 3 PRIORITY: 1 COMMENT_1: S/N PER DIODE ! LINENUM: 2.062 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-A WAVELENGTH: 1670.65 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 1200.0S S_TO_N: 15. S_TO_N_TIME: 1500.0S FLUXNUM_1: 4 PRIORITY: 1 COMMENT_1: S/N PER DIODE. ! LINENUM: 3.000 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ APERTURE: 2.0 SP_ELEMENT: MIRROR-A2 WAVELENGTH: PARAM_1: SEARCH-SIZE = 3, PARAM_2: BRIGHT=RETURN, PARAM_3: LOCATE = YES, NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_1: SEQ 3-3.036; REQ_2: ONBOARD ACQ FOR 3.01; REQ_3: AT 24-NOV-1994 +/- 1D; COMMENT_1: COUNT RATE FOR MIRROR A2 COMMENT_2: 16000 CNTS/S. STEP TIME IS COMMENT_3: 0.2S TO GIVE 3500 CNTS/STEP ! LINENUM: 3.010 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2800.0 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 3.011 NO SLEW; REQ_2: AT 24-NOV-1994 +/- 01D; ! LINENUM: 3.011 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2800.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 280.0S S_TO_N: 60. S_TO_N_TIME: 340.0S FLUXNUM_1: 8 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.015 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2265.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 3.016 NO SLEW; ! LINENUM: 3.016 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2265.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 160.0S PRIORITY: 1 FLUXNUM_1: 10 ! LINENUM: 3.020 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2485.7 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 3.021 NO SLEW; ! LINENUM: 3.021 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2485.7 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 180.0S S_TO_N: 50. S_TO_N_TIME: 150.0S FLUXNUM_1: 9 PRIORITY: 1 ! LINENUM: 3.0230 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2378.5 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 420.0S S_TO_N: 50. S_TO_N_TIME: 150.0S FLUXNUM_1: 9 PRIORITY: 1 ! LINENUM: 3.024 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACQ APERTURE: 2.0 SP_ELEMENT: MIRROR-A2 WAVELENGTH: PARAM_1: SEARCH-SIZE = 3, PARAM_2: BRIGHT=RETURN, PARAM_3: LOCATE = YES, NUM_EXP: 1 TIME_PER_EXP: 1.8S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 1 FLUXNUM_2: 2 PRIORITY: 1 REQ_2: ONBOARD ACQ FOR 3.025; REQ_3: AT 24-NOV-1994 +/- 1D; COMMENT_1: COUNT RATE FOR MIRROR A2 COMMENT_2: 16000 CNTS/S. STEP TIME IS COMMENT_3: 0.2S TO GIVE 3500 CNTS/STEP ! LINENUM: 3.025 TARGNAME: WAVE CONFIG: HRS OPMODE: ACCUM APERTURE: SC2 SP_ELEMENT: ECH-B WAVELENGTH: 2590.2 PARAM_1: FP-SPLIT=STD, PARAM_2: COMB=FOUR, PARAM_3: STEP-PATT=DEF, NUM_EXP: 1 TIME_PER_EXP: 109S PRIORITY: 1 REQ_1: CALIB FOR 3.026 NO SLEW; ! LINENUM: 3.026 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2590.2 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 180.0S S_TO_N: 60. S_TO_N_TIME: 110.0S FLUXNUM_1: 5 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.028 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2613.5 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 600.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 6 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.030 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2625.5 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 300.0S S_TO_N: 60. S_TO_N_TIME: 380.0S FLUXNUM_1: 9 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.032 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2717.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 180.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 7 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.034 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2728.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 300.0S S_TO_N: S_TO_N_TIME: FLUXNUM_1: 7 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! LINENUM: 3.036 TARGNAME: HD39060 CONFIG: HRS OPMODE: ACCUM APERTURE: 2.0 SP_ELEMENT: ECH-B WAVELENGTH: 2739.0 PARAM_1: STEP-PATT=DEF, PARAM_2: FP-SPLIT=STD, PARAM_3: COMB=FOUR, NUM_EXP: 1 TIME_PER_EXP: 300.0S S_TO_N: 50. S_TO_N_TIME: 140.0S FLUXNUM_1: 7 PRIORITY: 1 COMMENT_1: S/N PER DIODE. COMMENT_2: FLUXNUM REFERS TO THE COMMENT_3: ADDITIONNAL FLUXES IN COMMENT_4: COMMENTS LINES ! End of RPSS template