!  File:  4001C.PROP
!  Database:  PEPDB
!  Date:  20-FEB-1994:03:20:35

coverpage:

  title_1:         H2 SURVEY OF JUPITER N. AURORA DURING ULYSSES FLYBY
    sci_cat:       SOLAR SYSTEM
    proposal_for:  GTO/HRS
    cont_id:       4001
    pi_fname:      LAURENCE
    pi_mi:         M.
    pi_lname:      TRAFTON
    pi_inst:       TEXAS, UNIVERSITY OF
    pi_country:    USA
    pi_phone:      (512) 471-1476
    keywords_1:    UV SPECTRA, UV EMISSION, PLANETARY
    keywords_2:    ATMOSPHERES
    hours_pri:     2.89
    num_pri:       2
    realtime:      0
    time_crit:     X
    pi_position:   RESEARCH SCIENTIST
! end of coverpage

abstract:

    line_1:        Measure the H2 northern auroral emission of Jupiter during Ulysses flyby.
    line_2:        The results will be compared with FOC images and Ulysses X-rays to establish
    line_3:        the mechanism of X-ray emission from Jupiter.

!
! end of abstract

general_form_proposers:

  lname:           TRAFTON
    fname:         LAURENCE
    mi:            M.
    inst:          TEXAS, UNIVERSITY OF
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Observe Jupiter's UV aurora with the HRS medium
    line_2:        resolution mode and large science aperture during Ulysses flyby.

!

  question:        4
    section:       1
    line_1:        UV required
    line_2:        spatial resolution required

!

  question:        5
    section:       1
    line_1:        Certain central meridian longitudes of Jupiter and Saturn are needed.
    line_2:        Tracking of auroral features need (planetary rotation).

!

  question:        6
    section:       1
    line_1:

!

  question:        7
    section:       1
    line_1:        Initial reductions at STScI;
    line_2:        Final reductions and analysis at Univ. Texas at Austin.

!

  question:        8
    section:       1
    line_1:

!

  question:        10
    section:       1
    line_1:        Cluster of VAX 11/780's and 6410.

!

  question:        13
    section:       1
    line_1:        A brief medium resolution H2 emission survey of Jupiter's northern
    line_2:        aurora will be attempted during the Ulysses flyby using the HRS
    line_3:        with G160M.

!
!end of general form text

general_form_address:

  lname:           TRAFTON
    fname:         LAURENCE
    mi:            M.
    category:      PI
    inst:          TEXAS, UNIVERSITY OF

!
! end of general_form_address records

! No fixed target records found

solar_system_targets:

  targnum:         1
    name_1:        JUPITER-QUIET
    descr_1:       FEATURE JUPITER
    lev1_1:        STD = JUPITER
    lev2_1:        TYPE = CARTO,
    lev2_2:        LONG = 280,
    lev2_3:        LAT = -5
    wind_1:        CML OF JUPITER FROM EARTH BETWEEN
    wind_2:        230 360
    comment_1:     OBSERVE JUPITER'S DAYGLOW AT LONG=
    comment_2:     280D + 80D -50D AND
    comment_3:     LAT= -5D +/- 5D.
    fluxnum_1:     1
    fluxval_1:     V=-2.5
    fluxnum_2:     2
    fluxval_2:     SURF(1216)=18+/-6E-12
    fluxnum_3:     3
    fluxval_3:     W-LINE(1216)=0.01
    fluxnum_4:     4
    fluxval_4:     SURF-BKG(1216)=7.6E-12
    fluxnum_5:     5
    fluxval_5:     SURF(1600)=2.3E-15

!

  targnum:         2
    name_1:        JUPITER-NPR
    descr_1:       FEATURE JUPITER
    lev1_1:        STD = JUPITER
    lev2_1:        TYPE = CARTO,
    lev2_2:        LONG = 180,
    lev2_3:        LAT = +60
    wind_1:        CML OF JUPITER FROM EARTH BETWEEN 125
    wind_2:        235
    comment_1:     BLINDLY OBSERVE JUPITER'S BRIGHT
    comment_2:     NORTHERN AURORA.
    fluxnum_1:     1
    fluxval_1:     V=-2.5
    fluxnum_2:     2
    fluxval_2:     SURF(1216)=50E-7
    fluxnum_3:     3
    fluxval_3:     W-LINE(1216)=0.01
    fluxnum_4:     4
    fluxval_4:     SURF(1600)=1.5E-14

!
! end of solar system targets

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      JUPITER-QUIET
    config:        HRS
    opmode:        WSCAN
    aperture:      2.0
    sp_element:    G160M
    wavelength:    1255-1285
    num_exp:       2
    time_per_exp:  17.5M
    fluxnum_1:     2
    priority:      1
    param_1:       WAVE-STEP=30.0
    req_2:         AT 08-FEB-92:19 +/- 3D;
    req_3:         CYCLE 1/1-6;
    req_4:         GROUP 1,2 NO GAP;
    comment_1:     OK TO TWEAK EXPOSURE TO FIT ORBIT

!

    linenum:       2.000
    targname:      JUPITER-QUIET
    config:        HRS
    opmode:        WSCAN
    aperture:      2.0
    sp_element:    G160M
    wavelength:    1575-1605
    num_exp:       2
    time_per_exp:  17.5M
    fluxnum_1:     2
    priority:      1
    param_1:       WAVE-STEP=30.0
    comment_1:     OK TO TWEAK EXPOSURE TO FIT ORBIT

!

    linenum:       3.000
    targname:      JUPITER-NPR
    config:        HRS
    opmode:        WSCAN
    aperture:      2.0
    sp_element:    G160M
    wavelength:    1255-1285
    num_exp:       2
    time_per_exp:  17.5M
    fluxnum_1:     2
    priority:      1
    param_1:       WAVE-STEP=30.0
    req_1:         AT 08-FEB-92:18.8 +/- 16H;
    req_2:         GROUP 3,4 NO GAP;
    comment_1:     ATTEMPT TO SPAN LINES 3 AND 4 ON
    comment_2:     TWO CONSEQUETIVE ORBITS ON 8 FEB
    comment_3:     BETWEEN 17:16 AND 20:22 UT (I.E.
    comment_4:     JUPITER CM SYSTEM III LONG.=140-
    comment_5:     236 DEG. IF NOT POSSIBLE, THEN
    comment_6:     HALVE EXPOSURE TIMES AND USE ONLY

!

    linenum:       4.000
    targname:      JUPITER-NPR
    config:        HRS
    opmode:        WSCAN
    aperture:      2.0
    sp_element:    G160M
    wavelength:    1575-1605
    num_exp:       2
    time_per_exp:  17.5M
    fluxnum_1:     2
    priority:      1
    param_1:       WAVE-STEP=30.0
    comment_1:     (CONT) ONE ORBIT, CENTERED ON 180 DEG.
    comment_2:     WILL THEN NEED TO HALVE SPECTRAL RANGE
    comment_3:     AND REPLACE WSCAN BY ACCUM MODE.
    comment_4:     WILL NEED TO KNOW POSITION OF LSA
    comment_5:     ON JUPITER A POSTERIORI
    comment_6:     TOLERANCE ON DATE IS REALLY +/- 1.6H

!

    linenum:       5.000
    targname:      WAVE
    config:        HRS
    opmode:        WSCAN
    aperture:      SC2
    sp_element:    G160M
    wavelength:    1255-1285
    num_exp:       1
    time_per_exp:  60S
    priority:      1
    param_1:       WAVE-STEP=30.0
    req_1:         CALIB FOR 1,3;
    req_2:         SEQ 3,5 NO GAP

!

    linenum:       6.000
    targname:      WAVE
    config:        HRS
    opmode:        WSCAN
    aperture:      SC2
    sp_element:    G160M
    wavelength:    1575-1605
    num_exp:       1
    time_per_exp:  60S
    priority:      1
    param_1:       WAVE-STEP=30.0
    req_1:         CALIB FOR 2,4;
    req_2:         SEQ 4,6 NO GAP

!
! end of exposure logsheet

! No scan data records found