!   $Id: 5783,v 4.1 1994/12/09 20:28:14 pepsa Exp $

coverpage:

  title_1:         ULTRAVIOLET IMAGERY OF VENUS
    sci_cat:       SOLAR SYSTEM
    sci_subcat:    INNER PLANETS
    proposal_for:  GO
    pi_fname:      Larry
    pi_mi:         
    pi_lname:      Esposito
    pi_inst:       U.COLORADO LASP
    pi_country:    USA
    hours_pri:     0.08
    num_pri:       1
    wf_pc:         N
    hrs:           Y
    time_crit:     Y
    funds_length:  12
    off_fname:     LAURENCE
    off_mi:        D
    off_lname:     NELSON
    off_title:     DIRECTOR
    off_inst:      1760
    off_addr_1:    OFFICE OF CONTRACTS & GRANTS
    off_city:      BOULDER
    off_state:     CO
    off_zip:       80309
    off_country:   USA
    off_phone:     303/492-3695
! end of coverpage

abstract:

    line_1:        We intend to make an ultraviolet image of Venus as a 
    line_2:        companion observation to prop 4518 HIGH RESOLUTION 
    line_3:        SPECTROSCOPY OF VENUS.
!
! end of abstract

general_form_proposers:

  lname:           ESPOSITO
    fname:         LARRY
    title:         PI
    mi:            W
    inst:          U.COLORADO LASP
    country:       USA

!

  lname:           NA
    fname:         CHAN
    mi:            Y
    inst:          U.COLORADO LASP
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        2
    section:       1
    line_1:        Paper copy only.

!

  question:        3
    section:       1
    line_1:        Image will be taken on gyros in the next orbit after the 
    line_2:        spectroscopy observations.
!

  question:        4
    section:       1
    line_1:        The observation of Venus in the middle UV is crucial.
!

  question:        5
    section:       1
    line_1:        Venus is most safely observed near its maximum elongation, when
    line_2:        it is furthest from the Sun. A short slew will allow pointing to
    line_3:        Venus while HST is in the Earth's shadow. Venus is more than 43
    line_4:        degrees from the Sun from 31 May 1993 to 12 July 1993.

!

  question:        6
    section:       1
    line_1:        None.

!

  question:        7
    section:       1
    line_1:        none
!

  question:        8
    section:       1
    line_1:        None.

!

  question:        9
    section:       1
    line_1:        None.

!

  question:        10
    section:       1
    line_1:        none.
!
!end of general form text

general_form_address:

  lname:           Esposito
    fname:         Larry
    mi:            W
    category:      PI
    inst:          U.Colorado LASP
    addr_1:        LASP
    addr_2:        Campus Box 392
    city:          Boulder
    state:         CO
    zip:           803090392
    country:       USA
    phone:         303/492-7325
    telex:         910/940-3441

!
! end of general_form_address records

fixed_targets:

  targnum:         3
    name_1:        VENUS+5D
    descr_1:       I,606
    pos_1:         RA = 235.1777384D +/- 0.00001D,
    pos_2:         DEC = -15.5724451D +/- 0.00001D
    equinox:       2000
    comment_1:     FIXED POINTING AT ELONG
    comment_2:     51.88 DEG FROM SUN ON 1/9
    comment_3:     AND GETTING FARTHER...

! end of fixed target records

solar_system_targets:

  targnum:         1
    name_1:        VENUS
    descr_1:       PLANET VENUS
    lev1_1:        STD = VENUS
    lev2_1:        TYPE = POS_ANGLE,
    lev2_2:        ANG = 0,
    lev2_3:        RAD = 5.9,
    lev2_4:        REF = SUN
    wind_1:        VENUS ELONGATION
    comment_1:     SUN REFERENCE MORE DIRECT
    comment_2:     THAN CELESTIAL REFERENCE
    comment_3:     SUGGESTED BY STORRS.
    fluxnum_1:     1
    fluxval_1:     F(2070) = 10 +/- 5 E-10

!  targnum:         2
!    name_1:        VENUS+5D
!    descr_1:       PLANET VENUS
!    lev1_1:        STD = VENUS
!    lev2_1:        TYPE = POS_ANGLE,
!    lev2_2:        ANG = 180,
!    lev2_3:        RAD = 5 D,
!    lev2_4:        REF = SUN
!    wind_1:        VENUS ELONGATION
!    comment_1:     SUN REFERENCE MORE DIRECT
!    comment_2:     THAN CELESTIAL REFERENCE
!    comment_3:     SUGGESTED BY STORRS.
!    COMMENT_4:     5 DEGREE ANTISUNWARD OFFSET
!    COMMENT_5:     FOR SAFE POINTING TEST.
!    fluxnum_1:     1
!    fluxval_1:     F(2070) = 10 +/- 5 E-10

!
! end of solar system targets

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      VENUS+5D
    config:        S/C
    opmode:        DATA
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    req_1:         CYCLE 4 / 1-4;
    req_2:         PCS MODE f;
    req_3:         SEQ 1-4 NO GAP;
    comment_1:     POINTING BEYOND 50 DEG
    comment_2:     SOLAR AVOIDANCE LIMIT.
    comment_3:     EACH LINE ITS OWN OBSET.
!
    linenum:       2.000
    targname:      VENUS
    config:        WFPC2
    opmode:        image
    aperture:      wf2
    sp_element:    f255w
    num_exp:       1
    time_per_exp:  2s
    PARAM_1:       clocks=yes
    param_2:       atd-gain=15
    param_3:       cr-split=no
    s_to_n:        25
    fluxnum_1:     1
    priority:      1
    req_1:         seq 2-3 non-int;
    req_2:         DARK TIME;
    req_3:         PCS MODE g;
    comment_1:     use gyros
!
    linenum:       3.000
    targname:      VENUS
    config:        WFPC2
    opmode:        image
    aperture:      wf2
    sp_element:    f218w
    num_exp:       1
    time_per_exp:  20s
    PARAM_1:       clocks=yes
    param_2:       atd-gain=15
    param_3:       cr-split=no
    s_to_n:        25
    fluxnum_1:     1
    priority:      1
    req_2:         DARK TIME;
    req_3:         PCS MODE g;
    comment_1:     use gyros
!
    linenum:       4.000
    targname:      VENUS+5D
    config:        S/C
    opmode:        DATA
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    req_2:         PCS MODE F;
    comment_1:     POINTING BEYOND 50 DEG
    comment_2:     SOLAR AVOIDANCE LIMIT.
    comment_3:     EACH LINE ITS OWN OBSET.

!

!
! end of exposure logsheet

! No scan data records found