!  File:  1132C.PROP
!  Database:  PEPDB
!  Date:  16-FEB-1994:02:57:14

coverpage:

  title_1:         URANUS AND RINGS (WF/PC-28):
    title_2:       CYCLE 3 AND FUTURE-CYCLE CONTINUATION
    sci_cat:       SOLAR SYSTEM
    proposal_for:  GTO/WFC
    pi_title:      PROF.
    pi_fname:      JAMES
    pi_mi:         A.
    pi_lname:      WESTPHAL
    pi_inst:       CALTECH
    pi_country:    USA
    pi_phone:      (818)356-4900
    keywords_1:    URANUS, PLANETARY ATMOSPHERES, URANUS RING SYSTEM
    hours_pri:     2.00
    num_pri:       1
    pi_position:   PROFESSOR OF PLANEYA
! end of coverpage

abstract:

    line_1:        WF/PC obsevations will provide high-resolution images of Uranus and its rings
    line_2:        in spectral regions not covered by Voyager imaging cameras and/or not possible
    line_3:        from the Earth-based observations. At short wavelengths, the global
    line_4:        reflectivity of Uranus is less than that of a pure Rayleight atmosphere; thus
    line_5:        structure may be visible. The set of observations will be repeated one month
    line_6:        later to study secular changes. The ring system and the associated satellites
    line_7:        will be observed with the Planetary Camera.

!
! end of abstract

general_form_proposers:

  lname:           WESTPHAL
    fname:         JAMES
    mi:            A.
    inst:          CALTECH
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        2
    section:       1
    line_1:        WF/PC observations will provide high-resolution images of Uranus and its rings
    line_2:        in spectral regions not covered by Voyager imaging cameras and/or not possible
    line_3:        from the Earth-based observations. At short wavelengths, the global
    line_4:        reflectivity of Uranus is less than that of a pure Rayleigh atmosphere; thus
    line_5:        structure may be be visible. The set of observations will be repeated one
    line_6:        month later to study secular changes. The ring system ad the associated
    line_7:        satellites will be observed with the Planetary Camera.

!

  question:        3
    section:       1
    line_1:        WF/PC observations will provide high-resolution images of Uranus and its rings
    line_2:        in spectral regions not covered by Voyager. The set of observations will be
    line_3:        repeated one month later to study secular changes.
    line_5:        Observations to be done in cycle 9.

!

  question:        13
    section:       1
    line_1:        WF/PC observations will provide high-resolution images of Uranus and its rings
    line_2:        in spectral regions not covered by Voyager imaging cameras and/or not possible
    line_3:        from the Earth-based observations. At short wavelengths, the global
    line_4:        reflectivity of Uranus is less than that of a pure Rayleigh atmosphere; thus
    line_5:        structure may be visible. The set of observations will be repeated one month
    line_6:        later to study secular changes. The ring system and the associated satellites
    line_7:        will be observed with the Planetary Camera.

!
!end of general form text

general_form_address:

  lname:           GUNN
    fname:         JAMES
    mi:            E.
    category:      CON
    inst:          PRINCETON UNIVERSITY
    addr_1:        ASTROPHYSICAL SCIENCE
    addr_2:        PEYTON HALL
    city:          PRINCETON
    state:         NJ
    zip:           08540
    country:       USA
    phone:         (609)452-3802

!

  lname:           WESTPHAL
    fname:         JAMES
    mi:            A.
    title:         PROF.
    category:      PI
    inst:          CALTECH
    addr_1:        M/S 170-25
    addr_2:        DIVISION OF GEOLOGICAL
    addr_3:        & PLANETARY SCIENCES
    city:          PASADENA
    state:         CA
    zip:           91125
    country:       USA

!

  lname:           FABER
    fname:         SANDRA
    mi:            M.
    category:      CON
    inst:          UC SANTA CRUZ
    addr_1:        LICK OBSERVATORY
    addr_2:        NATURAL SCIENCE II, BLDG,160
    city:          SNTA CRUZ
    state:         CA
    zip:           95064
    country:       USA
    phone:         (408)429-2900

!

  lname:           DANIELSON
    fname:         G. EDWARD
    category:      CON
    inst:          CALTECH
    addr_1:        DIVISION OF GEOLOGICAL & PLANETARY SCIENCES
    addr_2:        M/S 170-25
    city:          PASADENA
    state:         CA
    zip:           91125
    country:       USA
    phone:         (818)3566861

!
! end of general_form_address records

! No fixed target records found

solar_system_targets:

  targnum:         1
    name_1:        URANUS
    descr_1:       PLANET URANUS
    lev1_1:        STD=URANUS

!
! end of solar system targets

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    sequence_1:    DEFINE
    sequence_2:    UWC
    targname:      #
    config:        WFC
    opmode:        IMAGE
    aperture:      WF1
    sp_element:    F284W
    num_exp:       1
    time_per_exp:  60S
    priority:      #
    param_1:       CR-SPLIT=NO, PRE-FLASH=YES
    req_2:         SEQ 1-4 NO GAP
    comment_1:     CYCLE 3-9 PROPOSAL VERSION
    comment_2:     3/25/92  17:05  TRL/RML.

!

    linenum:       2.000
    sequence_1:    ^
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    F230W
    num_exp:       1
    time_per_exp:  900S
    priority:      #
    param_1:       CR-SPLIT=0.50,
    param_2:       CR-TOLERANCE=0.0,
    param_3:       PRE-FLASH=YES

!

    linenum:       3.000
    sequence_1:    ^
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    F194W
    num_exp:       1
    time_per_exp:  1800S
    priority:      #
    param_1:       CR-SPLIT=0.50,
    param_2:       CR-TOLERANCE=0.0,
    param_3:       PRE-FLASH=YES

!

    linenum:       4.000
    sequence_1:    ^
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    F889N
    num_exp:       1
    time_per_exp:  300S
    priority:      #
    param_1:       CR-SPLIT=NO,
    param_2:       PRE-FLASH=YES

!

    linenum:       5.000
    sequence_1:    USE
    sequence_2:    UWC
    targname:      URANUS
    priority:      3
    req_1:         CYCLE 3 / 5-7

!

    linenum:       6.000
    sequence_1:    ^
    targname:      ^
    priority:      3
    req_1:         AFTER 5 BY 30D
    req_2:         +/-1D;

!

    linenum:       7.000
    targname:      URANUS
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F889N
    num_exp:       3
    time_per_exp:  60S
    priority:      2
    param_1:       CR-SPLIT=NO, PRE-FLASH=YES

!
! end of exposure logsheet

! No scan data records found