!   $Id: 5534,v 4.1 1994/07/27 19:03:01 pepsa Exp $

coverpage:

  title_1:         FOS GEOMAGNETICALLY INDUCED IMAGE MOTION CHARACTERIZATION
    proposal_for:  CAL/FOS
    pi_fname:      ANNE
    pi_lname:      KINNEY
    pi_inst:       STSCI
    pi_country:    USA
    pi_phone:      410-338-4831
! end of coverpage

abstract:

    line_1:        Measurements of the image drift due to the geomagnetic field will
    line_2:        be made on the blue FOS detector. Maps of the aperture image, with TALED
    line_3:        illumination at approximately 3 minute intervals will be used to
    line_4:        determine the amount of motion in both X and Y directions. Spectra
    line_5:        obtained with the onboard calibration lamps in RAPID readout mode
    line_6:        will permit determination of the uniformity of the image drift across
    line_7:        the diode array and an accurate sensitivity and phase measurement.
    line_8:        The latter data will also be used to determine how well the effect can
    line_9:        be corrected and if second order effects (hysteresis, local field
    line_10:       distortion due to permeable materials in the vicinity of the Digicons,
    line_11:       influence of the S/C magnetic torquers) are substantial.

!
! end of abstract

general_form_proposers:

  lname:           KEYES
    fname:         CHARLES (TONY)
    inst:          STSCI
    country:       USA

!

  lname:           KINNEY
    fname:         ANNE
    title:         PI
    inst:          STSCI
    country:       USA

!

  lname:           KORATKAR
    fname:         ANURADHA
    inst:          STSCI
    country:       USA

!

  lname:           TAYLOR
    fname:         CINDY
    inst:          STSCI
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Aperture maps, with TALED illumination, will be obtained over a full orbit,
    line_2:        at approximately 3 minute intervals, to
    line_3:        determine amout of image drift due to the geomagnietic field in both X and Y
    line_4:        Digicon coordinate. A similar set of internal cal lamp spectra, obtained at
    line_5:        higher time resolution, will permit a more accurate characterization of the
    line_6:        effect, over the full length of the diode array.

!

  question:        5
    section:       1
    line_1:        All observations are internal and may be obtained under gyro control.

!

  question:        6
    section:       1
    line_1:        This test is not stray light sensitive. All observations are internal
    line_2:        cal lamp and TALED measurements.

!

  question:        7
    section:       1
    line_1:        Data reduction will be performed at STSCI.
    line_4:        This program will determine the parameters required to compute corrections
    line_5:        in both the X and Y coordinates for the geomagnetically induced image
    line_6:        drift. These corrections are required to properly reduce
    line_7:        subsequent science data.

!
!end of general form text

general_form_address:

  lname:           KINNEY
    fname:         ANNE
    category:      PI
    inst:          STSCI

!
! end of general_form_address records

! No fixed target records found

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    sequence_1:    DEFINE
    sequence_2:    Y-MAP
    targname:      TALED
    config:        #
    opmode:        IMAGE
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       32
    time_per_exp:  32S
    priority:      1
    param_1:       SUB-STEP=4,
    param_2:       Y-SIZE=24,
    param_3:       COMB=YES

!

    linenum:       2.000
    sequence_1:    DEFINE
    sequence_2:    SPEC
    targname:      WAVE
    config:        #
    opmode:        RAPID
    aperture:      0.3
    sp_element:    G270H
    num_exp:       1
    time_per_exp:  96M
    priority:      1
    param_1:       READ-TIME=40

!

    linenum:       200.000
    sequence_1:    USE
    sequence_2:    Y-MAP
    config:        FOS/BL
    req_1:         CYCLE 4/200.00-231.00
    comment_1:     ALL LINES SHOULD BE IN ONE SU

!

    linenum:       201.000
    sequence_1:    USE
    sequence_2:    SPEC
    config:        FOS/BL

!

    linenum:       210.000
    sequence_1:    USE
    sequence_2:    Y-MAP
    config:        FOS/BL

!

    linenum:       211.000
    sequence_1:    USE
    sequence_2:    SPEC
    config:        FOS/BL

!

    linenum:       220.000
    sequence_1:    USE
    sequence_2:    Y-MAP
    config:        FOS/BL

!

    linenum:       221.000
    sequence_1:    USE
    sequence_2:    SPEC
    config:        FOS/BL

!

    linenum:       230.000
    sequence_1:    USE
    sequence_2:    Y-MAP
    config:        FOS/BL

!

    linenum:       231.000
    sequence_1:    USE
    sequence_2:    SPEC
    config:        FOS/BL

!
! end of exposure logsheet

! No scan data records found