!   $Id: 5551,v 4.1 1994/07/27 19:13:19 pepsa Exp $

coverpage:

  title_1:         GHRS GIMP CHARACTERIZATION--CYCLE 4
    proposal_for:  CAL/HRS
    pi_fname:      STEPHEN
    pi_lname:      HULBERT
    pi_inst:       STSCI
    pi_country:    USA
    pi_phone:      301-338-4911
! end of coverpage

abstract:

    line_1:        Measurements of the image drift due to the geomagnetic field will
    line_2:        be made on the GHRS D2 detector. Maps of the spectral cal lamp image
    line_3:        made at approximately 1 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:           HULBERT
    fname:         STEPEHN
    inst:          STSCI
    country:       USA

!

  lname:           SODERBLOM
    fname:         DAVID
    inst:          STSCI
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Aperture maps will be obtained,
    line_2:        at four different S/C pointings, at approximately 1 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:        7
    section:       1
    line_1:        Data reduction and analysis will be performed at STSCI.

!
!end of general form text

general_form_address:

  lname:           HULBERT
    fname:         STEPHEN
    category:      PI
    inst:          STSCI
    addr_1:        3700 SAN MARTIN DR
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA
    phone:         301-338-4911

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NORTH
    pos_1:         RA = 00H 00M 00.0S +/- 1H,
    pos_2:         DEC = +90D 00' 00.0" +/- 1D,
    equinox:       2000
    comment_1:     NORTH CELESTIAL POLE

!

    targnum:       2
    name_1:        SOUTH
    pos_1:         RA = 00H 00M 00.0S +/- 1H,
    pos_2:         DEC = -90D 00' 00.0" +/- 1D,
    equinox:       2000
    comment_1:     SOUTH CELESTIAL POLE

!

    targnum:       3
    name_1:        EQ6
    pos_1:         RA = 06H 00M 00.0S +/- 1H,
    pos_2:         DEC = +00D 00' 00.0" +/- 1D,
    equinox:       2000
    comment_1:     POINT NEAR CEL EQUATOR

!

    targnum:       4
    name_1:        EQ12
    pos_1:         RA = 12H 00M 00.0S +/- 1H,
    pos_2:         DEC = +00D 00' 00.0" +/- 1D,
    equinox:       2000
    comment_1:     POINT NEAR CEL EQUATOR

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    sequence_1:    DEFINE
    sequence_2:    SC2MAP
    targname:      #
    config:        HRS
    opmode:        IMAGE
    aperture:      SC2
    sp_element:    MIRROR-N2
    num_exp:       30
    time_per_exp:  51.2S
    priority:      1
    param_1:       NX=16,NY=16
    param_2:       DELTA-X=2,
    param_3:       DELTA-Y=2,
    comment_1:     STEPTIME=0.2S

!

    linenum:       1.100
    sequence_1:    DEFINE
    sequence_2:    SC2MAP
    targname:      #
    config:        S/C
    opmode:        POINTING
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    priority:      1
    param_1:       CONTROL=GYRO

!

    linenum:       2.000
    sequence_1:    DEFINE
    sequence_2:    SC2MAP
    targname:      WAVE
    config:        HRS
    opmode:        RAPID
    aperture:      SC2
    sp_element:    G270M
    wavelength:    2900.2
    num_exp:       1
    time_per_exp:  25M
    priority:      1

!

    linenum:       2.100
    sequence_1:    DEFINE
    sequence_2:    SPEC
    targname:      #
    config:        S/C
    opmode:        POINTING
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    priority:      1
    param_1:       CONTROL=GYRO

!

    linenum:       100.000
    sequence_1:    USE
    sequence_2:    SC2MAP
    targname:      NORTH
    req_1:         GROUP 100-130 WITHIN 1D;
    req_2:         CYCLE 4 / 100-130;

!

    linenum:       110.000
    sequence_1:    USE
    sequence_2:    SC2MAP
    targname:      SOUTH

!

    linenum:       120.000
    sequence_1:    USE
    sequence_2:    SC2MAP
    targname:      EQ6

!

    linenum:       130.000
    sequence_1:    USE
    sequence_2:    SC2MAP
    targname:      EQ12

!
! end of exposure logsheet

! No scan data records found