! Hubble Space Telescope Cycle 5 (1995) Phase II Proposal Template
! $Id: 5797,v 1.1 1994/12/14 19:16:35 pepsa Exp $
!
!   Refer to the HST Phase II Proposal Instructions to fill this out
!
!   Anything after a "!" is ignored, and may be deleted
!
!   All keywords with multiple entries are comma delimited except the
!   Visit_Requirements and Special_Requirements keywords which can be
!   delimited with carriage returns or semi-colons, but not commas
!
! For help call your Program Coordinator: n/a
!             Phone: n/a             , E-mail: n/a
!
! This partially completed template was generated from a Phase I proposal.
! Name of Phase I Proposal: harris-836.prop
! Date generated: Wed Dec 14 14:16:27 EST 1994
!

Proposal_Information                           ! Section 4
              Title:  Mapping Latitude Bands and the Great Red
                      Spot of Jupiter in the near and far UV
  Proposal_Category:  AR
Scientific_Category:  Solar System
             Cycle:    5

Investigators
     PI_name:         Walter M. Harris
     PI_Institution:  University of Michigan

          CoI_Name:   John Clarke
   CoI_Institution:   University of Michigan
           Contact:             ! Y or N (designate at most one contact)

          CoI_Name:   Gilda Ballester
   CoI_Institution:   University of Michigan
           Contact:             ! Y or N (designate at most one contact)

          CoI_Name:   G. Randall Gladstone
   CoI_Institution:   Southwest Research Institute
           Contact:             ! Y or N (designate at most one contact)


Abstract:                                ! Free format text (please update)
    Spectroscopy of the Jovian upper atmosphere in the NUV/FUV
    spectral range provides information about the structure,
    dynamics and atmospheric composition from the troposphere to
    the upper stratosphere.  Recent advances in our observational
    capabilities in the FUV/NUV range have now made tenable the
    additional study of the latitudinal structure of the Jovian
    upper atmosphere relative to the visible zone and belts.  The
    primary advances allowing this new research have come from the
    FOS, which provides much higher quality spectra than had been
    previously obtained from Jupiter in this band pass, and from
    the WFPC-II, which can now image the Jovian atmosphere in the
    UV.  There is clear evidence of banded structure in WFPC-II
    images of Jupiter extending wavelengths to below 1800.  The
    great red spot (GRS) is also visible in these images. We
    propose a program to compare images of the GRS and this banded
    structure with archived FOS spectra taken at several different
    latitudes and at the GRS.  We will also compare the FOS
    spectra with an IUE albedo map obtained in early July of this
    year.  We will develop a new model for the removal of grating
    light in the FOS, compare the results of the subtraction with
    first with IUE spectra taken at similar locations and then
    with structure seen in the images.  Lastly, we will develop
    and apply photochemical models to the FOS albedo spectra with
    the goal of determining the nature of the absorbing material.

Questions                       ! Free format text (please update)

     Observing_Description:

   Real_Time_Justification:



Calibration_Justification:              ! Move appropriate text from Real_Time_Justification

      Additional_Comments:


Fixed_Targets                           ! Section 5.1
  Target_Number:
    Target_Name:
Alternate_Names:
    Description:
       Position:                        ! Most common specification format is
                                        ! RA=0H 0M 0.00S +/- 0S,
                                        ! DEC=0D 0' 0.0" +/- 0",
                                        ! PLATE-ID=0000
        Equinox:
        RV_or_Z:
          RA_PM:                        ! Units are seconds of time per year
         Dec_PM:                        ! Units are seconds of arc per year
          Epoch:
Annual_Parallax:
           Flux:                        ! Include at least V and B-V
       Comments:


Solar_System_Targets                    ! Section 5.2
  Target_Number:
    Target_Name:
    Description:
        Level_1:                        ! Satellite of Sun
        Level_2:                        ! Satellite of Level_1
        Level_3:                        ! Satellite of Level_2
         Window:
           Flux:                        ! Include at least V and B-V
       Comments:


Generic_Targets                         ! Section 5.3
  Target_Number:
    Target_Name:
    Description:
       Criteria:
           Flux:
       Comments:


Scan_Data                               ! Appendix B
    Scan_Number:
       FGS_Scan:
  Cont_or_Dwell:
   Dwell_Points:
     Dwell_Secs:
     Scan_Width:
    Scan_Length:
    Sides_Angle:
   Number_Lines:
      Scan_Rate:
  First_Line_PA:
     Scan_Frame:
  Length_Offset:
   Width_Offset:


! This is a template for a single visit containing a single exposure
! Repeat exposure and visit blocks as needed

Visits                                  ! Section 6
      Visit_Number:
Visit_Requirements:                     ! Section 7.1

! Uncomment or copy visit level special requirements needed
! Most of these requirements (including ORIENT) will limit scheduling

        ! PCS MODE [Fine | Gyro]
        ! GUIDing TOLerance <angle>
        ! ORIENTation <angle1> TO <angle2>
        ! ORIENTation <angle1> TO <angle2> FROM <visit>
        ! ORIENTation <angle1> TO <angle2> FROM NOMINAL
        ! SAME ORIENTation AS <visit>
        ! CVZ
        ! PARallel
        ! AFTER <visit> [BY <time1> [TO <time2>]]
        ! AFTER <date>
        ! BEFORE <date>
        ! BETWEEN <date1> AND <date2>
        ! GROUP <visit-list> WITHIN <time>
        ! PERIOD <time> AND ZERO-PHASE <date>
        ! SEQ <visit-list> WITHIN <time>
        ! ON HOLD [FOR <visit>]

  On_Hold_Comments:
    Visit_Comments:

     Exposure_Number:                   ! Section 6.5
         Target_Name:
              Config:
              Opmode:
            Aperture:
          Sp_Element:
          Wavelength:
 Optional_Parameters:
Number_of_Iterations:
   Time_Per_Exposure:
Special_Requirements:                   ! Section 7.2

! Uncomment or copy exposure level special requirements needed

        ! INTeractive ACQuisition FOR <exp-list>
        ! ONBOARD ACQuisition FOR <exp-list>
        ! POSition TARGet <x-value>,<y-value>
        ! SAME POSition AS <exp>
        ! DO FOR TARGets <targ-list>    ! FGS only
        ! PARallel WITH <exp>
        ! GROUP-FGS <exp-list> WITHIN <time>
        ! SPATIAL SCAN <#> [<exp-list> | SINGLE-EXP ]
        ! RT ANALYSIS [FOR <exp-list>]
        ! REQuires UPLINK
        ! DARK TIME
        ! END ORBIT
        ! EXPAND
        ! MAXimum DURation [<time> | <%>]
        ! MINimum DURation [<time> | <%>]
        ! NO SPLIT
        ! PHASE <number1[0,1]> TO <number2[0,1]>
        ! SEQuence <exp-list> NON-INTerruptible

            Comments:

Data_Distribution                       ! Defaults indicated; change if desired

         Medium:        8MM             ! 8MM or 6250BPI or 1600BPI
Blocking_Factor:        10              ! 10 or 1
                                        ! Only astronomers with very old 9-
                                        ! track tape drives should consider
                                        ! a blocking factor of 1

        Ship_To:        PI_Address      ! STSCI or PI_Address or <free-text>
                                        ! PI Address from Phase I is:
                                        !
                                                 !  Space Research Bldg. 2455 Haywa
                                                 !  rd, Ann Arbor, MI 48109-2143
                                        !
                                        !
       Ship_Via:        UPS             ! UPS (2-day) or OVERNIGHT
                                        ! Overnight shipping done at PI expense

Recipient_Email:                        ! Needed if Ship_To: is not PI_Address
                                        ! <free-text>

! Let us know what you think of this template and software!
! Please send a list of your likes and dislikes to your Program Coordinator