DATA_SET_DESCRIPTION |
Data Set Overview
=================
The UltraViolet Spectrometer (UVS) on the Galileo spacecraft took
unique data of Comet Shoemaker-Levy/9's impact with Jupiter. A
preliminary analysis of this data is presented in this submission to
the Planetary Data System (PDS). It consists of two small tables
with detached labels and documentation.
Background
==========
Galileo observed the S-L9 fragment G impact by oscillating the
scan-platform so that the fields of view of the scan-platform
instruments moved to-and-fro across Jupiter. Each to-and-fro 'swath'
lasted 10 2/3 sec, and consisted of two 5 1/3 sec 'passes'.
During the observations, the UVS acquired one measurement every 7.6
msec (more precisely, 4.0/528 sec); during each measurement, the
counting gate was open for 6.0 msec. Thus, each 10 2/3 sec swath
contained 1408 6-msec samples. The data-taking was, however, not
continuous, and the data received was occasionally corrupted. The
data presented here and used in Hord et al. (1995) [HORDETAL1995]
has all been inspected and verified.
Tables in the Dataset
=====================
The following is a list of the UVS data files for the Shoemaker-Levy
fragment R and G impacts. Each file record represents one UVS RIM of
fourteen spectra, with a duration of 60.666 seconds.
FILENAME FIRST RECORD STARTS AT LAST RECORD STARTS AT
SCLK SCLK AT SPACECRAFT
UTC UTC AT SPACECRAFT
------------------------------------------------------------------------
Experimenter Data Records (EDRs)
GFRAGTIM.DAT 2486477:00 2486487:00
1994-199//07:02:14.445 1994-199//07:12:21.112
RFRAGTIM.DAT 2490632:00 2490643:00
1994-202//05:03:24.284 1994-202//05:14:31.617
Details of the structure and contents of these tables may be found
in the discussion below as well as in the detached PDS label.
GFRAGTIM.DAT
------------
This file contains the G fragment data and a timescale. Each record
has a 10 point header and 8008 data points.
Record 0 is the time scale. Each position holds the number of
seconds from the start of the rim for the corresponding position in
a data record. The header values of this record are zeros.
Records 1 to 11 contain all data records. The data starts at
position 10. All fiducials (except the 1st one in each Rim) have
been replaced with 44 -1's and there are an additional 84 -1's at
the end of each record to represent the 84 missing bytes in the last
spectra.
Header info for data records:
0 = rim timetag (Spacecraft Event Time)
1-5 contain the SCET converted to UTC format; value is at the s/c
1 = year
2 = day of year
3 = hours
4 = minutes
5 = seconds
6 = time value in seconds used to convert from SCET to earth based
observation time.
NOTE: There is a single -1 in record 6. This is a noise point
changed by hand. Its previous value was 33. Also, there is data for
the end of rim 2486485, but JPL made an error when they made the
file containing it so it is not included in this file. There are 2
fiducials 3 minor frames apart. It looks like a piece of data was
written at an incorrect time position, over the top of data already
there.
RFRAGTIM.DAT
------------
This file contains the R fragment data and a timescale. Each record
has a 10 point header and 8008 data points.
Record 0 is the time scale. Each position holds the number of
seconds from the start of the rim for the corresponding position in
a data record. The header values of this record are zeros.
Records 1 to 9 contain all data records. The data starts at position
10. All fiducials have been replaced with 44 -1's and there are an
additional 84 -1's at the end of each record to represent the 84
missing bytes in the last spectra.
Header info for data records:
0 = rim timetag (Spacecraft Event Time)
1-5 contain the SCET converted to UTC format
1 = year
2 = day of year
3 = hours
4 = minutes
5 = seconds
NOTE: Record 4 is timetagged 2490635:00 and record 5 is 2490639:00.
This three rim gap is the result of a change in the playback
requested by NIMS. At this time, there is no data for record 8
(2490642).
Processing
==========
These files were produced by the Galileo UVS/EUV team at the
Laboratory for Atmospheric and Space Physics at the University of
Colorado at Boulder. The data contained in the files were generated
during the analysis of UVS data from the Shoemaker-Levy 9 comet
Fragment G Jupiter impact. This analysis is reported in Geophysical
Research Letters, Vol 22, No. 12, pages 1565-1568, June 15, 1995, by
C.W. Hord, et al. [HORDETAL1995]
Software
========
The two tables in this dataset are small and in binary (XDR)
format.
Media/Format
============
This dataset is an electronic submission to PDS but may be included
on a future CD-ROM volume of UVS data from the Jupiter Tour. Formats
are based on standards for table objects established by PDS.
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