DATA_SET_DESCRIPTION |
Data Set Overview
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This data set is a digital archive of images acquired by the
Viking Orbiter 1 and 2 spacecraft. The archive will include
the best available Experiment Data Record (EDR) versions of
images acquired by the Viking Orbiter Visual Imaging Subsystems
(VIS). The archive is stored on compact read-only optical disk
media (CD-ROM) for distribution. The EDR image data are stored
on CD-ROM in a compressed format that allows exact
reconstruction of the original image. The images were
compressed in order to reduce the number of CD-ROMs required
for the archive. The average Viking Orbiter image is
compressed by a factor of about 3.5. Each CD-ROM in the
archive also includes documentation about the organization and
contents of the disk. Software is included to provide
programmers with tools to decompress image files. The CD-ROM
has index files containing information about all the images
stored in the archive. These index files can be loaded into a
database management system to help the user locate images of
interest.
The EDR images in this archive have not been processed in any
form other than organizing the original telemetry into raster
formatted files and compressing the image data using a Huffman
encoding algorithm. The reason for distributing unprocessed
data rather than processed versions of the images is that the
calibration files and processing procedures will continue to
evolve. This is due to improvements, not only in the
procedures, but also in the radiometric calibration data and in
the geometric information concerning spacecraft position and
pointing. By providing unprocessed images, improved image
processing capabilities can be reapplied to the original
unprocessed data.
To make full scientific use of the image collection, it is
necessary to understand the radiometric and geometric
properties of the Viking Orbiter imaging systems and to perform
corrections to the EDR data. A number of image processing
systems are available that provide radiometric and geometric
corrections, display capabilities, and analysis tools for
planetary images. Further information on processing Viking
Orbiter image data and the necessary radiometric and geometric
calibration data is available through the PDS Image Node at the
U.S. Geological Survey in Flagstaff, Arizona.
Processing Level Id : 2
Software Flag : N
Processing Start Time : 1990-11-01
Processing Stop Time : UNK
Parameters
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Description
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Data Number is an integer expressing the digital value of an
experiment's telemetry data.
Sampling Parameter Name : PIXEL
Data Set Parameter Name : DATA NUMBER
Data Set Parameter Unit : DIMENSIONLESS
Noise Level : UNK
Source Instrument Parameters
============================
Instrument Host ID : VO1
Data Set Parameter Name : DATA NUMBER
Instrument Parameter Name : RADIANCE
Important Instrument Parameters : 1
Instrument Host ID : VO2
Data Set Parameter Name : DATA NUMBER
Instrument Parameter Name : RADIANCE
Important Instrument Parameters : 1
Processing
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Processing History
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Source Data Set ID : MASTER DATA RECORD (MDR)
Software : UNK
Product Data Set ID : VO1/VO2-M-VIS-2-EDR-V2.0
Source Data Set ID : VO1/VO2-M-VIS-2-EDR-V1.0
Software : UNK
Product Data Set ID : VO1/VO2-M-VIS-2-EDR-V2.0
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CONFIDENCE_LEVEL_NOTE |
Overview
========
In the process of preparing the EDR images for inclusion in
this data set, several steps were taken to insure that the best
available image data and label information were archived. The
primary digital data source was a collection of magnetic tapes
produced by the Planetary Image Conversion Task. These tapes,
also known as the Planetary Archive tapes, constitute PDS
Version 1 of the Viking Orbiter image data set (PDS data set id
'VO1/VO2-M-VIS-2-EDR-V1.0'). The data on the Planetary Archive
tapes were derived from EDR tapes. The quality of the image
data on the Planetary Archive tapes was checked for problems
such as missing lines, segments of data from other images, and
mismatched images and labels. Some of the images received on
Earth were not available on these Planetary Archive tapes. In
addition, some Viking Orbiter images were never transferred to
EDR tapes. For images with data problems and for images not
available from either tape source, attempts were made to
retrieve the data from the Viking Master Data Record (MDR)
tapes. The accuracy of the image description keywords in the
image label was verified by comparing data from several
sources. These sources included the PDS Central Node image
catalog, image labels on the Planetary Archive tapes, and
Mission Test and Imaging System (MTIS) photoproducts. In cases
where there were discrepancies among the sources, label values
were chosen that occurred most frequently among the sources,
maintained consistency among images within a sequence, and
agreed with the VIS team planning notes. For example, a
discrepancy in exposure duration for an image might be resolved
by choosing the value of exposure duration for other images in
the same sequence. If a discrepancy could not be resolved,
that keyword was assigned the value 'UNKNOWN'. As a check on
the data compression procedure, each image was decompressed and
compared to the original image. The compressed image file was
accepted only if the results of decompression exactly matched
the original image data.
Many Viking Orbiter images are missing data and contain some
amount of noise. A common pattern of missing data is a series
of vertical bars with zero value pixels spaced at an interval
of 7 samples. The 7-sample interval results from the raw data
being stored on the spacecraft and transmitted to Earth in
packets that contained every seventh pixel. In addition, data
for a few horizontal image lines may be missing and such lines
are filled with zero values. The types of noise found in
Viking Orbiter images include single-pixel random noise and
several sources of coherent noise. The random noise is usually
due to telemetry errors. The coherent noise arises from
shuttering of the adjacent camera, filter wheel stepping, and
scan platform movements. If the amount of missing data and
noise is large, noise removal procedures may be needed to make
the image viewable. Box filtering techniques that fill in zero
values or average the bright and dark spikes of random noise
are often successful at noise removal.
It should be noted that the START_TIME and the STOP_TIME in the
PDS catalog, with values 1976-06-22T17:59:00.469Z and
1980-07-30T22:14:59.469Z respectively, are the times associated
with the version 1 data set VO1/VO2-M-VIS-2-EDR-V1.0. These
times are approximately correct for the current data set but
will be known more accurately only after data processing has
been completed. PDS labels embedded in each image file and the
index tables on the CD-ROM contain the exact times associated
with each image.
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