DATA_SET_DESCRIPTION |
Data Set Overview
=================
This dataset contains color mosaics produced from Pancam images
of the Mars Exploration Rover mission. These products were
generated by Jim Bell and Jonathan Joseph of the Pancam science
team.
Processing
==========
Individual raw Pancam Experiment Data Records (EDRs) were
calibrated to radiance, radiance factor, and estimated Lambert
Albedo following the methods described in BELLETAL2006. They were
then map projected into simple cylindrical and/or vertical
projection mosaics using software specifically designed for
mosaicking of MER/Pancam images, and developed under the direction
of Pancam Payload Element Lead Prof. Jim Bell. The mapping
software uses information from the geometric calibration of the
cameras to correct for slight lens distortions. Slight variations
in lighting conditions among images within a mosaic have been
corrected using small automated and/or manual multiplicative
scaling of individual frames to achieve output mosaics that are as
seamless as possible. Large variations in lighting conditions, for
example in mosaics spanning a large range of Martian local solar
time or spanning multiple Martian days, have not been corrected.
Additional post-processing using commercial image processing tools
like Adobe Photoshop has been applied to many of these mosaics in
order to filter out single or small groups of 'hot pixels' or to
attempt to manually correct particularly harsh seam boundaries.
For some mosaics including the horizon, choppy or limited coverage
of the sky has been replaced with a representation of the way the
sky would have appeared if the coverage had been complete, using
actual sky colors from the data's original partial sky coverage.
These archived mosaics were created primarily for public education
and outreach purposes, and have been created in false color,
approximate true color, and red/blue 3-D anaglyph representations.
Substantial additional information and details about these mosaics
can be found online on the Pancam Home web site at
http://pancam.sese.asu.edu/, following the 'Images' link.
Additional details about true color representations of the Martian
landscape can be found in BELLETAL2006 and BELLETAL2006B. While
they can serve some potential scientific interests (such as basic
assessments of geology and geomorphology), because of the
sometimes rather qualitative post-processing applied to many of
these Pancam mosaics, they should not be used for quantitative
image analysis work.
File Naming
===========
The PDS file naming scheme adopted for these mosaics begins with
either a target name assigned by the MER team, the name of the
large-format mosaic or panorama assigned by the MER team, or a
simple sol, rover (A = Spirit, B = Opportunity), and Pancam
sequence designator (Pnnnn). This is often followed by a brief
indicator of the specific camera (L = left or R = right) and
filter (numbers 1-7) indicator, using the filter designation codes
described in BELLETAL2003. Finally, a designator is often provided
to identify the image as a false color composite (F), an
approximate true color composite (ATC), or an anaglyph (ANA or
STEREO) intended to be viewed with red/blue glasses (red on the
left).
For example:
SOL2642B_P2354_L257F:
Opportunity sol 2642, Pancam sequence 2354, left camera, false
color composite RGB from filters L2, L5, and L7.
SOL661A_P2401_L256ATC:
Spirit sol 661, Pancam sequence 2401, left camera, approximate
true composite RGB from filters L2, L5, and L76.
THANKSGIVING_STEREO:
The Spirit rover's 'Thanksgiving Panorama', details of which
can be found at http://pancam.sese.asu.edu/, following the
'Images' link, choosing the '360 deg. Panoramas' link, then
clicking on the 'Thanksgiving Pan' link.
BURNS_CLIFF_L257F.TIF:
The Opportunity rover's 'Burns Cliff' mosaic, details of which
can be found at http://pancam.sese.asu.edu/, following the
'Images' link, choosing the 'Small Panoramas and Mosaics'
link, then clicking on the 'Burns Cliff 180 deg.' link. This
is a false color mosaic acquired in the Pancam left camera's
filters L2, L5, and L7.
Point of Contact for More Details
=================================
Prof. Jim Bell
School of Earth & Space Exploration
Arizona State University
Box 876004, Tempe, AZ 85287-6004
email: Jim.Bell@asu.edu
Office: (480) 965-1044
|