DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data set contains images where multiple frames are mosaicked
into a single RDR product. The methods for this process are applied
by MIPL under OPGS, associating projections with the mosaicking
process. It should be noted that these processes can be independent,
and that governing methods and software can differ between OPGS and
the other science instrument teams. For instance, it is possible
that OPGS and other science teams' software will transform individual
images to one of the projections discussed below, without involving
any mosaicking. Detailed mathematical descriptions of the mosaic
projections and algorithms will be available in a separate paper
'Mars Mosaic Projection Algorithms.'
More information is found in ALEXANDERETAL2008, BOSETAL2007, and
KELLERETAL2008.
Processing
==========
The following is a description of each mosaic:
- Cylindrical Projection: the image is overlaid onto azimuth and
elevation grid lines, with individual frame boundries super
imposed and annotated by number. In this case each pixel
represents a fixed angle in azimuth and elevation. Rows are of
constant elevation in Mars coordinates. The horizon is level, and
columns begin clockwise from Mars north.
- Camera Point Perspective: a perspective projection with horizontal
epipolar lines. The image view is as if the camera had a much
larger field of view.
- Cylindrical-Perspective Projection: a 360 degree view projection
similar to the Point Perspective mosaic except that this is like a
pinhole camera which follows the mosaic in azimuth. The horizon is
not level in order to preserve epipolar viewing.
- Polar Projection: concentric circles represent constant projected
elevation. Mars nadir is at the convergent center and the horizon
is corrected for lander tilt. North is up.
- Vertical Projection: the creation of this type of mosaic assumes
that the field is a plane tangent to the Martian surface with up
pointing north. This is not an orthorectified rendering, but was
found to be useful for rapid initial orientation.
- Orthographic Projection: this type of mosaic is a generalization
of the vertical projection intended primarily for use with
Microscopic Imager data. It differs in that an arbitrary axis of
projection (as well as X- and Y-axes in the plane of projection)
can be specified.
- XYZ: this mosaic contains XYZ values for each pixel in the mosaic
rather than intensity values. The inputs to the mosaic program are
XYZ files (or individual X, Y, or Z components), and the pixels
are interpreted in the same way - as the coordinate of the
corresponding pixel in Cartesian space. Like XYZ images, they may
consist of a single 3-band file with X, Y, and Z components, or
separate 1 band files for each component. XYZ mosaics can be
produced in any of the mosaic projections. Note: these mosaics
have a consistent coordinate system used applied to each input
image; the output mosaic may have only one coordinate system in
which the XYZ values are defined.
- Surface Normal (UVW): similar in concept to XYZ mosaics, a UVW
mosaic is simply a mosaic created from UVW (surface normal) input
images. The pixels represent the surface normals at each point.
Like Surface Normal (UVW) images, they can be single 3-band files
or separate 1-band files for each component. As with XYZ mosaics,
any projection may be used, and all output values must be defined
in the same coordinate system.
Data
====
1 or 3 16-bit signed integer or Float, PDS (SOAS) or dual PDS/VICAR
(OPGS) binary file.
Software
========
The MIPL Mars Program Suite was used to generate these RDRs.
Media/Format
============
The data set will initially be delivered and kept online. Upon
Mission completion, the RAC Operations RDRs will be delivered to PDS
on DVD.
|