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Modifying docs to represent changes from r905

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Zack Moratto
Zack Moratto committed Oct 23, 2009
1 parent 8c3c4a0 commit 50d0a93e9e84d38832364d396a1ac479a04f6074
Showing with 90 additions and 28 deletions.
  1. +34 −16 docs/book/examples.tex
  2. +56 −12 docs/book/tutorial.tex
@@ -54,18 +54,36 @@ \section{Mars Reconaissance Orbiter HiRISE}
At this time, we recommend mosaicking CCDs using the scripts available
at your institution (both USGS and University of Arizona have this
-capability). We are also providing a script that will take raw HiRISE
-images and combine them into a mosaic. Our script takes all red CCDs
-and projects them using the ISIS {\tt noproj} command into the
-perspective of RED5 CCD. From there, {\tt hijitreg} is performed to
-work out the relative offsets between CCDs. Finally the CCDs are
-mosaicked together using the average offset listed from {\tt hijitreg}
-using the {\tt handmos} command. Below is an outline of what our
-script does. It is based on the tutorial provided on the USGS ISIS
+capability). Having said that, we are also providing a script that
+will take raw HiRISE images and combine them into a mosaic name
+\texttt{}. Our script takes all red CCDs and projects
+them using the ISIS {\tt noproj} command into the perspective of RED5
+CCD. From there, {\tt hijitreg} is performed to work out the relative
+offsets between CCDs. Finally the CCDs are mosaicked together using
+the average offset listed from {\tt hijitreg} using the {\tt handmos}
+command. Below is an outline of what our script does. It is based on
+the tutorial provided on the USGS ISIS website.
- command outline
+ hi2isis # Import HiRISE IMG to Isis
+ spiceinit # Attach spice data
+ hical # Calibrate
+ histitch # Turn 20 files into 10
+ cubenorm # Remove boundary between histitchs
+ spiceinit
+ spicefit # For good measure
+ noproj # Project all images into perspective of RED5
+ hijitreg # Work out alignment between CCDs
+ handmos # Mosaic to single file
+ cubenorm # Clean up divisions
+To use our script, first go to the directory containing all of
+HiRISE's RED \texttt{IMG} files. Then feed the script one of those
+\texttt{IMG} files.
+ PSP_??????_????_RED?_?.IMG
Finally we recommend map projecting the product and normalizing both
@@ -150,8 +168,8 @@ \subsubsection*{Commands}
% Download all of the RED IMG for PSP_001513_1655 & %
% PSP_001777_1650 %
- ~/ PSP_001513_1655_RED0_0.IMG
- ~/ PSP_001777_1650_RED0_0.IMG
+ ~/ PSP_001513_1655_RED0_0.IMG
+ ~/ PSP_001777_1650_RED0_0.IMG
cam2map from=PSP_001513_1655_REDmosaic.norm.cub
cam2map from=PSP_001777_1650_REDmosaic.norm.cub ...
to=PSP_001777_1650_REDmosaic.norm.cub matchmap=true
@@ -262,8 +280,8 @@ \subsubsection*{Commands}
% Download all of the RED IMG for PSP_001364_2160 & %
% PSP_001760_2160 %
- ~/ PSP_001364_2160_RED0_0.IMG
- ~/ PSP_001760_2160_RED0_0.IMG
+ ~/ PSP_001364_2160_RED0_0.IMG
+ ~/ PSP_001760_2160_RED0_0.IMG
cam2map from=PSP_001364_2160_REDmosaic.norm.cub
cam2map from=PSP_001760_2160_REDmosaic.norm.cub ... matchmap=true
@@ -353,8 +371,8 @@ \subsubsection*{Commands}
% Download all of the IMG for PSP_001981_1825 & %
% PSP_002258_1825 %
- ~/ PSP_001981_1825_RED0_0.IMG
- ~/ PSP_002258_1825_RED0_0.IMG
+ ~/ PSP_001981_1825_RED0_0.IMG
+ ~/ PSP_002258_1825_RED0_0.IMG
cam2map from=PSP_001981_1825_REDmosaic.norm.cub
cam2map from=PSP_002258_1825_REDmosaic.norm.cub ... matchmap=true
@@ -103,7 +103,7 @@ \section{Preparing the Data}
images whose \ac{PDS} Product IDs are M01/00115 and E02/01461.
These data can be downloaded from the PDS directly, or they can be
found in the \texttt{data/MOC/} or the \texttt{examples/MOC/}
-directory of your Stere Pipeline distribution.
+directory of your Stereo Pipeline distribution.
These raw \ac{PDS} images (\texttt{M0100115.imq} and \texttt{E0201461.imq})
need to be imported into the \ac{ISIS} environment and radiometrically
@@ -147,13 +147,38 @@ \section{Preparing the Data}
\section{Running the Stereo Pipeline}
-The following example will utilize images from the example \ac{MOC}
-dataset, discussed above. The two example \ac{ISIS} 3 image files are
-\texttt{E0201461.cub} and \texttt{M0100115.cub}.
+For the rest of this chapter we'll show how to process data using a
+program called stereo with two different methods of rectifying the
+imagery. First we'll show how to run images that have been
+map-projected. Later we'll show how to use image that haven't been
+map-projected and are instead aligned using interest points. In both
+of these examples we'll be using the example MOC data set that was
+discussed above, \texttt{E0201461.cub} and \texttt{M010015.cub}.
+First we are going to add an addendum to preparing the data, we'll map
+project them. We could have used \texttt{mocproc} to map project the
+images in one go. Instead we'll call an \ac{ISIS} command called
+\texttt{cam2map}. This has the added advantage of allowing us to use
+the same map projection settings for both files, meaning that both map
+images will share the same origin.
+ ISIS 3> cam2map from=M0100115.cub
+ ISIS 3> cam2map from=E0201461.cub ...
+ matchmap=true
+Notice that we map-projected the images out of order. The reason for
+this is that \texttt{M0100115.cub} is the smaller image. By
+map-projecting the smallest image first, we insure that the least
+amount of black padding will happen to our projected files. That will
+also reduce the amount of processing required for the Ames Stereo
The \texttt{stereo} program (page \pageref{stereo}) is designed for
-automated tie point matching and stereo production, and is the first
-Stereo Pipeline tool we'll use.
+automated stereo production, and is the first Stereo Pipeline tool
+we'll use.
If you like, you should create a directory for the results of the
processing. The \texttt{stereo} program can generate a number of
@@ -162,10 +187,11 @@ \section{Running the Stereo Pipeline}
> ls
- E0201461.cub M0100115.cub
+ E0201461.cub E0201461.cub M0100115.cub
> mkdir results
The \texttt{stereo} program requires a \texttt{stereo.default} file
which can be altered for your needs. Its contents are detailed on
page \pageref{ch:stereodefault}. You may find it useful to save
@@ -181,10 +207,7 @@ \section{Running the Stereo Pipeline}
file distributed with the Stereo Pipeline. The \texttt{stereo.default}
included with the example data set has a smaller correlation window
(smaller values for the \texttt{H\_CORR\_*} and \texttt{V\_CORR\_*}
-variables) that is more suited to the MOC data. You may want to
-use both this \texttt{stereo.default} and the
-\texttt{stereo.default.example} to explore how the results are
+variables) that is more suited to the MOC data.
Alternatively, it is possible to not have to define the
\texttt{H\_CORR\_*} and \texttt{V\_CORR\_*} in
@@ -195,12 +218,33 @@ \section{Running the Stereo Pipeline}
window can be used as a starting point for a better search range if
the results for the first time are unacceptable.
+For this example use the \texttt{stereo.default} that is included with
+the example data set. It has a few key properties:
+ H_CORR_MIN -35
+ H_CORR_MAX -15
+ V_CORR_MIN -280
+ V_CORR_MAX -265
+The first says, \emph{`Don't do interest point alignment!'}. The other
+4 lines define what ranges the left image should search inside the
+right image for a match. The values above are tuned to make up for
+offset that is found in the map projected images. It may come to mind
+that we map projected the images using the same settings, why would
+there be an offset? The reason for this are because Isis doesn't have
+a perfect surface to project on to and that the camera position is
+slightly off.
Here is how the \texttt{stereo} program is called (there should be a
\texttt{stereo.default} file distributed along with the example data
set that will be used):
- ISIS 3> stereo E0201461.cub M0100115.cub results/E0201461-M0100115
+ ISIS 3> stereo results/E0201461-M0100115

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