Changes between Version 51 and Version 52 of Procedures/RCDPhotoProcessing


Ignore:
Timestamp:
Feb 24, 2011, 2:31:07 PM (13 years ago)
Author:
emca
Comment:

--

Legend:

Unmodified
Added
Removed
Modified
  • Procedures/RCDPhotoProcessing

    v51 v52  
    1212
    1313The next stages of the processing incorporate:
    14  * updating the photograph event file with the post-processed positional data and the exterior camera angles.
     14 * creating a kml file, viewing in goggle earth and removing any images that are not relevant to the study area
     15 * updating the photograph event file with the post-processed positional data and the exterior camera angles
    1516 * tagging the images with positional and navigational data as well as project information
    1617 * renaming the images to conform to ARSF standards
     
    2122To improve the chances of this single script approach working, follow the stages below to set up the data and remove as many anomalies as possible.
    2223
    23  1. Check the rcd/logs file for an ***!ImageEvents1.csv and ***!PhotoId1.csv file. There may be some empty files with this name so be sure to choose the correct one. If there are more then one then you need to specify which one to use.
    24  1. Open IPAS CO (on the windows machine). This is used to create a new image event file with post-processed positional data and omega,phi,kappa values.
    25   * Load in the *.sol file, the *!ImageEvents1.csv and *!PhotoId1.csv file
    26   * Camera Orientation Direction: -90
    27   * Event Offset: 0.006
    28   * Lever Arm values: x 0.112 y 0.061 z -0.60
    29   * Output file as *!ImageEvents1-processed.csv, file format ASCII Output
    30  1. Create a KML file and view it in Google Earth.
     24 
     25 1. Create a KML file and view it in Google Earth. Check the rcd/logs file for an ***!ImageEvents1.csv. There may be some empty files with this name so be sure to choose the correct one. If there are more then one then you need to specify which one to use.
    3126  * Run `kmlise_project.py -d <main_project_dir> -e ***ImageEvents1.csv > kml_file.kml` - this creates a kml file using the !ImageEvents1-processed.csv file
    3227  * Open the kml file in google earth
     
    3429  * Delete these tif files (not the raws) since they are not required.
    3530  * Delete the kml file created above as it is no longer needed. An updated one will be created by the delivery script.
     31 1. Open IPAS CO (on the windows machine). This is used to create a new image event file with post-processed positional data and omega,phi,kappa values.
     32  * Load in the *.sol file and from rcd/logs the *!ImageEvents1.csv and *!PhotoId1.csv file
     33  * Camera Orientation Direction: -90
     34  * Event Offset: 0.006
     35  * Lever Arm values: x 0.112 y 0.061 z -0.60
     36  * Output file as *!ImageEvents1-processed.csv, file format ASCII Output
    3637 1. Check the event log file for erroneous entries
    3738  * If there is no log file then this approach can not be used. See below section on tagging without log files.
     
    4243
    4344{{{
    44 make_delivery_folder.sh -c -d ~airborne/workspace/project_dir -y 2010 -j 297 -p EX01_01 -a "Example Site" -e ~airborne/workspace/project_dir/leica/rcd/logs/ImageEvent1-processed.csv -s ~airborne/workspace/project_dir/leica/ipas/proc/solfile.sol -n "PI Name" | tee camera_delivery.log
     45make_delivery_folder.sh -c -d ~airborne/workspace/project_dir -y 2010 -j 297 -p EX01_01 -a "Example Site" -e ~airborne/workspace/project_dir/leica/rcd/logs/ImageEvent1-processed.csv -n "PI Name" | tee camera_delivery.log
    4546}}}
    4647