| 11 | | 1. Create temporary thumbnail images of the processed tiff files using photo2thumb.py. Open the first image with eog and use either spacebar to scroll though the images or view/slideshow. Remove any images that that are over/under exposed. |
| 12 | | 1. Check there is a *_camera.sol file in the IPAS/proc directory. If there is not, then you will need to create one. See details here: http://arsf-dan.nerc.ac.uk/trac/wiki/Procedures/ProcessingChainInstructions/NavigationProcessing |
| 13 | | 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. |
| 14 | | * 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 **NOTE- this program currently falls over unless the eagle directory is clear of unrecognised files** |
| | 11 | 1. Get a camera .sol file |
| | 12 | * Check there is a *_camera.sol file in the IPAS/proc directory. If there is not, then you will need to create one. See details here: http://arsf-dan.nerc.ac.uk/trac/wiki/Procedures/ProcessingChainInstructions/NavigationProcessing |
| | 13 | 1. Remove "bad" images |
| | 14 | * Create temporary thumbnail images of the processed tiff files using photo2thumb.py. |
| | 15 | * Open the first image with eog and use either spacebar to scroll though the images or view/slideshow. Remove the corresponding tiff images for any that are over/under exposed. |
| | 16 | 1. Remove images that don't correspond to flightlines |
| | 17 | * Create a temporary kml file: `kmlise_project.py -d <main_project_dir> -e ***ImageEvents1.csv > kml_file.kml` Make sure the correct eventfile is being pointed to **NOTE- this program currently falls over unless the eagle directory is clear of unrecognised files** |
| 16 | | * Note which blocks of photographs do not overlap with any Eagle/Hawk data. Usually consists of a group of photographs at the start of the survey where they set up the exposure rates etc for the camera. Often the log sheet notes which images too. |
| 17 | | * Delete these tif files (not the raws) since they are not required. |
| 18 | | * Delete the kml file created above as it is no longer needed. An updated one will be created by the delivery script. |
| 19 | | 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. |
| | 19 | * Note which blocks of photographs do not overlap with any Eagle/Hawk data. Usually consists of a group of photographs at the start of the survey where they set up the exposure rates etc for the camera. Often the log sheet notes which images too. Delete these tif files (not the raws) since they are not required. |
| | 20 | * Delete the kml file created above as it is no longer needed (an updated one will be created by the delivery script) |
| | 21 | 1. create a new image event file with post-processed positional data and omega,phi,kappa values |
| | 22 | * Open IPAS CO (on the windows machine) |