This document outlines the functionality of various approaches within the Thin Slice Classifier project.
Authors: Freja Thoresen, Aidan Cowley, Romeo Haak, Jonas Lewe, Clara Moriceau, Piotr Knapczyk, Victoria Engelschion
- NASA PDS database (https://pdsimage2.wr.usgs.gov/Missions/Apollo/Lunar_Sample_Photographs/)
- Lunar Institute Data (https://www.lpi.usra.edu/lunar/samples/atlas/thin_sections/)
- Virtual Microscope (http://www.virtualmicroscope.org/explore)
Trained models can be downloaded from wandb.
https://wandb.ai/freja-thoresen/SimCLR https://wandb.ai/freja-thoresen/Geological%20Binary%20Classifier
To execute the binary classifier, run the msm_statistics.py
script using the following command:
combined_data2x.msm <image_directory_name>
This command will generate a "datasets" folder containing two sub-folders: "grain" and "rock_type". For example, in the "rock_type" sub-folder, images will be classified into either a "breccia" or a "basalt" folder based on the generated classification dictionary. Additionally, sample IDs will be added as prefixes to the existing file names for easier management. If using the binary classifier, ensure to remove the "other" folder.
This section assumes you have completed the Quick Guide in the Set everything up
section.
This script creates data folds, ensuring that images from the same sample are grouped together in either the training or testing sets. It is utilized by preprocessing_helper.py
.
This file is responsible for cleaning and organizing folders for training, testing, and validation. It ensures that images from the same sample are stored together.
This is the core component of the binary classifier, which is responsible for training and fine-tuning the networks.
You can adjust the network type and parameters by the following:
network = InceptionResNet(training_directory, validation_directory, test_directory,
epochs=20, finetune_epochs=30, batch_size=32)
The available networks include VGG16, VGG19, and InceptionResNet. Additional functionalities include:
-c
: Enables cross-validation training-f
: Enables fine-tuning after initial training-x
: Executes experiment 1 to check for repeated false positives-t
: Runs for only 2 epochs for testing purposes-g
: Draws precision-recall curves (not available for cross-validation)-T
: Evaluates model performance on the test set
To train the network for rock type prediction, use:
python networks.py -f -T ../datasets/rock_type
While not necessary for running the classifier, understanding the following information can be helpful regarding saved and processed files.
Contains links to all high-resolution JPEG and TIF images in the PDS database. This is used in the download_labels
function within sample_downloader.py
.
This file contains the moon sample metadata (msm) for the data from the PDS database. Essentially, this file contains information about the sample, specifying its superclass, subclass, sample ID, etc.
See https://pdsimage2.wr.usgs.gov/Missions/Apollo/Lunar_Sample_Photographs/A14VIS_0001/DATA/BASALT/FELDSPATHIC/14053/THIN_SECTIONS/S71-23315.LBL for an example
This file is a product of running lbl_parser.py. This file is used in processing_combined.py and statistic_combined.py if using the MsmStatisticsPdsimage class.
This file serves a similar purpose to pds_data.msm
but employs a slightly different data structure.
See https://www.lpi.usra.edu/lunar/samples/atlas/thin_section/?mission=Apollo%2011&sample=10058&source_id=JSC04230 for an example of the data saved.
This file is also utilized in processing_combined.py
.
IMPORTANT FILE. This file consolidates data from the lunar sample atlas and NASA's PDS. It also indicates grain size and rock type for the samples.
To create this file:
- Combine
lunar_institute.msm
andpds_data.msm
usingcombine_pds_and_lunar()
inprocessing_combined.py
. - Run the following lines of code with the newly created
combined_data.msm
inprocessing_combined.py
to generatecombined_data2x.msm
:
data_msm = load_file("combined_data.msm")
data_msm = {k: change_paths(v) for k, v in data_msm.items()}
write_to_file(data_msm, 'combined_data2x.msm')
This file is referenced by msm_statistics_combined.py
.
This file is usually the first point of reference for acquiring data. It contains the ImageFinder
class responsible for compiling links from NASA's PDS image database. The full_database_tree
is also available on GitHub for immediate use.
You can use this class as follows:
image_finder = ImageFinder()
image_finder.director(<mode>)
The director method has three modes: 'combine', 'all', and 'missed only'. Depending on your needs, replace <mode>
with one of these valid options. Running in "all" mode assumes you don't have any data yet and will attempt to scrape all links from NASA's PDS database located at:
https://pdsimage2.wr.usgs.gov/Missions/Apollo/Lunar_Sample_Photographs/.
Please note that the site may occasionally close connections to prevent bot behavior. If this occurs while in "full" mode, any links that could not be accessed will be saved to a file named 'leftover_urls'.
If you then run the director in "missed only" mode, it will retry accessing the missed URLs and attempt to scrape those links and their subdirectories. After calling "full" and "missed only" once, you should have all the links you need. Finally, you can run the director in "combine" mode to merge the results from the "database_tree" file produced by the "full" mode and "database_tree_rest" from the "missed only" mode into a single file called "full_database_tree".
Once you've created the "full_database_tree" file, you can use it to download label files and images. It is recommended to download the label files first, as they are essential for preprocessing. To download the labels, use:
all_urls = load_file('full_database_tree')
download_labels(all_urls, os.path.join('Data', 'labels'))
Be aware that the same issue of the remote host closing the connection might occur here as well, so you may need to run this function multiple times. Don't worry; it will inform you when everything has succeeded.
The other functions in this module are mainly used by different files but serve to fetch or download the actual images of a sample. The most critical function among them is process_local_samples
.
This file is responsible for parsing the label files from the PDS database. You can run the script using:
python lbl_parser.py <Directory where label files are stored> <Desired filename>
If everything is successful, you should receive an output file named pds_data.msm
.
This is an important file that assists in cleaning up and combining the two MSM files obtained from the PDS and LPI databases. It standardizes the information saved from both files into one. Call the necessary functions as needed.
This file is tasked with extracting specific statistics and information. Depending on which MSM file you are using, you'll need to select the appropriate class.
For example, if you're using combined_data2x.msm
, the relevant class is MSMCombinedStatistics
. In that case, you can initialize it like so on line 213:
statistic_type = MsmCombinedStatistics(data_msm)