|
| 1 | +## Inference Quickstart |
| 2 | + |
| 3 | +This quickstart shows how to (1) initialize the OlmoEarth model, (2) obtain a satellite |
| 4 | +image suitable for input to the model, and (3) compute embeddings from that satellite |
| 5 | +image. |
| 6 | + |
| 7 | +## Initializing the Model |
| 8 | + |
| 9 | +First, setup a Python 3.12 environment. You can use your favorite Python package |
| 10 | +manager, but here is an example with uv: |
| 11 | + |
| 12 | +``` |
| 13 | +curl -LsSf https://astral.sh/uv/install.sh | sh |
| 14 | +cd /path/to/olmoearth_pretrain/ |
| 15 | +uv sync |
| 16 | +``` |
| 17 | + |
| 18 | +Now we can use the `olmoearth_pretrain` library to initialize the model in pytorch. |
| 19 | +Below, we initialize the OlmoEarth-v1-Base model. |
| 20 | + |
| 21 | +```python |
| 22 | +# TBD, I'm assuming we will have model IDs or something like that to easily initialize |
| 23 | +# the model. |
| 24 | +import json |
| 25 | +from pathlib import Path |
| 26 | + |
| 27 | +import torch |
| 28 | + |
| 29 | +from olmo_core.config import Config |
| 30 | +from olmo_core.distributed.checkpoint import load_model_and_optim_state |
| 31 | + |
| 32 | +checkpoint_path = Path("/weka/dfive-default/helios/checkpoints/joer/phase2.0_base_lr0.0001_wd0.02/step667200") |
| 33 | +with (checkpoint_path / "config.json").open() as f: |
| 34 | + config_dict = json.load(f) |
| 35 | + model_config = Config.from_dict(config_dict["model"]) |
| 36 | + |
| 37 | +model = model_config.build() |
| 38 | + |
| 39 | +train_module_dir = checkpoint_path / "model_and_optim" |
| 40 | +load_model_and_optim_state(str(train_module_dir), model) |
| 41 | + |
| 42 | +device = torch.device("cuda") |
| 43 | +model.to(device) |
| 44 | +``` |
| 45 | + |
| 46 | +## Obtain Satellite Imagery |
| 47 | + |
| 48 | +Here, we obtain one Sentinel-2 image from the ESA Copernicus Browser. If you want to |
| 49 | +apply the model on multiple images of a location, like a time series of Sentinel-1 and |
| 50 | +Sentinel-2 images, see the |
| 51 | +[OlmoEarth embedding](https://github.com/allenai/rslearn/blob/master/docs/examples/OlmoEarthEmbeddings.md). |
| 52 | +and [OlmoEarth fine-tuning](https://github.com/allenai/rslearn/blob/master/docs/examples/FinetuneOlmoEarth.md) |
| 53 | +guides in rslearn. |
| 54 | + |
| 55 | +To download on image from the Copernicus Browser, follow these steps: |
| 56 | + |
| 57 | +1. Navigate to https://browser.dataspace.copernicus.eu/. Press Login to sign up for an |
| 58 | + account and login. |
| 59 | +2. Go to the Search tab at the top-left. Check Sentinel-2, then check L2A. This selects |
| 60 | + Sentinel-2 L2A images, which are the type of Sentinel-2 images that OlmoEarth is |
| 61 | + pre-trained on. |
| 62 | +3. Modify the time range if desired. Also, use the area of interest tool at the top |
| 63 | + right to select a spatial area to search over. |
| 64 | +4. Then, press Search. We recommend looking through the results to find a less cloudy |
| 65 | + image. You can press Visualize to preview the satellite image in the Browser before |
| 66 | + downloading it. Once you are satisfied, press the download icon next to the image in |
| 67 | + the search results. Once the download is complete, unzip the file. |
| 68 | + |
| 69 | +If you prefer to skip using the browser, you can download and unzip a Sentinel-2 image |
| 70 | +of Seattle: |
| 71 | + |
| 72 | +``` |
| 73 | +wget https://storage.googleapis.com/ai2-rslearn-projects-data/artifacts/example_sentinel2_l2a_scene_of_seattle.zip |
| 74 | +unzip example_sentinel2_l2a_scene_of_seattle.zip |
| 75 | +``` |
| 76 | + |
| 77 | +## Compute Embeddings |
| 78 | + |
| 79 | +Finally, we load the image in Python, normalize it, and apply the model on it to |
| 80 | +compute embeddings. |
| 81 | + |
| 82 | +First, we read all of the image bands at 10 m/pixel. We use the B02 band (one of the |
| 83 | +10 m/pixel bands) to determine the transform under which to read the remaining bands, |
| 84 | +since some are stored at lower resolutions. Note that here we assume that the .SAFE |
| 85 | +folder is in the working directory. |
| 86 | + |
| 87 | +```python |
| 88 | +import glob |
| 89 | +import numpy as np |
| 90 | +import rasterio |
| 91 | +from olmoearth_pretrain.data.constants import Modality |
| 92 | +from rasterio.vrt import WarpedVRT |
| 93 | +from rasterio.enums import Resampling |
| 94 | + |
| 95 | +# Get the JP2 filenames that we need to read, in the band order expected by OlmoEarth. |
| 96 | +fnames = [] |
| 97 | +for band_name in Modality.SENTINEL2_L2A.band_order: |
| 98 | + fname = glob.glob(f"*.SAFE/GRANULE/*/IMG_DATA/*/*_{band_name}_*.jp2")[0] |
| 99 | + fnames.append(fname) |
| 100 | + |
| 101 | +# Get the CRS and transform from the first band, which is B02. |
| 102 | +with rasterio.open(fnames[0]) as src: |
| 103 | + crs = src.crs |
| 104 | + transform = src.transform |
| 105 | + width = src.width |
| 106 | + height = src.height |
| 107 | + |
| 108 | +# We limit the width/height to 512x512 in case there is limited memory. |
| 109 | +width = 512 |
| 110 | +height = 512 |
| 111 | + |
| 112 | +# Now read all of the bands. |
| 113 | +image = np.zeros((len(fnames), height, width), dtype=np.int32) |
| 114 | +for band_idx, fname in enumerate(fnames): |
| 115 | + with rasterio.open(fname) as src: |
| 116 | + with rasterio.vrt.WarpedVRT( |
| 117 | + src, |
| 118 | + crs=crs, |
| 119 | + transform=transform, |
| 120 | + width=width, |
| 121 | + height=height, |
| 122 | + resampling=Resampling.bilinear, |
| 123 | + ) as vrt: |
| 124 | + image[band_idx, :, :] = vrt.read(1) |
| 125 | + |
| 126 | +# Rearrange to BHWTC. |
| 127 | +image = image.transpose(1, 2, 0)[None, :, :, None, :] |
| 128 | +``` |
| 129 | + |
| 130 | +Next, we normalize the image: |
| 131 | + |
| 132 | +```python |
| 133 | +from olmoearth_pretrain.data.normalize import Normalizer, Strategy |
| 134 | + |
| 135 | +normalizer = Normalizer(Strategy.COMPUTED) |
| 136 | +image = normalizer.normalize(Modality.SENTINEL2_L2A, image) |
| 137 | +``` |
| 138 | + |
| 139 | +Now we can apply the model on the image. We recommend applying it on inputs between |
| 140 | +1x1 and 128x128 in size. The patch size can be set between 1 and 8; smaller patch sizes |
| 141 | +generally perform better, but require more GPU time. |
| 142 | + |
| 143 | +```python |
| 144 | +from olmoearth_pretrain.train.masking import MaskedOlmoEarthSample, MaskValue |
| 145 | + |
| 146 | +# Run the model on the topleft 64x64 of the image. |
| 147 | +sample = MaskedOlmoEarthSample( |
| 148 | + sentinel2_l2a=torch.tensor(image[:, 0:64, 0:64, :, :], dtype=torch.float32, device=device), |
| 149 | + # The mask shape is BHWTS, where S is the number of band sets (3 for Sentinel-2). |
| 150 | + sentinel2_l2a_mask=torch.ones((1, 64, 64, 1, 3), dtype=torch.float32, device=device) * MaskValue.ONLINE_ENCODER.value, |
| 151 | + # The timestamps is (day of month 1-31, month 0-11, year). |
| 152 | + # The values here correspond to the date of our sample Sentinel-2 image of Seattle |
| 153 | + # (2025-08-22). |
| 154 | + timestamps=torch.tensor([22, 7, 2025], device=device)[None, None, :], |
| 155 | +) |
| 156 | +tokens_and_masks = model.encoder( |
| 157 | + sample, fast_pass=True, patch_size=4, |
| 158 | +)["tokens_and_masks"] |
| 159 | +# Get the Sentinel-2 features. |
| 160 | +modality_features = tokens_and_masks.sentinel2_l2a |
| 161 | +# Pool the features over the timestep and band set dimensions so we end up with a BHWC |
| 162 | +# feature map. |
| 163 | +pooled = modality_features.mean(dim=[3, 4]) |
| 164 | +``` |
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