aia_stack array 3D | sxr_value listlengths 1 1 | filename stringlengths 23 23 |
|---|---|---|
[[[-1.0,-1.0,-0.9995321035385132,-0.9192525148391724,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1(...TRUNCATED) | [
0.00000989999625744531
] | 2012-01-14T12:59:00.npy |
[[[-0.9461434483528137,-0.9438777565956116,-0.9920135140419006,-1.0,-1.0,-0.9148759841918945,-0.9907(...TRUNCATED) | [
0.000010025967640103772
] | 2012-01-14T13:00:00.npy |
[[[-1.0,-0.9158545732498169,-1.0,-1.0,-1.0,-1.0,-0.9621216654777527,-1.0,-0.9614366292953491,-0.9498(...TRUNCATED) | [
0.000010187264706473798
] | 2012-01-14T13:01:00.npy |
[[[-0.9014667272567749,-1.0,-1.0,-0.9568685293197632,-1.0,-1.0,-0.9735540747642517,-1.0,-1.0,-0.9581(...TRUNCATED) | [
0.000010357898645452224
] | 2012-01-14T13:02:00.npy |
[[[-0.8795495629310608,-1.0,-0.9820436239242554,-1.0,-1.0,-0.9100174307823181,-0.980678379535675,-0.(...TRUNCATED) | [
0.000010585401469143108
] | 2012-01-14T13:03:00.npy |
[[[-0.9678001403808594,-1.0,-1.0,-1.0,-1.0,-1.0,-0.8233076930046082,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-0(...TRUNCATED) | [
0.00001094841991289286
] | 2012-01-14T13:05:00.npy |
[[[-1.0,-1.0,-1.0,-1.0,-1.0,-0.9481445550918579,-0.9930708408355713,-1.0,-1.0,-0.9614616632461548,-1(...TRUNCATED) | [
0.000011176565749337897
] | 2012-01-14T13:06:00.npy |
[[[-0.970757246017456,-1.0,-0.9776056408882141,-1.0,-0.9809921383857727,-0.9160951375961304,-0.99318(...TRUNCATED) | [
0.000011437497960287146
] | 2012-01-14T13:07:00.npy |
[[[-1.0,-1.0,-1.0,-1.0,-0.9027549624443054,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-1.0,-0.95046848058700(...TRUNCATED) | [
0.00001161474301625276
] | 2012-01-14T13:08:00.npy |
[[[-0.8913042545318604,-1.0,-1.0,-0.8675825595855713,-0.9623752236366272,-0.9893751740455627,-1.0,-0(...TRUNCATED) | [
0.000011686980542435776
] | 2012-01-14T13:09:00.npy |
FOXES Dataset: SDO/AIA EUV Images + GOES Soft X-ray Flux
Pre-processed, pre-split multiwavelength EUV image stacks paired with simultaneous GOES soft X-ray (SXR) irradiance measurements. This dataset was created to train and evaluate FOXES (Framework for Operational X-ray Emission Synthesis), a Vision Transformer-based model that predicts solar SXR flux from spatially-resolved EUV imagery.
Code & model: griffingoodwin04/FOXES
Model card: griffingoodwin04/FOXES-model
Dataset Summary
Each sample is a single timestamp pairing:
- AIA image stack — 7-channel EUV image from SDO/AIA, one channel per wavelength band, normalized to
[-1, 1] - SXR flux value — simultaneous GOES B-channel (1–8 Å) soft X-ray irradiance in W/m²
The dataset covers multiple years of solar observations and is split by date into train, validation, and test sets to prevent temporal leakage.
Dataset Structure
Features
| Column | Type | Shape | Description |
|---|---|---|---|
filename |
string |
— | ISO 8601 timestamp used as a unique sample ID (e.g. 2012-03-07T00:12:00) |
aia_stack |
float32 |
(7, 512, 512) |
Multi-wavelength EUV image stack, pixel values in [-1, 1] |
sxr_value |
float32 |
scalar | GOES XRSB flux in W/m² (raw physical units, not log-normalized) |
AIA Wavelength Channels
The 7 channels in aia_stack correspond to SDO/AIA EUV bandpasses in the following order:
| Index | Wavelength (Å) |
|---|---|
| 0 | 94 |
| 1 | 131 |
| 2 | 171 |
| 3 | 193 |
| 4 | 211 |
| 5 | 304 |
| 6 | 335 |
Splits
| Split | Local directory |
|---|---|
train |
train/ |
validation |
val/ |
test |
test/ |
How to Use
With the FOXES pipeline (recommended)
The FOXES repo provides a downloader that reconstructs the expected local directory layout:
git clone https://github.com/griffin-goodwin/FOXES.git
cd FOXES
pip install -r requirements.txt
python download/hugging_face_data_download.py \
--config download/hf_download_config.yaml
Configure output paths in download/hf_download_config.yaml:
repo_id: "griffingoodwin04/FOXES-Data"
aia_dir: "/your/data/AIA_processed"
sxr_dir: "/your/data/SXR_processed"
splits:
- train
- validation
- test
This produces:
/your/data/
├── AIA_processed/
│ ├── train/ ← .npy files, shape (7, 512, 512) float32
│ ├── val/
│ └── test/
└── SXR_processed/
├── train/ ← .npy files, scalar float32
├── val/
└── test/
With the HuggingFace datasets library
from datasets import load_dataset
import numpy as np
ds = load_dataset("griffingoodwin04/FOXES-Data", split="train", streaming=True)
for sample in ds:
aia = np.array(sample["aia_stack"], dtype=np.float32) # (7, 512, 512)
sxr = float(sample["sxr_value"]) # W/m²
t = sample["filename"] # ISO timestamp string
break
Downloading a subset
from datasets import load_dataset
# Stream and take only 1000 samples from validation
ds = load_dataset("griffingoodwin04/FOXES-Data", split="validation", streaming=True)
ds = ds.shuffle(seed=42, buffer_size=3000).take(1000)
Acknowledgements
This work is a research product of Heliolab (heliolab.ai), an initiative of the Frontier Development Lab (FDL.ai). FDL is a public–private partnership between NASA, Trillium Technologies, and commercial AI partners including Google Cloud and NVIDIA.
This material is based upon work supported by NASA under award number No. 80GSFC23CA040.
Team: Griffin Goodwin, Alison March, Jayant Biradar, Christopher Schirninger, Robert Jarolim, Angelos Vourlidas, Viacheslav Sadykov, Lorien Pratt
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