Junchao Huang1,2 Guian Fang3
Shengju Qian4 Xianghao Kong5
Zhuoran Zhao5,6
Wei Huang7 Yihua Du6
Zixin Zhang6 Justin Cui8
Yuchao Gu7 Yukang Chen7 Xinting Hu
Tianyu He9 Shaoshuai Shi
Zhuotao Tian2 Xin Wang
Mike Zheng Shou3 Li Jiang1,2
1CUHK-SZ 2SLAI 3NUS
4CUHK 5HKUST 6HKUST-GZ
7NVIDIA 8UCLA 9MSRA
We present SolarWM, a fully open foundation for building interactive video world models from data preparation through scalable training and long-horizon inference.
- Open, reconfigurable data infrastructure. SolarWM converts 1.43 million canonical clips from 14 datasets into a unified, frame-aligned contract for observations, metric camera geometry, captions, quality metadata, selection, and provenance. Source processing is decoupled from training-mixture design.
- A scalable, backbone-native model family. One framework supports four 5B–33B models across Wan2.2, LTX-2.5, and MiniMax-H3 while preserving each backbone's native representation and objective.
- A simple three-stage training recipe. Bidirectional adaptation, teacher-forced autoregressive initialization, and distribution matching distillation form a shared route across heterogeneous video backbones, without specialized ODE or consistency-distillation initialization.
- Long-horizon interaction from short training clips. After training only on 5-second sequences, the resulting causal models support real-time interaction with rollouts spanning minutes to hours, without long-sequence fine-tuning or attention-sink mechanisms.
- September 3, 2026 — We open-source the training and inference code, the complete dataset, the data pipeline, model weights for all SolarWM-5B training stages, and bidirectional weights for SolarWM-14B, SolarWM-LTX, and SolarWM-H3.
The staged workflow is Stage0.5 FM → Stage1 TF-AnyFlow → Stage2 DMD via SGF, turning a bidirectional video model into a camera-controlled few-step autoregressive model.
- Stage0.5 learns full-clip bidirectional flow matching and establishes the base video, text, and camera-conditioned representation.
- Stage1 combines teacher forcing with the AnyFlow loss in one training stage. Clean history conditions noisy target chunks while the model learns both denoising and finite-step flow maps. This removes the need for a separate ODE or consistency-distillation initialization before Stage2/DMD.
- Stage2 performs DMD via self-gradient forcing (SGF), training the causal student on its own autoregressive rollout with a frozen teacher and a trainable critic.
| Backend | Stage0.5 (Bid-Cam) | Stage1 (TF-AnyFlow) | Stage2 (SGF) | Runtime interfaces |
|---|---|---|---|---|
| Wan2.2-5B | ✓ | ✓ | ✓ | train, infer, preencode |
| Wan2.2-14B | ✓ | Coming soon | Coming soon | train, infer, preencode |
| LTX-2.5 | ✓ | Coming soon | Coming soon | train, infer, preencode |
| MiniMax-H3 | ✓ | Coming soon | Coming soon | train, infer, preencode |
Wan, LTX, and MiniMax-H3 require separate runtime environments. Activate the environment for the selected backbone, then install the shared SolarWM source:
python -m pip install -e .
solarwm environment probeModel weights are available from the
SolarWM model collection. See the
Wan2.2 TI2V-5B guide for Stage0.5, Stage1,
and Stage2 commands. Data access options are described below.
The public
SolarWM-Data release
contains release controls, licenses, recipe and test indexes, small format
examples, and the SolarWM-Data-Annotation/ package. It does not include
the full releases-v1/raw-wds/ or releases-v1/latent-wds/ payloads.
For a released recipe that uses preencoded data, download its matching latent generation. That is sufficient for training and does not require raw-WDS. Raw-WDS is needed only when you want the full processed video corpus, online encoding, your own latent generation, or another workflow whose index points to raw data.
- Use preencoded latents. Each latent generation is published in a separate repository. See the latent-WDS release list for available downloads and generations that are still being uploaded.
- Rebuild raw-WDS from annotations.
SolarWM-Data-Annotation/is an annotation-only release with no videos. It contains the released camera trajectories, captions, metadata, source identities, and reconstruction tools. Follow its README to download the original videos from their source publishers and process them into the expectedraw-wds/layout. - Request prepared raw-WDS. Submit the Dataset Access Form. Approved applicants receive download instructions by email.
See the dataset access guide for download commands and the payload required by each training, validation, and inference example.
# Validate and render the exact resolved configuration.
solarwm config resolve \
--config configs/examples/wan22_ti2v_5b/train_stage0p5_fm_153f.yaml \
--set model.base_path=/path/to/SolarWM-models/SolarWM-5B-base \
--set checkpoint.path=/path/to/SolarWM-models/SolarWM-5B-bid-stage0p5-81f/model.pt \
--set data.index_root=/path/to/SolarWM-Data/releases-v1 \
--set data.transport.root=/path/to/SolarWM-Data/releases-v1 \
--set runtime.validate_every=0 \
--set runtime.output_dir=/path/to/output
# Train the released preencoded recipe without raw-WDS.
torchrun --standalone --nproc-per-node=8 \
-m solarwm train \
--config configs/examples/wan22_ti2v_5b/train_stage0p5_fm_153f.yaml \
--set distributed.world_size=8 \
--set train.global_batch_size=8 \
--set model.base_path=/path/to/SolarWM-models/SolarWM-5B-base \
--set checkpoint.path=/path/to/SolarWM-models/SolarWM-5B-bid-stage0p5-81f/model.pt \
--set data.index_root=/path/to/SolarWM-Data/releases-v1 \
--set data.transport.root=/path/to/SolarWM-Data/releases-v1 \
--set runtime.validate_every=0 \
--set runtime.output_dir=/path/to/output
# Run Wan2.2-5B Stage2 inference for the longest camera-backed horizon.
torchrun --standalone --nproc-per-node=1 -m solarwm infer \
--config configs/examples/wan22_ti2v_5b/infer_stage2_sgf_camera_length.yaml \
--set model.base_path=/path/to/SolarWM-models/SolarWM-5B-base \
--set checkpoint.path=/path/to/SolarWM-models/SolarWM-5B-sgf-stage2-81f \
--set data.index_root=/path/to/SolarWM-Data/releases-v1 \
--set data.transport.root=/path/to/SolarWM-Data/releases-v1 \
--set inference.run_id=my-camera-run \
--set runtime.output_dir=/path/to/output
# Preencode raw-WDS for the Wan2.2-5B 153f recipe.
torchrun --standalone --nproc-per-node=8 \
-m solarwm preencode \
--config configs/examples/wan22_ti2v_5b/preencode_153f.yaml \
--set model.base_path=/path/to/SolarWM-models/SolarWM-5B-base \
--set data.index_root=/path/to/wan153f-fixed-window-index \
--set data.transport.root=/path/to/SolarWM-Data/releases-v1 \
--set preencode.output_root=/path/to/latent-wds/wan22-ti2v5b-153f-480p-v1 \
--set preencode.logical_output_root=/path/to/recipes/wan22-ti2v5b-153f-480p-v1 \
--set runtime.output_dir=/path/to/outputThe quickstart walks through a complete Wan2.2-5B setup. Copyable commands for every released route are in the backend guides.
Every launch writes resolved-config.json and launch-manifest.json before
model allocation. Config overrides are explicit and included in the resolved
configuration identity.
Index rows always contain POSIX shard keys relative to the release directory:
{"sample_id":"...","shard":"raw-wds/abot/shards/kept-high-000001.tar"}Only the runtime root changes:
# Locally mounted storage
data:
index_root: /path/to/SolarWM-Data/releases-v1
transport:
kind: local
root: /path/to/SolarWM-Data/releases-v1
# Object-store streaming uses the same release-relative rows. Supply the
# release root from the distribution channel or deployment environment.
data:
index_root: /path/to/SolarWM-Data/releases-v1
transport:
kind: gcs
root: ${SOLAR_RELEASE_ROOT}
cache_dir: /path/to/solar-cache
cache_max_gib: 256- Quickstart
- Runtime environments
- Architecture
- Data contract
- Dataset overview and statistics
- Download and access
- Wan 2.2 TI2V-5B backend
- Wan 2.2 I2V-A14B backend
- LTX-2.5 backend
- MiniMax-H3 backend
We gratefully thank the teams behind Wan2.2, LTX-2.5, and MiniMax-H3 for releasing the code and pretrained models that make the SolarWM backbone family possible. We also thank the authors of all datasets and open-source projects listed in NOTICE.
If you use SolarWM-Data, the data engine, or the released models in your research, please cite our paper.
Paper: https://arxiv.org/abs/2609.02886
@misc{huang2026solarwmopendatascalable,
title={SolarWM: Open Data and Scalable Training for Long-Horizon Video World Models},
author={Junchao Huang and Guian Fang and Shengju Qian and Xianghao Kong and Zhuoran Zhao and Wei Huang and Yihua Du and Zixin Zhang and Justin Cui and Yuchao Gu and Yukang Chen and Xinting Hu and Tianyu He and Shaoshuai Shi and Zhuotao Tian and Xin Wang and Mike Zheng Shou and Li Jiang},
year={2026},
eprint={2609.02886},
archivePrefix={arXiv},
primaryClass={cs.CV},
url={https://arxiv.org/abs/2609.02886},
}SolarWM is licensed under Apache-2.0. See LICENSE and NOTICE. Model weights and backbone packages may carry their own licenses; review the license and model card in the corresponding release package before use or redistribution. In particular, LTX-2.5 derivatives are subject to the LTX-2.x Community License, and the MiniMax H3 Community License contains territory restrictions. Those packages are not relicensed under the SolarWM code license.