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GREAT Dataset

The GREAT dataset is a novel multi‑sensor (stereo camera, LiDAR, IMU) lunar surface dataset collected from a vehicle‑mounted platform in complex urban environments. It includes high‑precision multi‑frequency GNSS observations, tactical‑grade IMU, MEMS IMU, two CMOS cameras, and LiDAR. All sensors are hardware‑synchronized and well‑calibrated. The dataset comprises eight sequences covering the Wuhan University campus and surrounding urban/suburban areas, intended for evaluating multi‑sensor fusion navigation algorithms.

Source
github
Created
Nov 7, 2024
Updated
Nov 8, 2024
Signals
840 views
Availability
Linked source ready
Overview

Dataset description and usage context

GREAT DATASET

Introduction

Abstract

GREAT Dataset is a new multi‑sensor raw observation dataset collected from a vehicle in complex urban environments, featuring high‑precision multi‑frequency GNSS receivers, tactical‑grade IMU, MEMS IMU, two CMOS cameras, and LiDAR. All sensors are hardware‑synchronized and well‑calibrated. The dataset includes eight sequences covering the Wuhan University campus and nearby urban/suburban areas, supporting evaluation of various multi‑sensor fusion navigation algorithms.

Main Contributions

  • Provides raw GNSS observations, IMU measurements, camera images, and LiDAR scans with timestamps unified to GPS time via hardware sync.
  • Captures diverse environments (campus, urban canyon, suburb) to thoroughly assess SLAM robustness and accuracy.
  • Supplies high‑precision raw GNSS and inertial navigation data for robotics, SLAM, and satellite navigation research.

License

The dataset is released under the MIT License for academic use only. Commercial use or collaborations require contacting xingkonggreat@163.com.

Sensor Setup

Platform

Details and diagrams are provided in the original documentation.

Sensors

SensorModelFrequencyDetails
GNSS ReceiverSeptentrio PolaRx51 HzMulti‑frequency, multi‑system (GPS, GLONASS, GALILEO, BDS, IRNSS, QZSS)
Tactical‑grade IMUStarNeto XW‑GI7660200 HzGyro bias 0.3 (°/h), accel bias 100 mGal, angular random walk 0.01 (°/√h)
MEMS‑IMUADIS‑16470100 HzGyro bias 8 (°/h), accel bias 1500 mGal, angular random walk 0.34 (°/√h), velocity random walk 0.037 (m/s/√h)
CameraFLIR BFS‑PGE‑31S4C20 HzSony IMX265 sensor, global shutter, PoE GigE, max resolution 2048 × 1536
LiDARVelodyne VLP‑1610 HzVertical FOV 30° (+15° ~ ‑15°), vertical angular res 2°, 360° horizontal FOV, max range 100 m

Comparison with Other Datasets

DatasetGNSS RawMulti‑frequencyMEMS IMUTactical IMULiDARCameraHardware Sync
WHU‑Helmet××
SubT‑MRS×××
GEODE××
KITTI×××
Hilti SLAM×××
RobotCar××××
M2DGR×××
Brno Urban××
SmartPNT‑POS×××
OURS

Environment

Eight sequences are provided, including four day‑time campus runs, one night‑time campus run, two urban canyon runs, and two suburban runs. Sample images illustrate each environment.

Data Sequences

SequenceDateBuildingsDense TreesOverpasses/TunnelsDynamic VehiclesDynamic PedestriansGNSS ObservationsDuration (s)Difficulty
campus‑012020/10/27606.85Medium
campus‑022020/10/27806.9Medium
campus‑032020/10/271200.1Hard
campus‑night2020/10/29545.7Hard
suburb‑012020/10/291081.35Easy
suburb‑022020/10/29837Easy
urban‑012020/10/27767.3Medium
urban‑022022/10/231622.2Hard

Download

SequenceIMUImagesLiDARReference Solution
campus‑01IMU.zipImage.zipLiDAR.zipReference
campus‑02............
...............

Reference Solutions

Reference trajectories for each sequence have been plotted in Google Earth. Figures 7‑14 in the original document illustrate these trajectories.

Directory Structure

Raw GNSS observations and ephemerides are stored in the GNSS_RAW_DATA folder. Each sequence folder contains IMU data, stereo images, LiDAR scans, and reference solutions.

Development Toolkit

A script is provided to convert raw visual‑LiDAR observations to ROS bag files. The tool requires a ROS environment and necessary dependencies.

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