坐标奇异点导致视线与头部姿态预测的可靠性保障失效
Coordinate Singularities Break Conformal Coverage for Gaze and Head Pose

- 用球面或三维旋转空间的几何原生方式评分,避免坐标系畸变
- 在高仰角或接近万向节锁死区域,90%覆盖率下降至42%以下
- 无需重训练,仅改评分方式即可恢复可靠性,适合视觉系统部署
置信预测为视觉系统提供无需分布假设的可靠性保证,但其有效性依赖于输出空间误差度量方式。许多视觉任务输出位于曲面空间(如球面上的注视方向或三维头部旋转),但中间预测头、残差、不确定性估计或置信分数常以平面坐标图(如偏航-俯仰角或欧拉角)定义。我们发现,这种评分方式在坐标奇点附近(球面大俯角或三维旋转接近万向节锁死)引入系统性几何畸变。在四个数据集(ETH-XGaze、Gaze360、BIWI、AFLW2000-3D)上,名义90%的目标分片条件覆盖率在这些区域下降30-50个百分点,例如在ETH-XGaze上注视俯角超过70度时降至38.9%,在Gaze360上为42.0%;在BIWI和AFLW2000-3D上头部姿态俯角超60度接近万向节锁死时分别降至57.5%和55.2%,尽管边缘覆盖率仍近90%。我们证明这是结构性问题:标量阈值仅改变坐标图中预测集大小,不改变其畸变的轴比。通过引入黎曼体积密度这一几何量,可有效诊断覆盖失效位置。最终,采用无坐标的测地线评分可消除畸变,无需重训练且计算开销可忽略。
原文摘要 · Abstract (English)
Conformal prediction provides distribution-free reliability guarantees for vision systems, but these guarantees depend on how prediction errors are measured in the output space. Many vision tasks produce outputs on curved spaces (e.g. gaze directions on the sphere or 3D head rotations), yet intermediate prediction heads, residuals, uncertainty estimates, or conformal scores are often defined in flat coordinate charts such as yaw-pitch or Euler angles. We show that this scoring choice introduces systematic geometric distortion near coordinate singularities (large pitch angles on the sphere and poses approaching gimbal lock in 3D rotations). Across four datasets (ETH-XGaze, Gaze360, BIWI, AFLW2000-3D), slice-conditional coverage at a nominal 90% target drops by 30-50 percentage points in these regions, falling to 38.9% on ETH-XGaze and 42.0% on Gaze360 at gaze pitch above 70 degrees, and to 57.5% on BIWI and 55.2% on AFLW2000-3D at head pose pitch above 60 degrees near gimbal lock, despite marginal coverage remaining near 90%. We prove that this is structural. Scalar thresholding changes the size of chart-coordinate prediction sets but leaves their distorted axis ratios unchanged. To diagnose this hidden failure mode, we show that a simple geometric quantity, the Riemannian volume density, strongly correlates with where coverage collapse occurs. Finally, we show that coordinate-free geodesic scoring removes this distortion. It requires no retraining and adds negligible computational cost.
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