Dependence R2, also known as Distance Correlation R2 or D-R2, is a statistical measure that extends the traditional R2 concept to non-linear relationships. It was introduced by Gábor J. Székely and Maria L. Rizzo in 2009. Dependence R2 assesses the strength of the relationship between two variables, X and Y, by quantifying the proportion of the variance in Y that can be explained by X, regardless of the relationship being linear or non-linear.
Features bi-directional communication protocols linking directly with Pangolin Beyond and LA Sollinger systems to offer crisp, mathematically accurate laser visualization.
For designers looking to master the platform, official video tutorials cover essential operations: Depence - Syncronorm depence r2
(originally released as Depence² by Syncronorm GmbH ) is a monumental architectural simulation software that bridges the gap between multimedia design and real-time live show control. Built specifically to handle complex live performance environments, it allows operators to pre-visualize lighting, lasers, fountains, video, and special effects simultaneously within a photorealistic 3D rendering engine.
Accurate beam rendering with adjustable haze and cloud parameters. Dependence R2, also known as Distance Correlation R2
: Visualization of stage lighting, lasers, fountains, and video within a single 3D engine.
The answer depends on your scale. For a wedding DJ with 20 moving heads, —use MA3D (free) or Capture (cheaper). For a theme park fountain show, a concert tour with 500 moving lights, or a corporate event demanding photorealistic client approval before the truss is built, Depence R2 is non-negotiable. Rizzo in 2009
Dependence R2 is a valuable statistical measure that extends traditional R2 to non-linear relationships. Its ability to detect non-linear dependencies makes it a useful tool for data analysis, feature selection, and time series analysis. As data becomes increasingly complex, Dependence R2 is likely to play a more prominent role in statistical analysis and modeling.
