- Last observation
- Jan 28, 2022
- Closest stations
5 closest stations in all networks
|Velocity (mm/yr)||Velocity standard deviation (mm/yr)||Last observation||Intercept (mm)||Intercept standard deviation (mm)|
|White noise (mm)||Amplitude of first power law (mm/yr^(n1/4))||n1 (spectral index of first power law)||Lower frequency limit for band-pass (BP) filtered noise (cycle/year)||Upper frequency limit for band-pass (BP) filtered noise (cycle/year)||Number of poles for BP filtered noise||Amplitude of BP filtered noise (mm)||n2 (spectral index of second power law)||Amplitude of second power law (mm/yr^(n2/4))|
These results are preliminary. The station positions are unchecked and should not be used for any engineering applications. There may be errors in the antenna heights. The velocities are very dependent on the length of the span of observations. The presence of outliers (errant observations) sometimes contaminates the velocities.