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In 2015, we changed the method used to calculate fitted trends. Primarily, this was done to allow the calculation of realistic uncertainties, but at the same time we also began to use our monthly, rather than our annual data set.
Previously, trends were calculated using a simple linear regression. However, this method is unsuitable for calculating uncertainties in trends, as the observations in the series are not totally independent of each other. In order to attempt to account for this autocovariance, trends are now fitted using an Integrated Generalized Gauss Markov stochastic model (see below for a full description).
The data selection method remains the same as before:
For each period fitted, the time series is decomposed into the following components:
Note that no attempt has been made to assess the appropriateness of the linear regression model for any given fit. Rather, values have been calculated to illustrate global and regional trends. Therefore, individual values should not be treated as a research quality product suitable for publication, or for use in planning or policy making.
Should you wish to further investigate the trend at a particular site, we would invite you to download the RLR data and examine the relevant station documentation.
Sea level varies on time scales from seconds to millions of years as a result of a wide variety of physical processes [Harrison, 2002]. Hughes and Williams  highlighted the importance of spatial variations in the spectral shape of sea level using satellite altimeter data.
Bos et al  also showed the variety in temporal correlations in sea level using PSMSL tide gauge data. They used a range of stochastic models such as white noise, Autoregressive noise (both AR(1) and AR(5)), Autoregressive Fractionally Integrated (ARFI) noise and Generalized Gauss Markov (GGM) Noise. Rather than use multiple stochastic noise models we introduce a new, more general model, which requires three parameters, αL, αR and γ. This model is shown pictorially in the figure below as an idealized power spectrum plotted in log-log space. A Fractionally Integrated Generalized Gauss Markov (FIGGM) model has two regions separated at some frequency, fc, which is related to the AR(1) parameter, γ. To the left of fc, the spectrum has a slope in log-log space equal to αL and a slope of αR to the right of fc. All of the other models can be considered special cases of FIGGM. For instance AR(1) (also called First-Order Gauss Markov (FOGM) noise) simply has one parameter, γ, which describes where the break point is; αL is 0 and αR is -2. Power-law noise which simply has one slope can arise from a number of combinations of the three parameters. We estimate all three parameters together with the amplitude for the noise and the amplitude for a white noise component (spectrum will flatten at high frequencies). Using a FIGGM stochastic model means that the form of the noise in the data can take on that of any of the other models without implicit forcing of the parameters.