The time series of annual means provides an intuitive representation of internal variability.
Figure 3 shows the annual ADJ time series in different spatial areas. It is necessary to point out that the annual ERF time series also shows similar year-to-year variation features (not displayed here). In all cases (i.e., global mean, region A, grid B and grid C), the F curves from PD and PI simulations show different year-to-year variations. As a result, their difference (i.e., ADJ) also shows obvious year-to-year variation. Clearly, the amplitude of the time series is related to the spatial area of the research object. The larger the area, the more mutual cancellation occurs between positive and negative variations. As expected, the amplitude of the global mean ADJ time series is much smaller than that of other time series. This is why the simulation length required for estimating a global mean is much shorter than that needed for regional values. The amplitude of the time series for an individual model grid box depends on its location. Consisting with the spatial distribution of
Std shown in
Figure 2, grid B shows a much larger amplitude than grid C.
Internal variability is an intrinsic year-to-year fluctuation in the climate system that occurs during model simulation in the absence of external forcing. In theory, the annual ADJ time series should not exhibit long-term trends under constant forces. However, the time series may show obvious increasing or decreasing trends on decadal scales due to the chaotic feature of internal variability.
Figure 3 shows a variety of 10-year ADJ time series windows with strong increasing or decreasing trends, such as the 33
rd to 42
nd years in region A. There are also some 30-year ADJ time series windows with obvious trends, such as the 15
th to 44
th years in grid B. However, the strength of the trend over a longer period (i.e., 30 years) is hardly the same as the strength of the trend over a 10-year period. The following paragraphs will analyze the probability distributions of 10-year trends and 30-year trends.
Figure 4 shows the probability distributions of ADJ 10-year and 30-year trends. The trend is defined as the linear regressions slope for every 10-year or 30-year period in the time series of 50-year simulation. Each ensemble member can produce 41 10-year trends and 21 30-year trends. Because the year-to-year fluctuations are chaotic, these trends possess an approximately normal distribution, especially the 10-year trends. This is consistent with previous studies about internal variability on decadal time scales (e.g., [
10,
13]). It is also necessary to point out that the 75
th percentile of the trend distribution is not completely opposite to the 25
th percentile because of the limited sample size. The trend distributions of ERF are almost the same as ADJ (not shown). In order to better understand these trends, 10-year and 30-year changes are compared with annual mean ERF. The 25
th and 75
th percentiles of the 10-year trend distributions of global mean are −0.16 W m
−2 decade
−1 and 0.13 W m
−2 decade
−1, respectively. The 10-year changes caused by these two trends equal about a quarter of the magnitude of the global annual mean ERF (−0.57 W m
−2). Based on statistical theory, 30-year trends are usually much weaker than 10-year trends. The 25
th and 75
th percentiles of the 30-year trend distribution of global mean are −0.03 W m
−2 decade
−1 and 0.02 W m
−2 decade
−1, respectively. In other words, there is a 50% probability that 30-year changes are outside the range of −0.09 (−0.03 × 3) to 0.06 (0.02 × 3) W m
−2. In region A, half of the 30-year changes are outside the range of −0.96 (−0.32 × 3) to 1.47 (0.49 × 3) W m
−2. Compared to the magnitude of spatial and temporal averaged ERF in region A (−2.44 W m
−2), these 30-year changes cannot be neglected. On grid B, the annual mean ERF is −1.90 W m
−2, and half of 30-year changes are outside the range of −2.94 (−0.96 × 3) to 2.58 (0.86 × 3) W m
−2. On grid C, the annual mean ERF is −0.08 W m
−2, and half of 30-year changes are outside the range of −1.02 (−0.34 × 3) to 0.39 (0.13 × 3) W m
−2.
Figure 5 shows the 25
th and 75
th percentiles of trend distribution at each model grids. Here, the 75
th percentile of the trend distribution is generally opposite to the 25
th percentile. There is a 50% probability that the 10-year trend is stronger than 4 W m
−2 decade
−1 (≤−4 and ≥4) over high
Std areas (
Std > 5 W m
−2 in
Figure 2). Over most high
Std areas, the 25
th and 75
th percentiles of the 30-year trend are also relatively strong. In about half of the cases, 30-year changes can reach 2 (0.7 × 3 > 2) W m
−2. In short, the influence of internal variability on 10-year and 30-year trends cannot be neglected even on global scales.