From: Ben Santer
To: Tom Wigley , Karl Taylor , Thomas R Karl , John Lanzante , carl mears , "David C. Bader" , "'Dian J. Seidel'" , "'Francis W. Zwiers'" , Frank Wentz , Leopold Haimberger , Melissa Free , "Michael C. MacCracken" , "'Philip D. Jones'" , Steven Sherwood , Steve Klein , 'Susan Solomon' , "Thorne, Peter" , Tim Osborn , Gavin Schmidt , "Hack, James J."
Subject: Update on response to Douglass et al.
Date: Wed, 09 Jan 2008 19:52:15 -0800
Reply-to: santer1@llnl.gov
Dear folks,
I just wanted to update you on my progress in formulating a response to
the Douglass et al. paper in the International Journal of Climatology
(IJC). There have been several developments.
First, I contacted Science to gauge their level of interest in
publishing a response to Douglass et al. I thought it was worthwhile to
"test the water" before devoting a lot of time to the preparation of a
manuscript for submission to Science. I spoke with Jesse Smith, who
handles most of the climate-related papers at Science magazine.
The bottom line is that, while Science is interested in this issue
(particularly since Douglass et al. are casting doubt on the findings of
the 2005 Santer et al. Science paper), Jesse Smith thought it was highly
unlikely that Science would carry a rebuttal of work published in a
different journal (IJC). Regretfully, I agree. Our response to Douglass
et al. does not contain any fundamentally new science - although it does
contain some new and interesting work (see below).
It's an unfortunate situation. Singer is promoting the Douglass et al.
paper as a startling "new scientific evidence", which undercuts the key
conclusions of the IPCC and CCSP Reports. Christy is using the Douglass
et al. paper to argue that his UAH group is uniquely positioned to
perform "hard-nosed" and objective evaluation of model performance, and
that it's dangerous to leave model evaluation in the hands of biased
modelers. Much as I would like to see a high-profile rebuttal of
Douglass et al. in a journal like Science or Nature, it's unlikely that
either journal will publish such a rebuttal.
So what are our options? Personally, I'd vote for GRL. I think that it
is important to publish an expeditious response to the statistical flaws
in Douglass et al. In theory, GRL should be able to give us the desired
fast turnaround time. Would GRL accept our contribution, given that the
Douglass et al. paper was published in IJC? I think they would - we've
done a substantial amount of new work (see below), and can argue, with
some justification, that our contribution is more than just a rebuttal
of Douglass et al.
Why not go for publication of a response in IJC? According to Phil, this
option would probably take too long. I'd be interested to hear any other
thoughts you might have on publication options.
Now to the science (with a lower-case "s"). I'm appending three
candidate Figures for a GRL paper. The first Figure was motivated by
discussions I've had with Karl Taylor and Tom Wigley. It's an attempt to
convey the differences between our method of comparing observed and
simulated trends (panel A) and the approach used by Douglass et al.
(panel B).
In our method, we account for both statistical uncertainties in fitting
least-squares linear trends to noisy, temporally-autocorrelated data and
for the effects of internally-generated variability. As I've described
in previous emails, we compare each of the 49 simulated T2 and T2LT
trends (i.e., the same multi-model ensemble used in our 2005 Science
paper and in the 2006 CCSP Report) with observed T2 and T2LT trends
obtained from the RSS and UAH groups. Our 2-sigma confidence intervals
on the model and observed trends are estimated as in Santer et al.
(2000). [Santer, B.D., T.M.L. Wigley, J.S. Boyle, D.J. Gaffen, J.J.
Hnilo, D. Nychka, D.E. Parker, and K.E. Taylor, 2000: Statistical
significance of trends and trend differences in layer-average
atmospheric temperature time series, J. Geophys. Res., 105, 7337-7356]
The method that Santer et al. (2000) used to compute "adjusted" trend
confidence intervals accounts for the fact that, after fitting a trend
to T2 or T2LT data, the regression residuals are typically highly
autocorrelated. If this autocorrelation is not accounted for, one could
easily reach incorrect decisions on whether the trend in an individual
time series is significantly different from zero, or whether two time
series have significantly different trends. Santer et al. (2000)
accounted for temporal autocorrelation effects by estimating r{1}, the
lag-1 autocorrelation of the regression residuals, using r{1} to
calculate an effective sample size n{e}, and then using n{e} to
determine an adjusted standard error of the least-squares linear trend.
Panel A of Figure 1 shows the 2-sigma "adjusted" standard errors for
each individual trend. Models with excessively large tropical
variability (like FGOALS-g1.0 and GFDL-CM2.1) have large adjusted
standard errors. Models with coarse-resolution OGCMs and low-amplitude
ENSO variability (like the GISS-AOM) have smaller than observed adjusted
standard errors. Neglect of volcanic forcing (i.e., absence of El
Chichon and Pinatubo-induced temperature variability) can also
contribute to smaller than observed standard errors, as in
CCCma-CGCM3.1(T47).
The dark and light grey bars in Panel A show (respectively) the 1- and
2-sigma standard errors for the RSS T2LT trend. As is visually obvious,
36 of the 49 model trends are within 1 standard error of the RSS trend,
and 47 of the 49 model trends are within 2 standard errors of the RSS
trend.
I've already explained our "paired trend test" procedure for calculating
the statistical significance of the model-versus-observed trend
differences. This involves the normalized trend difference d1:
d1 = (b{O} - b{M}) / sqrt[ (s{bO})**2 + (s{bM})**2 ]
where b{O} and b{M} represent any single pair of Observed and Modeled
trends, with adjusted standard errors s{bO} and s{bM}.
Under the assumption that d1 is normally distributed, values of d1 >
+1.96 or < -1.96 indicate observed-minus-model trend differences that
are significant at some stipulated significance level, and one can
easily calculate a p-value for each value of d1. These p-values for the
98 pairs of trend tests (49 involving UAH data and 49 involving RSS
data) are what we use for determining the total number of "hits", or
rejections of the null hypothesis of no significant difference between
modeled and observed trends. I note that each test is two-tailed, since
we have no information a priori about the "direction" of the model trend
(i.e., whether we expect the simulated trend to be significantly larger
or smaller than observed).
REJECTION RATES FOR "PAIRED TREND TESTS, OBS-vs-MODEL
Stipulated sign. level No. of tests T2 "Hits" T2LT "Hits"
5% 49 x 2 (98) 2 (2.04%) 1 (1.02%)
10% 49 x 2 (98) 4 (4.08%) 2 (2.04%)
15% 49 x 2 (98) 7 (7.14%) 5 (5.10%)
Now consider Panel B of Figure 1. It helps to clarify the differences
between the Douglass et al. comparison of model and observed trends and
our own comparison. The black horizontal line ("Multi-model mean trend")
is the T2LT trend in the 19-model ensemble, calculated from model
ensemble mean trends (the colored symbols). Douglass et al.'s
"consistency criterion", sigma{SE}, is given by:
sigma{SE} = sigma / sqrt(N - 1)
where sigma is the standard deviation of the 19 ensemble-mean trends,
and N is 19. The orange and yellow envelopes denote the 1- and
2-sigma{SE} regions.
Douglass et al. use sigma{SE} to decide whether the multi-model mean
trend is consistent with either of the observed trends. They conclude
that the RSS and UAH trends lie outside of the yellow envelope (the
2-sigma{SE} region), and interpret this as evidence of a fundamental
inconsistency between modeled and observed trends. As noted previously,
Douglass et al. obtain this result because they fail to account for
statistical uncertainty in the estimation of the RSS and UAH trends.
They ignore the statistical error bars on the RSS and UAH trends (which
are shown in Panel A). As is clear from Panel A, the statistical error
bars on the RSS and UAH trends overlap with the Douglass et al.
2-sigma{SE} region. Had Douglass et al. accounted for statistical
uncertainty in estimation of the observed trends, they would have been
unable to conclude that all "UAH and RSS satellite trends are
inconsistent with model trends".
The second Figure plots values of our test statistic (d1) for the
"paired trend test". The grey histogram is based on the values of d1 for
the 49 tests involving the RSS T2LT trend and the simulated T2LT trends
from 20c3m runs. The green histogram is for the 49 paired trend tests
involving model 20c3m data and the UAH T2LT trend. Note that the d1
distribution obtained with the UAH data is negatively skewed. This is
because the numerator of the d1 test statistic is b{O} - b{M}, and the
UAH tropical T2LT trend over 1979-1999 is smaller than most of the model
trends (see Figure 1, panel A).
The colored dots are values of the d1 test statistic for what I referred
to previously as "TYPE2" tests. These tests are limited to the M models
with multiple realizations of the 20c3m experiment. Here, M = 11. For
each of these M models, I performed paired trend tests for all C unique
combinations of trends pairs. For example, for a model with 5
realizations of the 20c3m experiment, like GISS-EH, C = 10. The
significance of trend differences is solely a function of "within-model"
effects (i.e., is related to the different manifestations of natural
internal variability superimposed on the underlying forced response).
There are a total of 62 paired trend tests. Note that the separation of
the colored symbols on the y-axis is for visual display purposes only,
and facilitates the identification of results for individual models.
The clear message from Figure 2 is that the values of d1 arising from
internal variability alone are typically as large as the d1 values
obtained by testing model trends against observational data. The two
negative "outlier" values of d1 for the model-versus-observed trend
tests involve the large positive trend in CCCma-CGCM3.1(T47). If you
have keen eagle eyes, you'll note that the distribution of colored
symbols is slightly skewed to the negative side. If you look at Panel A
of Figure 1, you'll see that this skewness arises from the relatively
small ensemble sizes. Consider results for the 5-member ensemble of
20c3m trends from the MRI-CGCM2.3.2. The trend in realization 1 is close
to zero; trends in realizations 2, 3, 4, and 5 are large, positive, and
vary between 0.27 to 0.37 degrees C/decade. So d1 is markedly negative
for tests involving realization 1 versus realizations 2, 3, 4, and 5. If
we showed non-unique combinations of trend pairs (e.g., realization 2
versus realization 1, as well as 1 versus 2), the distribution of
colored symbols would be symmetric. But I was concerned that we might be
accused of "double counting" if we did this....
The third Figure is the most interesting one. You have not seen this
yet. I decided to examine how the Douglass et al. "consistency test"
behaves with synthetic data. I did this as a function of sample size N,
for N values ranging from 19 (the number of models we used in the CCSP
report) to 100. Consider the N = 19 case first. I generated 19 synthetic
time series using an AR-1 model of the form:
xt(i) = a1 * (xt(i-1) - am) + zt(i) + am
where a1 is the coefficient of the AR-1 model, zt(i) is a
randomly-generated noise term, and am is a mean (set to zero here).
Here, I set a1 to 0.86, close to the lag-1 autocorrelation of the UAH
T2LT anomaly data. The other free parameter is a scaling term which
controls the amplitude of zt(i). I chose this scaling term to yield a
temporal standard deviation of xt(i) that was close to the temporal
standard deviation of the monthly-mean UAH T2LT anomaly data. The
synthetic time series had the same length as the observational and model
data (252 months), and monthly-mean anomalies were calculated in the
same way as we did for observations and models.
For each of these 19 synthetic time series, I first calculated
least-squares linear trends and adjusted standard errors, and then
performed the "paired trends". The test involves all 171 unique pairs of
trends: b{1} versus b{2}, b{1} versus b{3},... b{1} versus b{19}, b{2}
versus b{3}, etc. I then calculate the rejection rates of the null
hypothesis of "no significant difference in trend", for stipulated
significance levels of 5%, 10%, and 20%. This procedure is repeated 1000
times, with 1000 different realizations of 19 synthetic time series. We
can therefore build up a distribution of rejection rates for N = 19, and
then do the same for N = 20, etc.
The "paired trend" results are plotted as the blue lines in Figure 3.
Encouragingly, the percentage rejections of the null hypothesis are
close to the theoretical expectations. The 5% significance tests yield a
rejection rate of a little over 6%; 10% tests have a rejection rate of
over 11%, and 20% tests have a rejection rate of 21%. I'm not quite sure
why this slight positive bias arises. This bias does show some small
sensitivity (1-2%) to choice of the a1 parameter and the scaling term.
Different choices of these parameters can give rejection rates that are
closer to the theoretical expectation. But my parameter choices for the
AR-1 model were guided by the goal of generating synthetic data with
roughly the same autocorrelation and variance properties as the UAH
data, and not by a desire to get as close as I possibly could to the
theoretical rejection rates.
So why is there a small positive bias in the empirically-determined
rejection rates? Perhaps Francis can provide us with some guidance here.
Karl believes that the answer may be partly linked to the skewness of
the empirically-determined rejection rate distributions. For example,
for the N = 19 case, and for 5% tests, values of rejection rates in the
1000-member distribution range from a minimum of 0 to a maximum of 24%,
with a mean value of 6.7% and a median of 6.4%. Clearly, the minimum
value is bounded by zero, but the maximum is not bounded, and in rare
cases, rejection rates can be quite large, and influences the mean. This
inherent skewness must make some contribution to the small positive bias
in rejection rates in the "paired trends" test.
What happens if we naively perform the paired trends test WITHOUT
adjusting the standard errors of the trends for temporal autocorrelation
effects? Results are shown by the black lines in Figure 3. If we ignore
temporal autocorrelation, we get the wrong answer. Rejection rates for
5% tests are 60%!
We did not publish results from any of these synthetic data experiments
in our 2000 JGR paper. In retrospect, this is a bit of a shame, since
Figure 3 nicely shows that the adjustment for temporal autocorrelation
effects works reasonably well, while failure to adjust yields completely
erroneous results.
Now consider the red lines in Figure 3. These are the results of
applying the Douglass et al. "consistency test" to synthetic data.
Again, let's consider the N = 19 case first. I calculate the trends in
all 19 synthetic time series. Let's consider the first of these 19 time
series as the surrogate observations. The trend in this time series,
b{1}, is compared with the mean trend, b{Synth}, computed from the
remaining 18 synthetic time series. The Douglass sigma{SE} is also
computed from these 18 remaining trends. We then form a test statistic
d2 = (b{1} - b{Synth}) / sigma{SE}, and calculate rejection rates for
the null hypothesis of no significant difference between the mean trend
and the trend in the surrogate observations. This procedure is then
repeated with the trend in time series 2 as the surrogate observations,
and b{Synth} and sigma{SE} calculated from time series 1, 3, 4,..19.
This yields 19 different tests of the null hypothesis. Repeat 1,000
times, and build up a distribution of rejection rates, as in the "paired
trends" test.
The results are truly alarming. Application of the Douglass et al.
"consistency test" to synthetic data - data generated with the same
underlying AR-1 model! - leads to rejection of the above-stated null
hypothesis at least 65% of the time (for N = 19, 5% significance tests).
As expected, rejection rates for the Douglass consistency test rise as
N increases. For N = 100, rejection rates for 5% tests are nearly 85%.
As my colleague Jim Boyle succinctly put it when he looked at these
results, "This is a pretty hard test to pass".
I think this nicely illustrates the problems with the statistical
approach used by Douglass et al. If you want to demonstrate that modeled
and observed temperature trends are fundamentally inconsistent, you
devise a fundamentally flawed test is very difficult to pass.
I hope to have a first draft of this stuff written up by the end of next
week. If Leo is agreeable, Figure 4 of this GRL paper would show the
vertical profiles of tropical temperature trends in the various versions
of the RAOBCORE data, plus model results.
Sorry to bore you with all the gory details. But as we've seen from
Douglass et al., details matter.
With best regards,
Ben
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Benjamin D. Santer
Program for Climate Model Diagnosis and Intercomparison
Lawrence Livermore National Laboratory
P.O. Box 808, Mail Stop L-103
Livermore, CA 94550, U.S.A.
Tel: (925) 422-2486
FAX: (925) 422-7675
email: santer1@llnl.gov
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