Journal of Geoscience and Environment Protection, 2014, 2, 144-152
Published Online June 2014 in SciRes. http://www.scirp.org/journal/gep
http://dx.doi.org/10.4236/gep.2014.23019
How to cite this paper: Strupczewski, W. G. et al. (2014). On Return Periodof the Largest Historical Flood. Journal of
Geoscience and Environment Protection, 2, 144-152. http://dx.doi.org/10.4236/gep.2014.23019
On Return Periodof the Largest Historical
Flood
Witold G. Strupczewski1, Krzysztof Kochanek1, Ewa Bogdanowicz2
1Institute of Geophysics, Polish Academy of Sciences, Księcia Janusza, Warsaw, Poland
2Institute of Meteorology and Water Management, Podleśna, Warsaw, Poland
Email: wgs@ igf. edu .pl , kochanek@igf.edu.pl, Ewa.Bogdanowicz@imgw.pl
Received April 2014
Abstract
The use of nonsystematic flood data for statistical purposes depends on reliability of assessment
both flood magnitudes and their return period. The earliest known extreme flood year is usually
the beginning of the historical record. Even though the magnitudes of historic floods are properly
assessed, a problem of their retun periods remains unsolved. Only largest flood (XM) is known
during whole historical period and its occurrence carves the mark of the beginning of the
historical period and defines its length (L). So, it is a common practice of using the earliest known
flood year as the beginning of the record. It means that the L value selected is an empirical
estimate of the lower bound on the effective historical length M. The estimation of the return
period of XM based on its occurrence, i.e .
ˆ
M=L
, gives the severe upward bias. Problem is to
estimate the time period (M) representative of the largest observed flood XM. From the discrete
uniform distribution with support of the probability of the L position of XM one gets
ˆ
M= L2
which has been taken as the return period of XM and as the effective historical record length. The
efficiency of using the largest historical flood (XM) for large quantile estimation (i.e. one with
return period T = 100 years) has been assessed using maximum likelihood (ML) method with
various length of systematic record (N) and various estimates of historical period length
ˆ
M
com-
paring accuracy with the case when only systematic records alone (N) are used. The i-th simula-
tion procedure incorporates systematic record and one largest historic flood (XMi) in the period M
which appeared in the Li year backward from the end of historical period. The simulation result
for selected distributions, values of their parameters, different N and M values are presented in
terms of bias (B) and root mean square error (RMSE) of the quantile of interest and widely
discussed.
Keywords
Flood Frequency Anal ysis, Historical Inf orma tion, Error Analysis, Maximum Likelihood,
Monte Carlo Simulati ons
1. Introduction
In the flood engineering there is usually a need to determine the flood of a given return period T years, i.e. the
W. G. Strupczewski et al.
145
flood quantile XT or design flood. The problems with the assessment stem from short time series (N = T), un-
known probability distribution function of annual peaks, error corrupted data, simplifying assumptions as of
identical independently distributed (i.i.d.) data and, in particular, the stationarity of relatively long series. All
these may cause a high uncertainty of upper quantile estimate. The only effect of a sample size is widely docu-
mented for various distribution models and estimation methods. Inclusion into Flood Frequency Analysis (FFA)
other sources of error would result in increasing uncertainty of design flood estimate. This is a feature not ap-
preciated by the engineers as they desire to have only one value for designing flood related structures.
To improve the accuracy of estimates of upper quantiles all possible sources of additional information are
used such as all independent peaks above the threshold, seasonal approach, regional analysis, record aug me nt -
tation by correlation with longer nearby records and augmentation of the systematic records by historical and
paleoflood data.
Frequency analysis of flood data arising from systematic, historical, and paleoflood records has been pro-
posed by several investigators (e.g. a review Stedinger & B a ke r, 1987, Frances et al., 1994). The use of non sys-
tematic flood data for statistical purposes depends on reliability of assessment both flood magnitudes and their
return period. If the historical record is available, you can find information about the floods larger than prevail-
ing majority of floods reported in the systematic record and in particular about the largest of all reported floods.
Serious difficulties are related to the availability and exhaustiveness of historical information, the quality and
accuracy of historical sources. Depending on the parameter number and their method of estimation, the esti-
mates of high quantiles are more or less sensitive to the largest observed floods.
The Gumbel, log Gumbel and Weibull distributions together with maximum likelihood method (ML) was
considered by Frances et al. (1994). To assess the statistical profit from historical information the asymptotic
variances of the quantile estimates got from the systematic records alone and the combined timeseries were
compared and in addition they were compared with computer simulation experiments’ results. The results of
their study performed for define length (M) of historical period indicate that value of historical data for estimat-
ing flood quantiles can be small or large depending on only three factors: the relative magnitudes of the length
of the systematic record (N) and the length of the historical period (M); the return period (T) of the flood quan-
tile of interest, and the probability threshold defining the historical floods.
Most often the first hydrological historical notice concerns a large flood and therefore it is not known what
had happened before. Then the date of the first recorded historical flood determines (is taken as) the historical
memory length L, i. e. L is the duration of nonsystematic period commencing on the large flood. Even if the
magnitudes of historic floods are properly assessed, a problem of their retun periods remains unsolved. Many of
the literature examples (specially Be nso n (1950), D al r ymp l e (1960), IAC WD (1962), Zha ng (1982) and NERC,
(1975: p. 177)) deal with effective length of historical record M used for frequency analysis which is always a
period from the first extraordinary flood to the beginning of the systematic record, i.e. L.
In other words, only the largest flood (XM) is known during whole historical period and its occurrence marks
the beginning of the historical period and defines its length (L) (Figure 1). It is because the beginning of the
historical period was somehow forced by the appearance of the largest flood then its magnitude (XM) likely cor-
responds to a longer return period than L (or if in systematic record all observations are smaller than XM then to
(L + N) - period). Consequently, the upward bias of the upper quantile estimates can be expected, if the histori-
cal period of length L is taken in FFA as the nonsystematic observation period, or coming from an underestima-
tion of the return period (
ˆ=ML
) of XM value .
Problem is to estimate the time period (M) representative of the largest observed flood XM, to evaluate the ef-
ficiency of using the largest historical flood (XM) for large quantile estimation and to compare it with the case
when only systematic records alone (N) are used. To keep and preserve for the FFA the unspoiled genuine in-
formation contained in the observation (XM, L), the return period
( )
ˆ
M
of the largest observed historical flood
XM should be assessed without using the data from the systematic record and only the information that the sys-
tematic record does not contain the flood larger than the XM value is utilized. Every effort should be taken to
establish M accurately on the basis of the occurrence of the largest recorded flood XM and an investigation of
any information prior to XM event.
Obviously the empirical return period of the historical flood assessed on the base of the year of occurrence L
(time span) represents just the lower limit of its empirical return period. There is an upper limit too, which,
however, can not be estimated unambiguously. This is due to a simple reason. If historical sources report the
occurence of a large flood in the given year, it is almost sure that if a similar or more serious flood had occurred
W. G. Strupczewski et al.
146
Figure 1. The case of N systematic and one largest flood in the
beginning of historical period.
the year before the mentioned flood, it would also has been noted and commented (Hirsch & Sted i nge r, 1987).
The same can be stated for horizon of two, three, four, etc. years. If we could identify this time span, we would
have determined the upper limit of the empirical return period.
2. Literature Review
The earliest and simplest procedures for employing historical and paleoflood data were based on plotting posi-
tions and graphical concepts (Zha n g, 1982, 1985, Bernieur et al., 1986, Wang & Adams, 1984; Hirsch, 1985;
Cohn, 1986). The common practice is using the earliest known flood year as the beginning of the historic record,
i.e. taking
. The estimation of M based on the date of the first extraordinary flood occurrence exacer-
bates the severe imprecision Defining as historical floods all floods during the M period above a given threshold
and taking four different plotting position formulas, Hirsch and Stedinger (1987) have illustrated by Monte
Carlo (MC) experiment the magnitude of the upward bias of the plotting position of the largest sample elements
if the earliest known high flood year (L) is taken as the beginning of the historical record. Doing so they notice
that L is a random variable, which is dependent on the flood-producing process itself that would be a violation of
the assumption of the plotting position formulae.
Hosking and Wallis (1986b) use the MC computer simulation to assess whether a single paleoflood estimate,
when included in a single-site ML flood frequency analysis procedures, it gives a worthwhile increase in the
accuracy of estimates of extreme floods. They find that the main factors affecting the utility of this kind of pa-
leological information are the specification of the fitted flood frequency (whether it has two or three unknown
parameters) and the size of the measurement error of paleodischarge estimates. Errors in estimating the date of
the paleoflood is considered as to be of minor importance. For distributions with higher CV or skewness the dif-
ference between the effects of the errors of the magnitude of paleoflood and its return period is smaller.
Note that the randomness of the systematic records time series of i.i.d. variable can also be so metimes que s-
tioned and undermined, for instance when the largest value XM of a time series intentionally terminates the
N-elements’ systematic record. Then the XM is the last element of the N-element time-series. Such a case may
arise when a water gauge was swept by a heavy flood (XM) and later not restored or intentionally as the conse-
quence of the hydrological moving network design focused on the assessment of the variability range of annual
peak flows. As before, the use of such a series in the FFA with
ˆ=ML
will lead to an overestimation of large
quantiles.
3. Problem Formulation
The object of the paper is to assess by ML method whether there is any use for FFA of the largest flood termi-
nating the time series assuming its magnitude (XM) is known. Therefore, the value of using the largest flood
terminating observation period relative to using records without it is examined by comparing the bias (B) and the
root mean square error (RMSE) of flood quantiles of two two-parameter distributions, namely Gumbel and
Weibull while applying the simulation experiments. The emphasis is put on the effect of misspecification of the
return period (M) of the largest historical (paleo-) flood (XM) and on the proper assesment of the M estimate on
the basis of XM occurrence (L). So far the above case has not been presented in the hydrological literature.
The theoretical framework of our research is based on Maximum Likelihood estimation which has been gen-
W. G. Strupczewski et al.
147
erally found to have desirable properties for combine systematic and historical information (Frances et al., 1994;
Stedinger & Cohn, 1986; Naulet et al. 2005). It is assumed that the annual maximum floods are independent and
identically distributed.
4. Assessment of the Return Period M of the XM flood
Dealing with the plotting positions Hirsch and Stedinger (1987) considered that the time of occurrence of the
earliest documented historical flood L as the random variable defining a lower bound of the sample size used for
computation of plotting positions. The position L of the largest in M period element (XM ) (Figure 1) is the ran-
dom variable being discretely uniformly distributed in the M period, i.e. pt = 1/M for t = 1, 2M. Obviously
the magnitude of the largest element (XM) is also a random variable. It can correspond in the population to a
smaller or larger value of the exceedance probability than 1/M defining the true return period (MR) of the ob-
served XM, therefore, the difference (MRL) is not restricted in sign.
Assume that the return interval (M) of XM is known. As L is unformly distributed variable in the M length
time series with support L [0, 1, …, M], one gets E(L) = M/2 and V(L) = M2/12. In reality M is not known and
its assesment is our goal. Taking the observed L value as the estimate of the expecting value, i.e. L = E(L) we get
the M estimate equal
ˆ2ML=
. Because regardless of the estimation method the quantile estimators are not in
general linear function of
ˆ
M
, the minimum bias of quantile
( )
( )
ˆ
ˆˆ

= −


ppp
BxEx Mx
does not necessarily
correspond to the zero-bias of
ˆ
M
, i.e. to
ˆ2=ML
. As in the systematic period (N) all its elements are smaller
than XM, one can get
()
ˆ2= +
M LN
.
5. Simulation Procedure
The simulation procedure described here incorporates N systematic record and one largest historic flood (XM) in
the period M which appeared in the L year backward from the end of historical period (Figure 1). Obviously the
systematic record and both magnitude (XM) and year of occurrence (L) randomly vary from simulation to simu-
lation. As an estimate of the length of the historical period shall be success ive l y
ˆ,2=MLL
and the actual
value
ˆ=MM
.
Generate a gauged record x1, x2, …, xN of independent random variates from the assumed (two-parameter)
flood-like distribution [F(x)] with parameters chosen to give specified values of CV.
Generate historical series of the same distribution of the length M, i. e. y1, y2, …, yM, and find the maximum
event (XM) of the historical series denoting the time (L) of its occurrence. Since the random variables (XM) and
L are mutually independent the XM can be generated from the distribution of the largest element in a M-element
series, i.e. F(M) = F1, M(y) = FM(y), while the corresponding time of its occurrence (L) from the discrete uniform
distribution with support {1, 2, …, M}.
Fit a flood frequency distribution by the method of maximum likelihood. If the fitted distribution has a distri-
bution function F(x, θ) and a density function f(x, θ), where θ is a vector of unknown parameters, then the like-
lihood function (L) is taken to be
()( )( )
( )
ˆ1
1
;,;; ;
=

== ⋅= ⋅


Lθθ θ θ
N
M
x xxi
i
x yFyXMfyXMfx
, (1)
i.e., the use of incomplete data likelihood, where
ˆ,2and =MLL M
and for systematic record
( )
( )
1
;;
=
=
Lθ θ
N
xi
i
x fx
. (2)
Calculate quantile estimates
( )
1
ˆ
ˆ11 ;
=− θ
T
XF T
for
ˆ,2and =MLL M
and the systematic record (N)
only (i.e. when
ˆ0=M
), where F–1 is the inverse distribution function of the fitted flood frequency distribution,
ˆ
θ
is the maximum likelihood estimate of , and T is the return period of interest.
Repeat steps 1 4 a large number of times (i) and calculate the mean and variance of
ˆ
T
X
, and hence the
relative bias RB and relative RMSE of
ˆ
T
X
taking
ˆ,2and =
iii
M LLM
and the systematic record (N) only
(
ˆ0M=
), considered as an estimator of the true quantile
W. G. Strupczewski et al.
148
( )
111 ;
= −
T
X FTq
If in a generated series one gets max(x1, x2, …, xN) XM such a series is ignored which allows us to assume
ˆ2=ML
.
6. Simulation Results
Results of simulation experiments are shown for Gumbel and Weibull distribution with four values of the coef-
ficient of variation CV = 0.25, 0.5, 0.75, 1.0, two length of systematic records N = 15, 50 and the length of ef-
fevtive historical period M = Nexp( a) where a [0,3]. Due to the limited capacity of this paper without the loss
of generality, only the selected results were presented in Figures 2-5, namely for CV = 0.25 and 1.0; the results
for CV = 0.5 and 0.75 locate themselves between those presented in the Figures. Results got for the correct value
of the return period (
ˆ=MM
) are compared with those got for
ˆ,2=
ii
MLL
. For completion the results for the
systematic record only (i.e.
ˆ0=M
) were presented in all Figures. Of course, for this case the results does not
depend on M and, in consequence, on log(M/N).
7. Discussion Results
The shorter the gauged record (N), the more useful historical information would be;
Using as the estimate of the return period of largest historical flood (XM) the historical memory length (L)
results in upward bias RB exceeding the bias got while using the systematic record only. Its value is growing
with CV (and CS). It is accompanied by reduction of RMSE;
Using in ML estimation the exact return period (M) of the largest historical flood (XM) the bias is reduced
and R MSE is considerable lower;
(a) (b)
(c) (d)
Figure 2. Relative bias (RB) and relative root mean square error (RRMSE) of
100
ˆ=T
X
for gauge record length N = 15 as a function of historic period M for
ˆ0,,2 ,.=
i ii
ML LM
Parent distribution Gumbel with CV equal: (a) 0.25 and (b)
1.0. Fitted distribution Gumbel.
Gumbel - Relative bias
CV = 0.25, N = 15
-2
-1
0
1
2
3
4
5
6
0.0 1.02.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Gumbel - Relative bias
CV = 1.0, N = 15
-4
-2
0
2
4
6
8
10
0.0 1.0 2.0 3.0
log (M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Gumbel - Relative RMSE
CV = 0.25, N = 15
6
7
8
9
10
11
12
0.0 1.0 2.0 3.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
Gumbel - Relative RMSE
CV = 1.0, N = 15
10
12
14
16
18
20
0.0 1.0 2.0 3.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
W. G. Strupczewski et al.
149
(a) (b)
(c) (d)
Fig ure 3. RB and RRMSE of
100
ˆ=T
X
for gauge record length N = 50 as a
function of historic period M for
ˆ0,,2 ,.
=
i ii
ML LM
Parent distribution
Gumbel with CV equal (a) 0.25 and (b) 1.0. Fitted distribution Gumbel.
(a) (b)
(c) (d)
Fig ure 4. RB and RRMSE of
100
ˆ=T
X
and gauge record length N = 15 for
historic period M for
ˆ0,,2 ,.=
i ii
ML LM
Parent distribution Weibull with CV
equal (a) 0.25 and (b) 1.0. Fitted distribution Weibull.
Gumbel - Relative bias
CV = 0.25, N = 50
-1.0
-0.5
0. 0
0. 5
1. 0
1. 5
2. 0
2. 5
3. 0
0.0 1.0 2.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Gumbel - Relative bias
CV = 1.0, N = 50
-1.0
0. 0
1. 0
2. 0
3. 0
4. 0
5. 0
0.0 1.02.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Gumbel - Relative RMSE
CV = 0.25, N = 50
4. 0
4. 5
5. 0
5. 5
6. 0
6. 5
0.0 1.0 2.03.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
Gumbel - Relative RMSE
CV = 1.0, N = 50
7. 5
8. 0
8. 5
9. 0
9. 5
10.0
10.5
11.0
0.01.0 2.03.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
Weibull - Relative bias
CV = 0.25, N = 15
-2
-1
0
1
2
3
0.01.0 2.03.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Weibull - Relative bias
CV = 1.0, N = 15
-4
-2
0
2
4
6
8
10
12
14
0.0 1.0 2.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Weibull - Relative RMSE
CV = 0.25, N = 15
2
3
4
5
6
7
8
0.0 1.0 2.0 3.0
log (M/N)
RRMSE (in %)
Systematic
Li
2Li
M
Weibull - Relative RMSE
CV = 1.0, N = 15
12
17
22
27
32
0.0 1.0 2.0 3.0
log (M/N)
RRMSE (in %)
Systematic
Li
2Li
M
W. G. Strupczewski et al.
150
(a) (b)
(c) (d)
Fig ure 5. RB and RRMSE of
100
ˆ=T
X
and gauge record length N = 50 for
historic period M for
ˆ0,,2 ,.=
i ii
ML LM
Parent distribution Weibull with CV
equal (a) 0.25 and (b) 1.0 and N = 50. Fitted distribution Weibull.
Therefore to benefit from the largest historical observation every effort should be made to establish M accu-
rately;
In the absence of any information about the period preceding the occurrence of XM one should put
ˆ
M
equal 2L or 2(L + N).
The use of
ˆ2ML
=
instead of
reduces the bias more than twice, but it is still ca 40% larger than
the bias obtained at a known return period M of XM, and comparable or lower than the bias from systematic
record (N) .
The inclusion of the largest historical flood in FFA with
ˆ2ML=
(i. e . the effective historical record length)
gives the substantial reduction in RRMSE of extreme flood estimates, however it is ca 40% lower than if the
true M value would be available.
The benefit from including the largest historical flood measured by the reduction of bias and RMSE depends
on:
1) the length of systematic record (N),
2) the ratio of the true return period of XM, i.e. M to N,
3) the ratio of N to the return period of quantile of interest T,
4) the CV and skewness of the parent distribution.
8. Conclusions
Errors in historical data of course diminish the utility of the data for improvement the estimate of the flood mag-
nitude at the given return period. In the simulations which produced Figures 2-5 it was assumed that the magni-
tude of largest historical flood (XM) was measured without error and the same was assumed for systematic re-
cord. It is realistic to suppose that the XM flood was measured much less accurate than the gauged record. Error
in estimating the largest historical magnitude (XM) is much more important than error in estimating the date of
its occurrence (e.g. Hosking & W allis, 1986). It is significant that inspi re d by the practice of efforts to improve
the accuracy of estimates of flood quantiles through a fuller use of the information they give just the opposite
Weibull - Relative bias
CV = 0.25, N = 50
-1.0
-0.5
0. 0
0. 5
1. 0
1. 5
2. 0
0.0 1.0 2.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Weibull - Relative bias
CV = 1.0, N = 50
-2
0
2
4
6
8
0.0 1.0 2.0 3.0
log(M/N)
Relative bias (in %)
Systematic
Li
2Li
M
Weibull - Relative RMSE
CV = 0.25, N = 50
1. 5
2. 0
2. 5
3. 0
3. 5
4. 0
4. 5
0.0 1.0 2.03.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
Weibull - Relative RMSE
CV = 1.0, N = 50
8
10
12
14
16
18
0.0 1.0 2.0 3.0
log(M/N)
RRMSE (in %)
Systematic
Li
2Li
M
W. G. Strupczewski et al.
151
effect leading to increased uncertainty of flood estimates. On top of that, this already significant uncertainty is
magnified by the unknown non-stationarity of the river’s regime over such a long time.
It remains to refer to the general problem of historical information when the applied distribution model is
false, what is always the case (Strupczewski et al., 2002a, b; Węglarczyk et al., 2002). It is obvious that the dif-
ferent distribution models fitted to the same systematic observations can give large differences in estimates of
high quantiles. Supplementing systematic records by historical floods for FFA would reduce these differences
and make the estimates more accurate. On the other hand, the uncertainty of the paleohistorical floods (both in
terms of their magnitude and return period) combined with considerable increase of the complication of the
problem (when compared to analysis of systematic data only) provoke a question whether the whole operation is
worth a candle. Therefore, whether to include the palehistorical information or turn a blind eye to it is a matter
of conscience.
Acknowledgem ents
This research project was partly financed by the grant of the Polish National Science Centre titled Modern sta-
tistical models for analysis of flood frequency and features of flood waves, decision nr DEC-2012/05/B/
ST10/00482.
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