YODEN%20Shigeo - PowerPoint PPT Presentation

About This Presentation
Title:

YODEN%20Shigeo

Description:

March 3-4, 2005: SPARC Temperature Trend Meeting at University of Reading Spurious Trend in Finite Length Dataset with Natural Variability YODEN Shigeo – PowerPoint PPT presentation

Number of Views:53
Avg rating:3.0/5.0
Slides: 54
Provided by: yod80
Category:

less

Transcript and Presenter's Notes

Title: YODEN%20Shigeo


1
March 3-4, 2005 SPARC Temperature Trend Meeting
at University of Reading
Spurious Trend in Finite Length Dataset with
Natural Variability
  • YODEN Shigeo
  • Dept. of Geophysics, Kyoto Univ., JAPAN
  1. Introduction
  2. Statistical considerations
  3. Internal variability in a numerical model
  4. Spurious trend experiment
  5. Concluding remarks

2
1. Introduction
  • Causes of interannual variations of
  • the stratosphere-troposphere coupled system

3
  • Observed variations

4
Linear Trend of the Monthly Mean
Temperature ( Berlin, NCEP )
A spurious trend may exist in finite length
dataset with natural variability.
5
2. Statistical considerations
  • Nishizawa and Yoden (2005, JGR in press)
  • Linear trend
  • We assume a linear trend
  • in a finite-length dataset with random
    variability
  • Spurious trend
  • We estimate the linear trend
  • by the least square method
  • We define a spurious trend as

N 5 10 20
N 50
6
  • Moments of the spurious trend
  • Mean of the spurious trend is 0
  • Standard deviation of the spurious trend is
  • Skewness is also 0
  • Kurtosis is given by

standard deviation of natural variability
Monte Carlo simulation with Weibull (1,1)
distribution
kurtosis of natural variability
7
  • Probability density function (PDF)
  • of the spurious trend
  • When the natural variability is Gaussian
    distribution
  • When it is non-Gaussian
  • Edgeworth expansion of the PDF
  • Cf. Edgeworth expansion of sample mean (e.g.,
    Shao 2003)

8
  • Non-Gaussian distribution

Edgeworth expansion of the cumulative
distribution function, of
is written by and and is
the PDF and the distribution function of
, respectively. where is k - th
Hermite polynomial and is k - th cumlant (
).
9
  • Errors of t -test, Bootstrap test, and Edgeworth
    test for a non-Gaussian distribution of
    for a finite data length N

10
We need accurate values of the moments of natural
internal variability for accurate statistical
text.
But the length of observed datasets is at most
50 years.
11
3. Internal variability in a numerical model
  • 3D global Mechanistic Circulation Model
  • Taguchi, Yamaga and
  • Yoden(2001)
  • simplified physical processes
  • Taguchi Yoden(2002a,b)
  • parameter sweep exp.
  • long-time integrations
  • Nishizawa Yoden(2005)
  • monthly mean T(90N,2.6hPa)
  • based on 15,200 year data
  • reliable PDFs

12
  • Labitzke diagram for normalized temperature
    (15,200 years)

stratosphere
troposphere
Different dynamical processes produce these
seasonally dependent internal variabilities ? An
nual mean may introduce extra uncertainty or
danger into the trend argument
13
  • Estimation error of sample moments
  • depends on deta length N and PDF of internal
    variability
  • Normalized sample mean (mN -µ)/se
  • Standard deviation of sample mean
  • The distribution converges to a normal
    distribution

14
  • Spatial and seasonal distribution of moments
  • 10 ensembles of 1,520-year integrations
  • without external trend
  • 65
  • More information
  • moments of variations ? moments of spurious trends

15
  • How many years do we need
  • to get statistically significant trend ?
  • - 0.5K/decade in the stratosphere
  • 0.05K/decade in the troposphere

Max value of the needed length Month
for the max value
16
(No Transcript)
17
  • How small trend can we detect
  • in finite length data with statistical
    significance ?

50-year data
20-year data K/decade
K/decade
18
4. Spurious trend experiment
  • Cooling trend run
  • 96 ensembles of 50-year integration
  • with external linear trend
  • -0.25K/year around 1hPa

Normal (present) Cooled (200 years)
Difference

K/50years
19
JAN (large internal variation)
20
Ensemble mean of estimated trend and standard
deviation of spurious trend
21
  • Comparison of significance tests
  • Edgeworth test true
  • The worst case in 96 runs
  • but both test look good

22
  • Application to real data
  • 20-year data of NCEP/NCAR reanalysis

23
Bootstrap test
t-test
24
5. Concluding remarks
  • Recent progress in computing facilities has
  • enabled us to do parameter sweep experiments
  • with 3D Mechanistic Circulation Models.
  • Very long-time integrations (15,000 years)
  • give reliable PDFs (non-Gaussian, bimodal, .
    ),
  • which give nonlinear perspectives
  • on climatic variations and trend.
  • Statistical considerations on spurious trend
  • in general non-Gaussian cases
  • Edgeworth expansion of the spurious trend PDF
  • detectability of true trend for finite data
    length
  • enough length of data, enough magnitude of
    trend
  • evaluation of t-test and bootstrap test

25
  • Ensemble transient exp.(e.g., Hare et al., 2004)
    vs.
  • Time slice (perpetual) exp.(e.g., Langematz,
    200x)
  • assumption
  • internal variability is independent of time
  • m - member ensembles of N - year transient runs
  • estimated trend in a run
  • mean of the estimated trends
  • two L-year time slice runs
  • estimated mean in each run
  • estimated trend
  • comparison under the same cost mN 2L

26
  • Statistics of internal variations of the
    atmosphere
  • could be well estimated by long time
    integrations
  • of state-of-the-art GCMs.
  • Those give some characteristics of the nature
    of
  • trend.
  • New Japan reanalysis data JRA-25
  • now internal evaluation is ongoing

27
  • Time series of monthly averaged zonal-mean
    temperature
  • January

28
  • Estimated trend K/decade

90N
29
  • Normalized estimated trend and significance

90N
30
Thank you !
31
  • Estimated trend K/decade

90N
32
  • Normalized estimated trend and significance

90N
33
Daily Temperature at 30 hPa K for 19 years
(1979-1997)
1. Introduction
  • Difference of the time variations between the
    two hemispheres
  • annual cycle periodic response to the solar
    forcing
  • intraseasonal variations mostly internal
    processes
  • interannual variations external and internal
    causes

North Pole
34
  • Difference of Gaussian distribution and Edgeworth
    for a non-Gaussian distribution of for a
    finite data length N

35
3. Spurious trends due to finite-length
datasets with internal variability
  • Nishizawa, S. and S. Yoden, 2005
  • Linear trend
  • IPCC the 3rd report (2001)
  • Ramaswamy et al. (2001)
  • Estimation of sprious trend
  • Weatherhead et al. (1998)
  • Importance of variability
  • with non-Gaussian PDF
  • SSWs
  • extreme weather events
  • We do not know
  • PDF of spurious trend
  • significance of the estimated
  • value

36
Normalized sample variance
stratosphere
troposphere
  • The distribution is similar to ?2distribution in
    the troposphere, where internal variability has
    nearly a normal distribution
  • Standard deviation of sample variance

37
Sample skewness
stratosphere
troposphere
38
Sample kurtosis
stratosphere
troposphere
39
  • Years needed for statistically significant trend
  • -0.5K/decade in the stratosphere
  • 0.05K/decade in the troposphere

40
(No Transcript)
41
(No Transcript)
42
  • Significance test of the estimated trend
  • t-test
  • If the distribution of is Gaussian,
  • then the test statistic
  • follows the t-distribution with the
    degrees of freedom n -2

43
2. Trend in the real atmosphere
  • Datasets
  • ERA40
  • 1958-2002
  • 1000-1 hPa
  • NCEP/NCAR
  • 1948-2003
  • 1000-10 hPa
  • JRA25
  • 1979-1985,1991-1997
  • 1000-1 hPa
  • Berlin Stratospheric data
  • 1963-2000
  • 100-10 hPa

44
EQ
  • Time series
  • of monthly averaged zonal-mean temperature
  • January

90N
50N
45
EQ
July
90N
50N
46
  • Same period (1981-2000)
  • January

90N
50N
47
July
90N
50N
48
  • Same vertical factor
  • January

90N
50N
49
July
90N
50N
50
  • Mean
  • 90N

Mean difference
from ERA40
51
50N
Mean difference
from ERA40
52
  • standard deviation
  • 90N

stddev difference
from ERA40
53
50N
stddev difference
from ERA40
Write a Comment
User Comments (0)
About PowerShow.com