成層圏 対流圏結合系における...
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成層圏-対流圏結合系における
極端気象変動の現象論
余田 成男
京都大学 大学院理学研究科 地球惑星科学専攻
数学協働プログラム研究集会「地球科学における極端現象と疎構造」京都大学数理解析研究所 2014年11月13・14日
極端気象変動(変化)
IPCC, 2012: Summary for Policymakers. In: Managing the Risks of Extreme Events and Disasters to Advance Climate Change Adaptation [Field, C.B., et al., Eds.]
Figure SPM.3: The effect of changes in temperature distribution on extremes.
Different changes in temperature distributions between present and future climate and their effects on extreme values of the distributions.
研究の学術的背景
成層圏突然昇温現象
極端気象変動の典型
周極渦の変形・崩壊非線型性の強い地球規模の力学的現象
その出現予測は大変難しい問題
北極上空 10hPa(~高度30 km)での気温 [K] の時間変化
70 K
Mukougawa et al. (2012)
5 日
2009年
突然昇温時の周極渦の時間変化 (3日間隔)
寒
寒北極
7/18
アニメーション: 2009年1月における北極域周極渦の3次元構造の時間発展
野口 峻佑 (2014)https://sites.google.com/a/dpac.dpri.kyoto-u.ac.jp/noguchi/Home/research
dynamical interpretation of SSWs with TEM equations TEM equations
generalized E-P relationship
Equator WinterPole
dA/dt > 0div F < 0W
W
C
CdU/dt < 0
V > 0
downward control(Haynes et al. 1991)
time
A
amplification
thermal gradient –windshear balance
成層圏-対流圏結合系の多重時間スケール変動像2008~11年の科学研究費基盤(A)の成果
北半球では、冬季に大きな日々・季節内・年々の変動
月平均気温の頻度分布は、冬季には大きく歪み、バイモーダルにも
220 240 260 280 [K]
6月
7月
8月
9月
10月
11月
12月
1月
2月
3月
4月
5月
北極上空での月平均気温の頻度分布15,200年分の力学モデル実験Nishizawa and Yoden (2005)
2000年代
1990年代
北極上空での気温の季節内変動・年々変動 Noguchi and Yoden (2012)
7 9 11 1 3 5 月
研究目的
本研究は、成層圏-対流圏結合系における
極端気象変動の力学的関連性の総合的な理解と
その予測能力の向上を目的とする
現在気候の観測・予報データ解析による
結合系変動の現状把握と、
過去気候の再現実験による
モデル検証・改良を踏まえて、
予測の不確実性を押さえて
未来気候の結合系変動に対する影響評価を行う
独創性及び革新性
① 成層圏突然昇温現象という極端気象を、
強非線型性な力学現象の不規則で稀な出現と認識
非ガウス型確率密度関数の先端部に関わる統計解析
複雑精緻な気候モデルではどうか ?
過去気候ではどうだったか ?
将来気候ではどうなるのか ?
220 240 260 280 [K]
12月
1月
2月
Nishizawa and Yoden (2005)
出現間隔の統計:
ポアソン過程?
極端気象変動に関する統計則
従来の経験則風速: ワイブル分布
降雨量: ガンマ分布
雲特性: 対数正規分布
・・・・・・
周極渦崩壊の形態学観測事例数の不足
数値実験による代用
計算結果データに基づいて経験則をつくる
vs 演繹的な法則
強非線型現象の不規則で稀な出現
独創性及び革新性
② あらゆる階層の数値モデルを用いて系統的に実験
○ 理想化簡略化した低次元モデル(LOM)100~101自由度; 簡単概念・定性的
○ 全球3次元の力学モデル(MCM)104~106自由度; メカニズム理解
○ 大気大循環モデル(GCM),数値天気予報モデル(NPM),気候モデル(CGCM)106~109自由度; 複雑精緻・定量的
1980年代は低次元モデル、
1990年代からは3次元力学モデル、
これからは、複雑精緻モデルも総合的に活用
波及効果
① 過去気候の再現実験
古気候学・古環境情報学との融合研究の推進
京都大学理学研究科と気象研究所の間で共同研究契約を締結済
気候モデルによる縄文期気候再現実験Kitoh (2012)
1月 5月 9月
2月 6月 10月
3月 7月 11月
4月 8月 12月
月平均地表気温の現代気候との差
波及効果
② アンサンブル実験データを活用して、
極端気象変動の予測可能性に関する新たな枠組みを構築
異常天候の予測能力の向上に貢献
2009年成層圏突然昇温現象の気象庁1ヶ月アンサンブル予報結果 Mukougawa (2012)
ー 観測結果ー アンサンブル予報
(50メンバー)
SPARC / SNAPStratospheric Network for the Assessment of Predictability
初期時刻
初期時刻
初期時刻に依存した予測可能性
観測結果
アンサンブル予報
The 6th IAGA/ICMA/CAWSES workshop on "Long-Term Changes and Trends in the Atmosphere" NCAR, Center Green Conference Center, Boulder, Colorado, USA, June15–18, 2010 -alpha
1. Introduction2. Spurious trend in a finite-length dataset3. Seasonally dependent detectability 4. Concluding remarks
Long-term trends in stratospheric temperatureand their detectability in future simulations
under the situation of large natural variability
YODEN ShigeoDept. of Geophysics, Kyoto Univ., JAPAN
stratospheric temperature trends Randel, W. J., et al. (2009, JGR )
“An update of observed stratospheric temperature trends” limited time period of observations
• radiosonde network (1958~)• NOAA operational satellites (MSU:1979~2007, SSU:1979~2005)
homogeneity adjustment is necessary
1. Introduction
Radiosonde stations for RATPAC-lite dataset
large seasonal dependence large latitudinal dependence large height dependence
Temperature trends:1979–2005SSU & MSU4; 60N–60S
El Chichon Pinatubo
RATPAC-lite
T(solar max) – T(solar min) [K]
anthropogenic influences (mostly?)• increase of CO2, H2O, …; decrease of O3, …
natural influences• large volcanic eruptions, 11-year solar cycle
large natural variability
South Pole(NCEP)
North Pole(NCEP)
North Pole(Berlin)
courtesy ofDr. Labitzke
natural variability in the stratosphere Labitzke diagram
histograms of the monthly mean T (p=30 hPa)Length of the observed dataset isat most 50 years.
Only numerical experimentscan supply much longer datasets
to obtain statistically significant results,although they are not real but virtual.
7 models with volcanic aerosol heating Temperature trends:1980–1999global mean
numerical simulations with high-end climate models Austin, J., et al. (2009, GRL ) “Coupled chemistry climate
model simulations of stratospheric temperatures and their trends for the recent past”
In this talk Nishizawa and Yoden (2005, JGR )
“Distribution functions of a spurious trend in a finite length data set with natural variability: Statistical considerations and a numerical experiment with a global circulation model”
analysis with a simple linear trend model with non-Gaussian natural variability (Edgeworth expansion)
seasonally dependent detectability of a linear trend
linear trend+
random variability
N=5N=5N=10N=20N=50
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
( ) ( ), 1, ,i iX n an b n n Nε= + + =
ˆˆ ˆ( )i i iX k a k b= +
1
ˆ'12'
( 1)( 1)1 ( )
2
i i
i
N
in
a a a
aN N N
Nn n ε=
= −
=+ −
+ × −
∑
( )i nε
N = 5 10 20
N = 50
2. Spurious trend in a finite-length dataset
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
32
'12 12
( 1)( 1)a NN N N ε εσ σ σ
−= ≈
+ −
standard deviation ofnatural variability
kurtosis ofnatural variability
+ Monte Carlo simulationwith Weibull (1,1) distribution
Probability density function (PDF)of the spurious trend
When the natural variability is Gaussian distribution
When it is non-GaussianEdgeworth expansion of the PDF Cf. Edgeworth expansion of sample mean (e.g., Shao 2003)
( )
2
'2
'
12
' 0,'
1( ) ( ) .2
a
a
x
a Na
f x f x e σσ πσ
−
= =
Distribution function of the spurious trend Edgeworth expansion
where and are PDF and CDF of , respectivelyand
where is k-th Hermite polynomialand is k-th cumlant of ( )
For further details, see Nishizawa and Yoden (2005; JGR)
(0,1)N
An example of Weibull(1,1),of which
seasonal dependence of internal interannual variabilityis large in temperature at the North Pole due to the occurrence of SSWs in winter stratosphere breakdown of the polar vortex is a highly nonlinear process
3. Seasonally dependent detectability
Real atmosphere (Berlin data) MCM(15,200years)30hPa 2.6hPa
Labitzke diagram of the polar stratospheric [T] (Nishizawa and Yoden, 2005, JGR )
stratosphere troposphere
Different dynamical processes produce these seasonally
dependent internal variability↓
“Annual mean” may introduceextra uncertainty or danger
into trend studies
non-Gaussian nature of internal interannual variability Nishizawa and Yoden (2005, JGR ) normalized pdfs of monthly [T] at the north pole
Example of cooling trend run- 96 ensembles of 50-year integration- with external linear trend
-0.25K/year around 1hPa
Natural variability small in summer (July) large in winter (Feb.)
a cooling trend experiment 96 ensembles of 50-year integration
with external linear trend -0.25K/year around 1hPa
necessary data length [years]to detect a linear trend of- 0.5K/decade with 90% conf.
month
pres
sure
[hPa
]
0.1
Jan Dec100
necessary magnitude of the trend [K/decade] todetect with a 20-year dataset
seasonally dependent detectability How many years do we need to get a statistically significant
trend ? How small trend can we detect in finite length data with a
statistical significance ?
0.525
T(North Pole)
10
J F M A M J J A S O N D
[hPa]1
10
100
1000
[years]
20
4060
6080
80100
100
100
120
120
120
120
140 140
140
140
140160
160 160180
220
180
stratosphere- 0.5K/decade(MCM; 15,200years)
troposphere+0.05K/decade
(AOGCM; 1,000years)
North Pole
seasonally dependent detectability in the troposphere a natural variability run of AOGCM for 1,000 years necessary data length [years] to detect a linear trend of
+0.05K/decade with 90% statistical significanceNishizawa, Yoden & Nozawa (unpublished)
4. Concluding remarks Advancement in computing powers has enabled us to
do parameter sweep experiments with 3D MCMs
Very long-time integrations give reliable PDFs non-Gaussian, bimodal, ...nonlinear perspectives on climatic variations and trend
Statistics of natural variability are important to assess the detectability of a linear trend should be estimated well by the state-of-the-art GCMs
J F M A M J J A S O N D
[hPa]1
10
100
1000
[years]
20
4060
6080
80100
100
100
120
120
120
120
140 140
140
140
140160
160 160180
220
180
stratosphere- 0.5K/decade(MCM; 15,200years)
troposphere+0.05K/decade
(AOGCM; 1,000years)
North Pole
seasonally dependent detectability in the troposphere a natural variability run of AOGCM for 1,000 years necessary data length [years] to detect a linear trend of
+0.05K/decade with 90% statistical significanceNishizawa, Yoden & Nozawa (unpublished)
Dependence ofmodel-simulated heavy rainfall
on the horizontal resolutionduring the Jakarta flood event
in January-February 2007SOLA, vol.7, p.193-196 (2011)
Shigenori Otsuka, Nurjanna J. Trilaksono,Shigeo Yoden,
Kyoto University, JAPANKazuo Saito, and Shugo Hayashi
MRI-JMA, JAPAN
Heavy rainfall during the Jakarta Flood event in 31 January--2 February, 2007Wu et al. (2007, SOLA)repeated torrential with pronounced two peaks in a day:
midnight (4 - 5 hours) and morning (3 - 4 hours)torrential rains coincided with a strong and persistent
trans-equatorial monsoon flow from the N. Hemisphere
1. Introduction
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Date and Time (Local time)
Rain
fall
(mm
/hr)
Hourly precipitationat Jakarta
Computational domainshorizontal domainDomain 01
∆x = 20 km115 x 103 grids
Domain 02∆x = 4 km
150 x 150 grids
∆x = 5 km120 x 120 grids
Domain 02’∆x = 2 km
250 x 250 grids
vertical dimain0 ≤ z* ≤ 22.1 km
40 levels
Domain 01
Domain 02’(inside)
Domain 02
horizontal map of TBB at 03 LT 1 Feb, 2007for the best member of each resolution
A: Ocean
B: Northern coast
C: Mountain
D: Southern coast
A
B
C
D
2-km model 4-km model MTSAT IR1
5-km model 20-km model
Statistics on rain rateCumulative Distribution Functions (CDFs)
2-km model 4-km model TRMM
5-km model 20-km model