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Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the NAO Mark P. Baldwin

Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

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Page 1: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Mark P. Baldwin, University of Exeter

Imperial College

12 December 2012

Stratospheric Processes:Influence on Storm Tracks and the NAO

Mark P. Baldwin

Page 2: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

(From Baldwin and Dunkerton, Science 2001)

Page 3: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

(From Baldwin and Dunkerton, Science 2001)

60 Days

Page 4: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the
Page 5: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

British Snow Storms

Page 6: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Text

60 days following weak stratospheric winds 60 days following strong stratospheric winds

Observed Average Surface Pressure Anomalies (hPa)

From Baldwin and Dunkerton., 2001

Page 7: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Surface temperature anomalies

4

westerly phases of the QBO, respectively (Fig. 1).The predictability that derives from the ENSO phe-

nomenon is assessed by repeating the analysis that wasperformed for the QBO, but for composites based on

warm versus cold years of the ENSO cycle, as definedby the eight warmest and eight coldest JFM-mean seasurface temperature (SST) anomalies in the equatorialPacific “cold tongue region” (6°S-6°N, 180°W-90°W).

TABLE 2. Frequency of occurrence of extreme cold events (days in which daily minimum temperature drops below 1.5 standard devia-tions below the JFM mean) during the 60-day interval (days +1-60) following the onset of weak and strong vortex conditions at 10-hPaand between Januarys when the QBO is easterly and westerly. The samples are indicated in Fig. 1. Individual results not exceeding the95% confidence level are italicized.

-1.5 std. temperature threshold Total Weak vortex:days +1-60

Strong vortex:days +1-60

QBO:easterly

QBO:westerly

< -17° C in Juneau, Ak. 334 104 66 96 61

< -18° C in Chicago, Il. 411 149 67 115 81

< -6° C in Atlanta, Ga. 416 149 73 90 56

< -10° C in Washington, D. C. 392 153 77 96 66

< -9° C New York, NY. 403 164 99 89 69

< 1° C in London, UK 442 157 77 85 29

< -3° C in Paris, Fr. 446 148 68 98 48

<-9° C in Stockholm, Sw. 348 154 54 56 23

<-9° C in Berlin, Ger. 450 142 77 107 60

< -22° C in St. Petersburg, Ru. 381 137 46 74 46

< -20° C in Moscow, Ru. 472 152 80 90 84

< -29° C in Novosibirsk, Ru. 480 155 69 67 58

< -4° C in Shanghai, China 471 170 84 107 92

< -1° C in Tokyo, Japan 328 130 60 92 58

Days 1-60 followingstratospheric anomalies QBO easterly-westerly ENSO (warm-cold)

FIG 2. The difference in daily mean surface temperature anomalies between the 60-day intervalfollowing the onset of weak and strong vortex conditions at 10-hPa (left panel); between Janu-arys when the QBO is easterly and westerly (middle panel); and between winters (January-March) corresponding to the warm and cold episodes of the ENSO cycle (right panel). Thesamples used in the analysis are documented in Fig. 1. Contour levels are at 0.5 C.From Thompson et al., J. Climate 2002

Page 8: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Text

Observed Average Surface Pressure Anomalies (hPa)

From Baldwin and Dunkerton, 2001

Page 9: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Weather Extremes Related to Stratospheric Variability

• Severe cold weather at high latitudes is more common during weak vortex events.

• Winter weather extremes (low temperatures, snow, etc.) are much more common during weak vortex events.

• Atlantic blocking occurs almost exclusively during weak vortex events.

• Strong winds and ocean wave events are much more common during strong vortex events.

Page 10: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the
Page 11: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Baroclinic eddies!

Vertical shear!

PV inversion!

Barotropic mode!

Wave, mean-flow interaction!

Internal tropospheric dynamics!

Page 12: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

10

Page 13: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

10

• Baldwin and Dunkerton (JGR 1999) suggested that the redistribution of mass in the stratosphere, in response to changes in wave driving, may be sufficient to influence the surface pressure significantly, consistent with the theoretical results of Haynes and Shepherd (1989).

Page 14: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

10

• Baldwin and Dunkerton (JGR 1999) suggested that the redistribution of mass in the stratosphere, in response to changes in wave driving, may be sufficient to influence the surface pressure significantly, consistent with the theoretical results of Haynes and Shepherd (1989).

• Ambaum and Hoskins (JClim 2002) used “PV thinking” to explain how stratospheric PV anomalies affect surface pressure.

Page 15: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Wave Drag

Anomalous wave drag leads to variations in vortex strength

“Wave Driven Pump”

Page 16: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

12

Diagram  from  Ambaum  and  Hoskins  J  Climate  (2002).

15 JULY 2002 1971A M B A U M A N D H O S K I N S

FIG. 3. (a) Dec–Mar climatological mean of tropopause height inmeters. The contour interval is 500 m and the lowest contours overnorthern Canada and Japan represent 8500 m. (b) Regression of tro-popause height with NAO index. The contour interval is 100 m(. . . , ⌃50, 50, 150, . . .). (c) Same as (b) but for the PV500 index.(d) Same as (b) but for the NAOt index.

FIG. 4. Schematic of the bending of isentropic surfaces (labeled⇥0, ⇥1, and ⇥2) toward a positive potential vorticity anomaly. Thearrows represent winds associated with the potential vorticity anom-aly, becoming weaker away from the anomaly.

dient over the Arctic. As expected, the tropopause ishigher over the Azores high associated with the NAO,and is lower over the enhanced Iceland low. However,over the rest of the Arctic the tropopause is generallyhigher.Key to the higher Arctic tropopause with increased

NAO index is the stratosphere. The stratospheric vortexincreases in strength with increasing NAO index. Thelinear correlation between the NAO and PV500 indicesof 0.46 is an indication of this as the PV500 index is agood measure of the strength of the stratospheric vortex.The height of the Arctic tropopause increases with thePV500 index, as shown in Fig. 3c. The NAOt index canbe seen as that part of the NAO index that is not linearlyassociated with increases in the stratospheric vortexstrength. In Fig. 3d we see that the regression of tro-popause height on this index indeed hardly shows thisraised tropopause over the Arctic while the signaturesover the Iceland and Azores regions are retained. Weconclude that the rising of the tropopause with increas-ing NAO index is associated with the stratospheric com-ponent of the NAO.The reason why this occurs is the dominance of the

stratospheric potential vorticity anomaly. As discussedin Hoskins et al. (1985), isentropic surfaces bend towardisolated positive potential vorticity anomalies—see theschematic in Fig. 4. The tropopause at higher latitudescan be associated with a potential vorticity surface. Sim-ilarly, the potential temperature of tropopause parcelswill have to be conserved on changes that are not as-

sociated with diabatic effects at the tropopause. So wemay assume that the potential temperature of the tro-popause is more or less fixed for changes in potentialvorticity in the stratosphere. This then implies that thetropopause will move upward for a positive stratospher-ic potential vorticity anomaly.We can quantify how changes in the height of the

tropopause are associated with potential vorticity anom-alies in the stratosphere: using isentropic coordinatesand hydrostatic balance, the potential vorticity P maybe defined as

f ⇧ ⌥ 1 ⇤pP � , with � � ⌃

� g ⇤⇥

with the usual notation. A change in potential vorticity⌅P will be associated with a change in stratification of⌅� and a change in absolute vorticity of ⌅⌥. Accordingto quasigeostrophic scaling, the relative magnitude ofthe stratification and vorticity contributions is measuredby the Burger number Bu � (NH/ fL)2. Logarithmicderivatives of the potential vorticity now give

⌅P ⌅�� ⌃(1 ⇧ Bu) .

P �

Unless alternative scales are imposed geometrically,geostrophic adjustment will tend to make the Burgernumber close to unity for any potential vorticity anom-aly, that is, it will tend to make the horizontal lengthscale L close to the Rossby deformation radius asso-ciated with the height scale H. We now consider thepressure difference between an isentropic surface abovethe potential vorticity anomaly (⇥top) and the isentropicsurface that touches the Arctic tropopause (⇥tpp). Finitedifference approximations for � and ⌅� in the strato-sphere now are

1 p ⌃ p 1 ⌅p ⌃ ⌅ptop tpp top tpp� � ⌃ , ⌅� � ⌃ ,g ⇥ ⌃ ⇥ g ⇥ ⌃ ⇥top tpp top tpp

Page 17: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

13

Polar  cap  “PV600K  Index”  ~20-­‐25  hPa

Correlation between JFM PV 600K Index and Zonal-Mean PV Anomalies, JFM

20 30 40 50 60 70 80 90Latitude

300

400

500

600

700

800

Pote

ntia

l Tem

pera

ture

-0.6

5

-0.5

5

-0.55

-0.4

5

-0.45

-0.3

5

-0.35-0.35

-0.2

5

-0.25

-0.2

5

-0.1

5

-0.15

-0.15

-0.15-0.05

-0.05

-0.05

-0.0

5

-0.05

-0.05

-0.05

0.05

0.05

0.05

0.05

0.05

0.15

0.15

0.15

0.25

0.25

0.35

0.35

0.45

0.45

0.55

0.55

0.55

0.65

0.65

0.75

0.75

0.85

0.95

Create  an  index  of  vortex  strength  as  defined  by  PV  at  600K  (20-­‐25  hPa).

Page 18: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

14

Composite of 24 negative events: PV at 600K

-120 -80 -40 0 40 80 120Lag (Days)

20

30

40

50

60

70

80

90

Latit

ude

Composite of 23 positive events: PV at 600K

-120 -80 -40 0 40 80 120Lag (Days)

20

30

40

50

60

70

80

90

Latit

ude

Page 19: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

15

Composite of 24 negative events: PV at Equivalent Lat 70N

-120 -80 -40 0 40 80 120Lag (Days)

Pote

ntia

l Tem

pera

ture

265 300 350 395430475530

600

700

850

Composite of 23 positive events: PV at Equivalent Lat 70N

-120 -80 -40 0 40 80 120Lag (Days)

Po

tent

ial T

empe

ratu

re

265 300 350 395430475530

600

700

850

From Baldwin and Birner, in prep.

Page 20: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

15

Composite of 24 negative events: PV at Equivalent Lat 70N

-120 -80 -40 0 40 80 120Lag (Days)

Pote

ntia

l Tem

pera

ture

265 300 350 395430475530

600

700

850

Composite of 23 positive events: PV at Equivalent Lat 70N

-120 -80 -40 0 40 80 120Lag (Days)

Po

tent

ial T

empe

ratu

re

265 300 350 395430475530

600

700

850

Weak Vortex Event

Strong Vortex Event

From Baldwin and Birner, in prep.

Page 21: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

16

Diagram  from  Ambaum  and  Hoskins  J  Climate  (2002).

15 JULY 2002 1971A M B A U M A N D H O S K I N S

FIG. 3. (a) Dec–Mar climatological mean of tropopause height inmeters. The contour interval is 500 m and the lowest contours overnorthern Canada and Japan represent 8500 m. (b) Regression of tro-popause height with NAO index. The contour interval is 100 m(. . . , ⌃50, 50, 150, . . .). (c) Same as (b) but for the PV500 index.(d) Same as (b) but for the NAOt index.

FIG. 4. Schematic of the bending of isentropic surfaces (labeled⇥0, ⇥1, and ⇥2) toward a positive potential vorticity anomaly. Thearrows represent winds associated with the potential vorticity anom-aly, becoming weaker away from the anomaly.

dient over the Arctic. As expected, the tropopause ishigher over the Azores high associated with the NAO,and is lower over the enhanced Iceland low. However,over the rest of the Arctic the tropopause is generallyhigher.Key to the higher Arctic tropopause with increased

NAO index is the stratosphere. The stratospheric vortexincreases in strength with increasing NAO index. Thelinear correlation between the NAO and PV500 indicesof 0.46 is an indication of this as the PV500 index is agood measure of the strength of the stratospheric vortex.The height of the Arctic tropopause increases with thePV500 index, as shown in Fig. 3c. The NAOt index canbe seen as that part of the NAO index that is not linearlyassociated with increases in the stratospheric vortexstrength. In Fig. 3d we see that the regression of tro-popause height on this index indeed hardly shows thisraised tropopause over the Arctic while the signaturesover the Iceland and Azores regions are retained. Weconclude that the rising of the tropopause with increas-ing NAO index is associated with the stratospheric com-ponent of the NAO.The reason why this occurs is the dominance of the

stratospheric potential vorticity anomaly. As discussedin Hoskins et al. (1985), isentropic surfaces bend towardisolated positive potential vorticity anomalies—see theschematic in Fig. 4. The tropopause at higher latitudescan be associated with a potential vorticity surface. Sim-ilarly, the potential temperature of tropopause parcelswill have to be conserved on changes that are not as-

sociated with diabatic effects at the tropopause. So wemay assume that the potential temperature of the tro-popause is more or less fixed for changes in potentialvorticity in the stratosphere. This then implies that thetropopause will move upward for a positive stratospher-ic potential vorticity anomaly.We can quantify how changes in the height of the

tropopause are associated with potential vorticity anom-alies in the stratosphere: using isentropic coordinatesand hydrostatic balance, the potential vorticity P maybe defined as

f ⇧ ⌥ 1 ⇤pP � , with � � ⌃

� g ⇤⇥

with the usual notation. A change in potential vorticity⌅P will be associated with a change in stratification of⌅� and a change in absolute vorticity of ⌅⌥. Accordingto quasigeostrophic scaling, the relative magnitude ofthe stratification and vorticity contributions is measuredby the Burger number Bu � (NH/ fL)2. Logarithmicderivatives of the potential vorticity now give

⌅P ⌅�� ⌃(1 ⇧ Bu) .

P �

Unless alternative scales are imposed geometrically,geostrophic adjustment will tend to make the Burgernumber close to unity for any potential vorticity anom-aly, that is, it will tend to make the horizontal lengthscale L close to the Rossby deformation radius asso-ciated with the height scale H. We now consider thepressure difference between an isentropic surface abovethe potential vorticity anomaly (⇥top) and the isentropicsurface that touches the Arctic tropopause (⇥tpp). Finitedifference approximations for � and ⌅� in the strato-sphere now are

1 p ⌃ p 1 ⌅p ⌃ ⌅ptop tpp top tpp� � ⌃ , ⌅� � ⌃ ,g ⇥ ⌃ ⇥ g ⇥ ⌃ ⇥top tpp top tpp

Page 22: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Composite Anomalous Pressure, 33 Weak Vortex events

-90 -60 -30 0 30 60 90Lag (days)

Pr

essu

re A

nom

aly,

7 h

Pa b

etw

een

ticks

PV index at 600K

330K

320K

315K

310K

305K

17

Page 23: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

18

Correlation: JFM Polar Cap PV600K Index with Tbar

-90 -70 -50 -30 -10 10 30 50 70 90Latitude

1000

700

500

300

200

100

70

50

30

20

10

hPa

-0.8

-0.8

-0.6

-0.6

-0.4

-0.4

-0.2

-0.2

-0.2

0.0 0.0

0.0

0.0

0.0

0.0

0.0

0.00.0 0.2

0.2

0.2

0.2

0.4

0.4

0.4

+ PV anom.

- PV anom.

600K surface

CorrelaAon  during  winter  (JFM)  between  the  600K  PV  index  and  zonal-­‐mean  temperature.    The  JFM  daily  correlaAon  between  PV530  and  polar  cap  tropopause  T  anomalies  is  0.90.  

From Baldwin and Birner, in prep.

Page 24: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

Page 25: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

Page 26: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

Page 27: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

• The larger the slope, the larger the potential for baroclinic disturbances to gain kinetic energy by baroclinic conversion.

Page 28: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

• The larger the slope, the larger the potential for baroclinic disturbances to gain kinetic energy by baroclinic conversion.

Page 29: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

• The larger the slope, the larger the potential for baroclinic disturbances to gain kinetic energy by baroclinic conversion.

• Stratospheric PV variations affect directly the slope of isentropic surfaces near and below the tropopause.

Page 30: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

19

Effects on baroclinic eddies

• Papritz and Spengler (2015, QJ) proposed using the slope of isentropic surfaces as a measure for baroclinicity.

• The larger the slope, the larger the potential for baroclinic disturbances to gain kinetic energy by baroclinic conversion.

• Stratospheric PV variations affect directly the slope of isentropic surfaces near and below the tropopause.

Page 31: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

20

Correlation: JFM Polar Cap PV600K Index with Tbar

-90 -70 -50 -30 -10 10 30 50 70 90Latitude

1000

700

500

300

200

100

70

50

30

20

10

hPa

-0.8

-0.8

-0.6

-0.6

-0.4

-0.4

-0.2

-0.2

-0.2

0.0 0.0

0.0

0.0

0.0

0.0

0.0

0.00.0 0.2

0.2

0.2

0.2

0.4

0.4

0.4

+ PV anom.

- PV anom.

600K surface

CorrelaAon  during  winter  (JFM)  between  the  600K  PV  index  and  zonal-­‐mean  temperature.    The  JFM  daily  correlaAon  between  PV530  and  polar  cap  tropopause  T  anomalies  is  0.90.  

NAO+

From Baldwin and Birner, in prep.

Page 32: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

21

Correlation: JFM Polar Cap PV600K Index with Tbar

-90 -70 -50 -30 -10 10 30 50 70 90Latitude

1000

700

500

300

200

100

70

50

30

20

10

hPa

-0.8

-0.8

-0.6

-0.6

-0.4

-0.4

-0.2

-0.2

-0.2

0.0 0.0

0.0

0.0

0.0

0.0

0.0

0.00.0 0.2

0.2

0.2

0.2

0.4

0.4

0.4

+ PV anom.

- PV anom.

600K surface

CorrelaAon  during  winter  (JFM)  between  the  600K  PV  index  and  zonal-­‐mean  temperature.    The  JFM  daily  correlaAon  between  PV530  and  polar  cap  tropopause  T  anomalies  is  0.90.  

From Baldwin and Birner, in prep.

NAO–

Page 33: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

22

CorrelaAon  during  winter  (JFM)  between  the  600K  PV  index  and  zonal-­‐mean  temperature.    The  JFM  daily  correlaAon  between  PV530  and  polar  cap  tropopause  T  anomalies  is  0.90.  

NAO–

Anomalous Baroclinicity (slope of isentropic surfaces)

Page 34: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Text

Observed Average Surface Pressure Anomalies (hPa)

From Baldwin and Dunkerton., 2001

Page 35: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Text

60 days following weak stratospheric winds 60 days following strong stratospheric winds

Observed Average Surface Pressure Anomalies (hPa)

From Baldwin and Dunkerton., 2001

Page 36: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Weak Vortex Regimes

-1

-10

0

0

2

4

a

Strong Vortex Regimes

-1

0

00

0

2

b

Text

60 days following weak stratospheric winds

Observed Average Surface Pressure Anomalies (hPa)

From Baldwin and Dunkerton., 2001

Page 37: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

26

Changing  the  depth  of  the  troposphere  affects  1)  vorAcity  in  the  column,  and  2)  surface  pressure.  modest  tropospheric  effect?

Movement  of  mass  by  the  wave-­‐driven  pump

wave-­‐driven  pump

Page 38: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

27

ERA-­‐40  observaAons

Regression  between  PV600K  index  and  Polar  Cap  p’

DiagnosAc  for  observaAons  or  models

Page 39: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

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ERA-­‐40  observaAons

Regression  between  PV600K  index  and  Polar  Cap  p’

Tropospheric  amplificaAon

DiagnosAc  for  observaAons  or  models

Page 40: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

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Summary

Page 41: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

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Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

Page 42: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

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Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

Page 43: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

28

Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

• Consistent with PV theory, vertical motion in the UTLS displaces isentropic surfaces (and the tropopause) in a north-south dipole. This changes the slopes of isentropic surfaces in the UTLS—which should affect eddy growth rates, and enhance N-S movement of mass—reinforcing the NAO signal.

Page 44: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

28

Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

• Consistent with PV theory, vertical motion in the UTLS displaces isentropic surfaces (and the tropopause) in a north-south dipole. This changes the slopes of isentropic surfaces in the UTLS—which should affect eddy growth rates, and enhance N-S movement of mass—reinforcing the NAO signal.

• The NAO signal from the stratosphere is self reinforcing, through modifying baroclinic eddies. Eddy processes amplify the stratospheric signal.

Page 45: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

28

Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

• Consistent with PV theory, vertical motion in the UTLS displaces isentropic surfaces (and the tropopause) in a north-south dipole. This changes the slopes of isentropic surfaces in the UTLS—which should affect eddy growth rates, and enhance N-S movement of mass—reinforcing the NAO signal.

• The NAO signal from the stratosphere is self reinforcing, through modifying baroclinic eddies. Eddy processes amplify the stratospheric signal.

• A simple polar cap pressure diagnostic can be used to evaluate the fidelity of S–T coupling in models.

Page 46: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

28

Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

• Consistent with PV theory, vertical motion in the UTLS displaces isentropic surfaces (and the tropopause) in a north-south dipole. This changes the slopes of isentropic surfaces in the UTLS—which should affect eddy growth rates, and enhance N-S movement of mass—reinforcing the NAO signal.

• The NAO signal from the stratosphere is self reinforcing, through modifying baroclinic eddies. Eddy processes amplify the stratospheric signal.

• A simple polar cap pressure diagnostic can be used to evaluate the fidelity of S–T coupling in models.

Page 47: Stratospheric Processes: Influence on Storm …...Mark P. Baldwin, University of Exeter Imperial College 12 December 2012 Stratospheric Processes: Influence on Storm Tracks and the

28

Summary • The stratospheric “wave-driven pump” creates PV

anomalies corresponding to weak and strong vortex conditions. Equivalently, it moves mass into and out of the polar cap. This is the annular mode pattern.

• Both PV theory and mass movement explain 1) why the surface pattern looks like the NAO, and why the NAO is the preferred response to stratospheric forcing.

• Consistent with PV theory, vertical motion in the UTLS displaces isentropic surfaces (and the tropopause) in a north-south dipole. This changes the slopes of isentropic surfaces in the UTLS—which should affect eddy growth rates, and enhance N-S movement of mass—reinforcing the NAO signal.

• The NAO signal from the stratosphere is self reinforcing, through modifying baroclinic eddies. Eddy processes amplify the stratospheric signal.

• A simple polar cap pressure diagnostic can be used to evaluate the fidelity of S–T coupling in models.