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Page 1: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2005 Miami

Active Radars

Page 2: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

From Neil Tyson’s address/campaignOn the Future of NASA Univ. Wash. Jan 20, 2005

“LEO (low earth orbits) are old hat and boring. NASA must do new stuff – space”

President’s commission --- “Vision” (thing)

Winners: Space Exploration Planetary Science Astrobiology Astrophysics Astronomy

Losers: Beyond Einstein missions Earth Science

Page 3: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Page 4: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Winds --- see elsewhere

Page 5: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Toward a Surface Pressure Model Function• A Scatterometer doesn’t measure Winds. It measures

Capillaries & Short Gravity Waves, related to zo., u*

• Fortunately, there exists a relation U10/u* = F(z, zo, stratification…).– Established over land, assumed over the ocean .– Verified in the 26 years since Seasat.

There’s an easy extrapolation to: • Fortunately, there exists a relation UG/u* = F(z, zo, stratification, , ……).

– Established in UW PBL_LIB. is a constant, a similarity parameter.

– Verified in the last 10 years of satellite dataR. A. Brown 2004 EGU 2005 Miami

Page 6: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Try a direct correlation with pressureSince VG = P / ( f ) Use ECMWF/NCEP surface pressures analyses get P and VG ; substitute VG for U10 in the Model Function i.e. We’re using the model surface pressures as truth rather than the PBL analysis of U10

Results: VG correlates with o as well as U10

* Better alias selection with scatterometer data alone * High winds appear * Low winds, directions appear * Stratification, Thermal Wind Effects

Prospects:

R. A. Brown EGU 2004

Page 7: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Example of o vs look angle for U10 = 20m/s; Incidence = 45

Example of o vs look angle for VG = 27m/s; Incidence = 45

R. A. Brown 2004 EGU

Page 8: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Page 9: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Producing smooth wind fields

R. A. Brown 2003 U. ConcepciÓn

Usually from rain Direction information is poor

Page 10: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Raw scatterometer windsUWPressure field smoothed

JPL Project Local GCM nudge smoothed = Dirth

(JPL)

R. A. Brown 2003 PORSEC, U. ConcepciÓn

Page 11: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

• QuikSCAT pressure gradients are comparable to ECMWF in general– QuickSCAT implies stronger

gradients in frontal zones.

• Comparison with ECMWF similar in both hemispheres

• Good correlation overall• We’ve grown accustomed to

this level of quality in QS-SLP

QuikSCAT

Foster, 2005

Page 12: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Dashed:ECMWF R. A. Brown 2005

Swath QuikScat surface pressure fields available at http://PBL.atmos.

washington.edu

Page 13: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

ECMWF analysis

QuikScat analysis

Surface Pressures

J. Patoux & R. A. Brown 2003 PORSEC, U. ConcepciÓn; 2005 Miami

Page 14: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Agreement between satellite and ECMWF pressure fields indicate that both Scat winds and the nonlinear PBL model (VG/U10) are accurate within 2 m/s.

Results from Satellite Scatterometer surface pressure analyses:

3-month, zonally averaged offset angle <VG, U10> of 19° suggests the mean PBL state is near neutral. This is the nonlinear PBL predicted angle (18°).

Swath deviation angle observations show thermal wind and stratification effects, implying temperatures.

VG rather than U10 could be used to initialize GCMs

Predicted higher winds from pressure gradients (than from GCM or buoys) agree with OLE effect, observations.

R. A. Brown 2004 EGU

• SLP gradients (e.g. from buoys) provide surface truth for VG, hence U10.

Page 15: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Page 16: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Storms & Fronts Analyses

Page 17: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

In the second case, the system is decaying but a secondary low is developing behind the remnants of the cold front. Note also the correspondence between convergence and clouds.

Fronts: Location; Analysis; Frontogenesis; Prognosticators

R. A. Brown, J. Patoux003

Page 18: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Analysis of QuikScat derived fronts and pressure fields

suggests there are correlations between frontal characteristics, upper level conditions (PV) and

subsequent development of explosive storms development

Patoux, J., PhD thesis Univ. of Washington, 2003. MWR in press

Page 19: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Page 20: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Southern Hemisphere Pressures

ECMWF & NSCAT Comparison

• Surface Pressure Fields of 102 Storms surveyed for 1996:

* 5% missed entirely (vs 20% in 1990)* 70% misplaced average an 280 km* 25% good matches (-3 mb ave. diff.)

R. A. Brown 2003 PORSEC, U. ConcepciÓn; 2005 Miami

Page 21: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Revelations from scatterometers • Great global surface pressure fields are available daily.• The winds are higher; the low pressures are lower &

more frequent; heat fluxes are greater; and surface stress is much greater than climatology states.

• Data on storms and fronts is exceptional. (Patoux, J., G.J. Hakim and R.A. Brown, 2004: Diagnosis of frontal instabilities over the Southern Ocean, Monthly Weather Review, in press)• Storms frequency, strength and statistics are different• Fronts (defined as wind convergence zones) are ubiquitous,

persistent and provide new data

Page 22: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old
Page 23: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

The global marine wind and pressure data from scatterometers (the 19 deg turning) and SARs (OLE surface imprints) indicate that the nonlinear OLE (Rolls) are present 50 – 70% of the time.

Hence the nonlinear PLB model prevails (the Ekman solution does not exist). While this is a nonlinear finite perturbation, it can have large effects on measurements 10-km or less and in the mean.

Air-Sea fluxes are non-homogeneous, take place in advective plumes, and interact with the inversion. New PBL models are needed to get good heat and momentum fluxes for ocean and climate modeling.

K-theory (diffusion modelling) is physically incorrect for modeling these fluxes.

Winds are higher than climate and ocean modelers thought.

Page 24: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

• In addition to better initialization of GCMs;• Global marine surface winds and pressures are

best available• Storms and fronts analyses are revolutionary.

– Provides surface truth for storms– Provides statistics for storms– Possibility of predictors of storms genesis.

• Winds and fluxes are different than climatology records. Climate and ocean dynamics modelers take note.

Page 25: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old
Page 26: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old
Page 27: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old
Page 28: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

The Contributions of Scatterometry• The microwave scatterometers have now provided over two decades of

inferred surface winds over the oceans. These data have been extensively studied and compared to in situ measurements so that they comprise a ‘surface truth’ base comparable to other sources of winds. In fact, in many cases these products are revolutionary, changing the way we view the world. Examples are:

Mainline products

• The surface winds are exceptional in resolution and coverage.• The nonlinear solution applied to satellite surface winds provides sufficient

accuracy to determine surface pressure fields from satellite data alone. We can uniquely offer a continuous record of QS-derived surface pressure fields: these pressure fields extend through the Tropics - a region that is poorly characterized by numerical weather forecast models - and contain fine details that are absent from numerical model analyses

• The pressure fields can be used as a low pass filter to aid ambiguity selection and provide smooth wind fields from scatterometer data alone.

Page 29: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

From the Scatterometers (2)Storms and Weather Revelations• The scatterometer data allow study of the development of fronts in general

and frontal waves in particular: QS reveals mesoscale features that are not captured by numerical models or other satellite-borne instruments, in particular the surface signature of frontal instabilities that sometimes develop into secondary cyclones. (Patoux, J., G.J. Hakim and R.A. Brown, Diagnosis of frontal instabilities over the Southern Ocean, Monthly Weather Review, in press).

• These data allow us to build a climatology of primary and secondary cyclones (in particular their kinematics as revealed by scatterometer winds), to test the hypothesis that explosive frontal storm development may have surface predictors (e.g. surface PV anomaly coincident with upper-level vorticity) and to investigate the possibility that the strength of storms and fronts is increasing due to global warming

• Capturing storm and frontal dynamics require at least 25-km resolution. New revelations are stimulating and surely forthcoming from QuikScat data. (Brown, R.A., Comments on the synergism between the analytic PBL model and remote sensing data, Bound.-Layer Meteor., in press)

Page 30: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

From the scatterometers (3)Basic Revelations• The numerical global models of the 90s were inadequate in representing

Southern Hemisphere and tropical weather systems. In 1991, they missed 20% of the So. Hemisphere storms. After the scatterometer revelations, the numerical models improved resolution and incorporated satellite data so they now (2004) miss only 5% of the storms (tho miss-locating 70% by an average 250km). QuikScat data forms the basis of this evaluation.

• The data indicate that the global climatology surface wind record is too low by 10 – 20%.

Basic Science• There is evidence from these data that the secondary flow characteristics

of the nonlinear PBL solution (Rolls or Coherent Structures) are present more often than not over the world’s oceans. This contributes to basic understanding of air-sea fluxes.

• The revealed dynamics of the typical PBL indicate that K-theory models are physically incorrect. This will mean revision of all GCM PBL models. QuikScat data will help convince them.

• The conclusions from these observations are important yet often ignored by the modeling community. The continued accumulation of data from QuikScat is essential to wake up the community.

Page 31: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

SLP from Surface Winds• UW PBL similarity model

• Use “inverse” PBL model to estimate from satellite

• Use Least-Square optimization to find best fit SLP to swaths

• Extensive verification from ERS-1/2, NSCAT, QuikSCAT

10 10( , , , , , )G f P T SST q CSu

1010logN

o

uUk z u

10NU

P (UGN )

(UGN )

R. A. Brown 2005

Page 32: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Using SLP to Assess Direction

• Winds derived from SLP are optimal smooth winds

• Arbitrary threshold of 35o from Model U10

used to distinguish potentially wrong ambiguity choice

• Look for an ambiguity with closer direction to Model winds in these cases

R. A. Brown 2005

Page 33: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Station B

2 - 5 km

Taking measurements in the Rolls

Station A

1-km

RABrown 2004

U

V Mean Flow Hodograph

Z/ 1

2

3

The Mean Wind

The OLE winds

Hodographfrom center zone

Hodographfrom convergent zone

Page 34: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Station B

2 - 5 km

Taking measurements in the Rolls

Station A

1-km

RABrown 2004

U

V Mean Flow Hodograph

Z/ 1

2

3

The Mean Wind

The OLE winds

Hodographfrom center zone

Hodographfrom convergent zone

Page 35: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

The gradient wind correction is described in Patoux and Brown (2002) and uses the simple balance of forces in natural coordinates shown in the figure

The Gradient Wind Correction

R. A. Brown 2003 U. ConcepciÓn

Page 36: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

R. A. Brown 2004 EGU

Geostrophic balance Gradient balance

Page 37: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

On the right, the gradient wind correction has been included. The obtained pressure field is very similar to the uncorrected one, except for the center of the anticyclone, where the radius of curvature is smaller, and the effect of the correction bigger. The pressure gradients are weaker and the central area of the high is flatter, which seems in better agreement with ECMWF.

R. A. Brown 2003 U. ConcepciÓn

Page 38: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Best surface winds, pressures availableMuch Better Storms Depiction

Shows Evolution of Fronts & Cyclones

Better Hurricane PBLs, GCM Initializations, forecasts

Proof of Rolls (OLE) Ubiquity (PBL model) Higher Winds (heat

fluxes) for Climate models

R. A. Brown 2005

Page 39: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

* Great global surface marine winds are available daily.

Revelations from scatterometers * Great global surface pressure fields are available daily. * Ship or Buoy winds are not good surface truth in general. * GCM PBL models have the wrong physics.* The oV saturates (due to white water) @ U10 ~ 35 m/s, but the oH does not saturate even at U10 ~ 65 m/s.* The winds are higher, the low pressures are lower & more frequent, heat fluxes are greater and stress much greater than climatology states. Climate modelers take note. * Scatterometer derived pressure fields can be used to de-alias winds and correct (smooth) o single or small area anomalies (rain or nadir/edge ambiguities).* Data on storms and fronts is revolutionary. (Patoux, J., G.J. Hakim and R.A. Brown, 2004: Diagnosis of frontal instabilities over the Southern Ocean, Monthly Weather Review, in press)

Page 40: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

1. The winds are non-homogeneous at the surface over a 0.1-5 km horizontal distance. Upper high velocity wind is advected to the surface in lines. OLE must be taken into account in surface truth measurements (In the average and point values). (Brown, Canadian Jn. Remote Sensing, 28, 340-345, 2002)

R. A. Brown 2005

2. The average wind profile is different from the Ekman solution –and from a profile 100m away – the nonlinear wind solution (and hence fluxes of momentum, heat, CO2 etc.) is 10-50% different, depending on stratification and thermal wind. In a satellite’s 25-km footprint there will be 10-OLE so the periodic effect will be the average. Not true at 6-km or less --- the SAR resolution. (Brown & Foster, The Global Atmos.-Ocean System, 2, 163-183, 1994; 185-198, 1994; 199-219, 1994.)

3. The PBL contains advecting flow not amenable to diffusion modeling. Numerical models cannot portray correct physics of mean flow without extreme increase in resolution.

Page 41: R. A. Brown 2005 Miami Active Radars. From Neil Tyson’s address/campaign On the Future of NASA Univ. Wash. Jan 20, 2005 “LEO (low earth orbits) are old

Dashed:ECMWF