Benefits from Advances in the Data Assimilation Earth Observations from Space · 2016. 12. 12. ·...

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Benefits from Advances in the Data Assimilation Benefits from Advances in the Data Assimilation Benefits from Advances in the Data Assimilation Benefits from Advances in the Data Assimilation of of of of Earth Observations from Space Earth Observations from Space Earth Observations from Space Earth Observations from Space John Le Marshall John Le Marshall John Le Marshall John Le Marshall 1 1 1 , Robert Norman , Robert Norman , Robert Norman , Robert Norman 2 2 2 , Yi Xiao , Yi Xiao , Yi Xiao , Yi Xiao 1 1 1 , Chris Tingwell , Chris Tingwell , Chris Tingwell , Chris Tingwell 1 1 1 , Kefei Zhang , Kefei Zhang , Kefei Zhang , Kefei Zhang 2 2 2 , Paul Lehmann , Paul Lehmann , Paul Lehmann , Paul Lehmann 1 1 1 , , , , David Howard David Howard David Howard David Howard 1 1 1 , Tim Morrow , Tim Morrow , Tim Morrow , Tim Morrow 1 1 1 , Jim Jung , Jim Jung , Jim Jung , Jim Jung 3 3 3 , Jaime Daniels , Jaime Daniels , Jaime Daniels , Jaime Daniels 4 4 4 and Steve Wanzon g and Steve Wanzon g and Steve Wanzon g and Steve Wanzon g 3 3 3 ……. ……. ……. ……. 1 1 1 Bureau of Meteorology, Melbourne, Australia Bureau of Meteorology, Melbourne, Australia Bureau of Meteorology, Melbourne, Australia Bureau of Meteorology, Melbourne, Australia 2 2 2 RMIT University, Melbourne, Australia RMIT University, Melbourne, Australia RMIT University, Melbourne, Australia RMIT University, Melbourne, Australia 3 3 3 UW/CIMSS, Madison,USA UW/CIMSS, Madison,USA UW/CIMSS, Madison,USA UW/CIMSS, Madison,USA 4 NOAA/NESDIS/STAR, College Park, USA NOAA/NESDIS/STAR, College Park, USA NOAA/NESDIS/STAR, College Park, USA NOAA/NESDIS/STAR, College Park, USA

Transcript of Benefits from Advances in the Data Assimilation Earth Observations from Space · 2016. 12. 12. ·...

Page 1: Benefits from Advances in the Data Assimilation Earth Observations from Space · 2016. 12. 12. · Earth observations From Space Fig. 8(c). SH 500hPa height anomaly correlation for

Benefits from Advances in the Data AssimilationBenefits from Advances in the Data AssimilationBenefits from Advances in the Data AssimilationBenefits from Advances in the Data Assimilation

of of of of

Earth Observations from Space Earth Observations from Space Earth Observations from Space Earth Observations from Space

John Le MarshallJohn Le MarshallJohn Le MarshallJohn Le Marshall1111, Robert Norman, Robert Norman, Robert Norman, Robert Norman2222, Yi Xiao, Yi Xiao, Yi Xiao, Yi Xiao1111, Chris Tingwell, Chris Tingwell, Chris Tingwell, Chris Tingwell1111, Kefei Zhang, Kefei Zhang, Kefei Zhang, Kefei Zhang2222, Paul Lehmann, Paul Lehmann, Paul Lehmann, Paul Lehmann1111, , , ,

David HowardDavid HowardDavid HowardDavid Howard1111, Tim Morrow, Tim Morrow, Tim Morrow, Tim Morrow1111, Jim Jung, Jim Jung, Jim Jung, Jim Jung3333, Jaime Daniels, Jaime Daniels, Jaime Daniels, Jaime Daniels4444 and Steve Wanzon gand Steve Wanzon gand Steve Wanzon gand Steve Wanzon g3333 …….…….…….…….

1111 Bureau of Meteorology, Melbourne, AustraliaBureau of Meteorology, Melbourne, AustraliaBureau of Meteorology, Melbourne, AustraliaBureau of Meteorology, Melbourne, Australia

2222 RMIT University, Melbourne, AustraliaRMIT University, Melbourne, AustraliaRMIT University, Melbourne, AustraliaRMIT University, Melbourne, Australia

3333 UW/CIMSS, Madison,USAUW/CIMSS, Madison,USAUW/CIMSS, Madison,USAUW/CIMSS, Madison,USA4 NOAA/NESDIS/STAR, College Park, USANOAA/NESDIS/STAR, College Park, USANOAA/NESDIS/STAR, College Park, USANOAA/NESDIS/STAR, College Park, USA

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Overview

• The Importance of EOS (in the SH)

• Recent and Impending Benefits

• The Advanced Sounders

• Atmospheric Motion Vectors - Himawari – 6,7,8

• Radio Occultation

• Future Prospects

• Summary

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Observing System Experiments (OSEs)

With and Without Satellite Data

• Systems Examined

– ACCESS (APS1) – Operational data base (Australian Op. Sys)

– 28 October to 30 November 2011

– GFS (2010) - Operational data base (US Op. Sys)

– 15 August to 30 September 2010

The Importance of EOS ( in the SH)

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There are currently 31 data-stream/distinct instrument-type products, Radiances

HIRS (multi-platform)AMSUA (multi-platform)AMSUB/MHS (multi-platform)IASI (multi-platform)AIRSCrISATMS

GPS-RO (multi-platform)AVHRR (via SST analysis)AATSR (via SST analysis)AMSR-E (via SST analysis)

Wind products (sfc or AMV)

ASCAT (multi-platform)Himawari-8 IRHimawari-8 VISHimawari-8 cloudy WV 6.7Meteosat-10 IRMeteosat-10 cloudy WV 7.3Meteosat-10 VISMeteosat-10 HRVISMeteosat-7 IRMeteosat-7 VISMeteosat-7 cloudy WVGOES-15 IRGOES-15 cloudy WVGOES-13 IRGOES-13 cloudy WVTerra/Aqua IRAqua cloudy WVAqua clear sky WVNOAA-15/NOAA-18/NOAA-19 IRMetOp-A/MetOp-B IR

Within 3 years there will be 11 more:

Radiances

Himawari-8 Clear sky radiancesSEVERI Clear sky radiancesSEVERI All sky radiancesSAPHIRMWTS-2MWHS-2SSMIS (multi-platform)

GPS ZTD

Winds

RapidScatADM-Aeolus/ALADINLeoGeo IR AMVs (multi-platform)VIIRSWindsat

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0.6

0.65

0.7

0.75

0.8

0.85

0.9

0.95

1

0 24 48 72 96 120 144HOURS

SAT

NOSAT

AC

A high quality (AC=0.9) 24 hour (1 day) forecast without using satellite datais of the same quality as a 96 hour (4 days) forecast using satellite data.

ACCESS FORECAST SKILL (AC) VERSUS TIME SH 500hPa HGT 26 October - 31 November 2011

These curves show

how forecast accuracy

degrades with time.

From Le Marshall et al. 2013. The considerable impact of earth observations from space on numerical weather prediction. JSHESS

The Importance of EOS in the Southern hemisphere

In the SH EOS extend the length of a high quality numerical forecast by a factor of four

In the northern hemisphere EOS extend the length of a high quality forecast by a factor of 1.6

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Earth observations From Space

Fig. 8(c). SH 500hPa height anomaly correlation for the

control (SAT) and no satellite (NOSAT), 28 October to 30

November 2011 using ACCESS and verifying against the

control analysis

Fig. 8(f). NH 500hPa height anomaly correlation for the

control (SAT) and no satellite (NOSAT), 28 October to 30

November 2011 using ACCESS and verifying against the

control analysis

0.6

0.65

0.7

0.75

0.8

0.85

0.9

0.95

1

0 24 48 72 96 120 144HOURS

AC: 500hPa HGT 20111026-20111131

SAT

NOSAT

AC

0.8

0.82

0.84

0.86

0.88

0.9

0.92

0.94

0.96

0.98

1

0 24 48 72 96 120 144HOURS

AC

NOSAT

SAT

AC: 500hPa HGT 20111026-20111131

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Earth observations From Space

Fig. 8(g). SH 500hPa height anomaly correlation for the

control (SAT) and no satellite (NOSAT), 15 August to 30

September 2010 using GFS and verifying against the

control analysis

Fig. 8(hNH 500hPa height anomaly correlation for the

control (SAT) and no satellite (NOSAT), 15 August to 30

September 2010 using the GFS and verifying against the

control analysis

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ACCESS-G 48 to 72 hour rainfall forecast for 9 November 2011 using satellite data.

ACCESS-G 48 to 72 hour rainfall forecast for 9 November 2011 using no satellite data.

Daily rain gauge analysis for 9 November 2011.

Daily rainfall values.

Hi Impact Weather

9 November 2011 NOSAT SAT

Correlation between observed

and forecast rainfall (Aust.

Region)

0.282 0.699

Hanssen and Kuipers (Aust.

Region)

0.360 0.596

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Table 1. ACCESS-G verification statistics for all of Australia for

the month of November 2011 for forecasts produced with (SAT)

and without (NOSAT) satellite data

1 – 30 November 2011 ( 72-96 hrs) NOSAT SAT

Correlation between observed and forecast

rainfall (Full Aust. Region)

0.25 0.41

Hanssen and Kuipers (Full Aust. Region) 0.36 0.51

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Atlantic basin mean hurricane track errors for the control (all data) and no satellite data case, 15 August to 30 September 2010 using GFS and verifying against the control (all data) analysis.

Atlantic Basin Hurricane Track

Mean Errors

0

50

100

150

200

250

300

0 12 24 36 48 72 96 120

54 50 39 35 29 20 16 13

Forecast Time [hours]

Storm Counts

Tra

ck E

rro

r [N

M]

Control

No_satell ite

Hi Impact Weather

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CURRENT

2016

ConventionalData

Surface: synops, ships, buoysSondes, extra wind profilersAircraft: AIREPS, AMDARS

EOS Satellite observations (26 inst.)Wind: Scatterometer surface winds (ASCAT (2)), AMVs from GEOS(H, GE,GW,MS,M8,IN) & POES(MA,MB,A,T, N(3))GNSS-RO: (C(6), G,M) bending angle observationsSST: AVHRR, AATSR, AMSR-E

Satellite observations (14inst.): IR and MW radiances

Platform Instrument

NOAA-18NOAA-19MetOp-A

MetOp-B

EOS: AquaSuomi-NPP

AMSU-A/B AMSU-A/B AMSU-A/B + HIRSIASI (138 channels)AMSU-A/B + HIRSIASI (138 channels)AIRS (139 channels)CrIS (134 channels)ATMS

Current NWP Usage

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F

U

T

U

R

E

Instrument/observation Platform Comments

AHI clear sky radiances Himawari-8 Improved DA in AUS region

COSMIC-2 Receivers

Bending Angle

COSMIC-2

Constellation

Improved Global Analysis

GPS Sat2Ground ZTD GPS Improved moisture analysis

SEVERI clear and

SEVERI all-sky IR radiances

Meteosat-8 Indian Ocean coverage, potential

to improve TC forecasts

SAPHIR

water vapour sensitive

microwave radiances

Megha-

Tropiques

Potential to improve tropical, TC

analyses and forecasts

MWTS-2 and MWHS-2

microwave radiances

Fengyun-3C General improvement to analysis

RapidScat

Scatterometer surface winds

International

Space Station

Significant improvement to TC

track forecasts

SSMIS

microwave radiances

DMSP

F17,18,19

General improvement to analysis

ADM Aeolus ADM General improvement to (wind)

analysis

LeoGeo AMVs multiplatform General improvement to (wind)

analysis – high lattitude

Future Usage

(14 new

instruments)

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AIRSAIRSAIRSAIRS

IASIIASIIASIIASI

CrISCrISCrISCrIS

Ultraspectral Ultraspectral Ultraspectral Ultraspectral

Advanced SoundersAdvanced SoundersAdvanced SoundersAdvanced Sounders

Recent and Impending Advances - Examples

AMVs

GPS RO

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Operational ECMWF system September to December 2008.

Averaged over all model layers and entire global atmosphere. %

contribution of different observations to reduction in forecast error.

Advanced Sounders have largest single instrument impact in reducing forecast

errors.Courtesy: Carla Cardinali and Sean Healy, ECMWF 22 Oct. 2009

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ACCESS APS2: Forecast Sensitivity to Observations

Global 24-hour forecast error reduction from each of the observation types assimilated in ACCESS

• Three months: April, May and June 2016. Himawari-8 AMVs included in full period.• All types of observations are beneficial, i.e. reduce the forecast error. • Total impact (LH panel) is dominated by satellite instruments (e.g. the IASI, AMSU and CrIS

sounding instruments carried on polar orbiters and AMVs) - due to large numbers & global coverage.

• Greater impact per observation (RH panel) comes from balloon upper air measurements plus surface measurements from drifting and fixed buoys.

Colours:

SatelliteUpper air networkSurface network

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AIRSAIRSAIRSAIRS

IASIIASIIASIIASI

CrISCrISCrISCrIS

Ultraspectral Advanced Sounders

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Spectral Coverage and Example

Observations of AIRS, IASI, and CrIS

AIRS, 2378

CrIS, 1305

IASI, 8461

CIMSS

CIMSS

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Retrieval Accuracy Vs Spectral Resolution (i.e., number of spectral radiance observations)

Temperature

Water Vapor

# chnls/δν

18/15 cm-1

800/1.2 cm-1

1600/0.6 cm-1

3200/0.3 cm-1

# chnls/δν

18/15 cm-1

800/1.2 cm-1

1600/0.6 cm-1

3200/0.3 cm-1

The vertical resolution and accuracy increases greatly going from multi-spectral to ultra-spectral resolution. The improvement in ultra-spectral performance is proportional to the square root of the number of channels (i.e., S/N)

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AIRS Data AssimilationAIRS Data AssimilationAIRS Data AssimilationAIRS Data AssimilationJJJJ. Le Marshall, J. Jung, J. Derber, R. Treadon, . Le Marshall, J. Jung, J. Derber, R. Treadon, . Le Marshall, J. Jung, J. Derber, R. Treadon, . Le Marshall, J. Jung, J. Derber, R. Treadon,

S.J. Lord, S.J. Lord, S.J. Lord, S.J. Lord, M. Goldberg, C. Barnet, W. Wolf and HM. Goldberg, C. Barnet, W. Wolf and HM. Goldberg, C. Barnet, W. Wolf and HM. Goldberg, C. Barnet, W. Wolf and H----S Liu, J. Joiner,S Liu, J. Joiner,S Liu, J. Joiner,S Liu, J. Joiner,

and J Woollen……and J Woollen……and J Woollen……and J Woollen……

1 January 2004 – 31 January 2004

Used operational GFS system as Control

Used Operational GFS system Plus AIRS

as Experimental System

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Figure1(a). 1000hPa Anomaly Correlations for the GFS with (Ops.+AIRS) and

without (Ops.) AIRS data, Southern hemisphere, January 2004

S. Hemisphere 1000 mb AC Z

20S - 80S Waves 1-20

1 Jan - 27 Jan '04

0.6

0.65

0.7

0.75

0.8

0.85

0.9

0.95

1

0 1 2 3 4 5 6 7

Forecast [days]

An

om

aly

Co

rrela

tio

n

Ops

Ops+AIRS

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N. Hemisphere 500 mb AC Z

20N - 80N Waves 1-20

10 Aug - 20 Sep '04

0.6

0.65

0.7

0.75

0.8

0.85

0.9

0.95

1

0 1 2 3 4 5 6 7

Forecast [days]

An

om

aly

Co

rrela

tio

n

1/18fovs AIRS

allfovs AIRS

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Day 5 Average Anomaly Correlation

Waves 1- 20

2 Jan - 15 Feb 2004

0.83

0.835

0.84

0.845

0.85

0.855

0.86

nh 500 sh 500+.04 nh 1000+.04 sh 1000+.1

control

short airs

airs-152ch

airs-251ch

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AIRS Data AssimilationAIRS Data AssimilationAIRS Data AssimilationAIRS Data Assimilation

Using Cloudy Fields of ViewUsing Cloudy Fields of ViewUsing Cloudy Fields of ViewUsing Cloudy Fields of View

1 January – 24 February 2007

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AIRS Data AssimilationAIRS Data AssimilationAIRS Data AssimilationAIRS Data Assimilation

Using Cloudy Fields of ViewUsing Cloudy Fields of ViewUsing Cloudy Fields of ViewUsing Cloudy Fields of View

Initial Experiments: 1 January – 24 February 2007

Assume :

Rj = ( 1 – αj ) Rclr + αj Rcld

Only variability in AIRS fov is cloud amount αj

9 AIRS fovs on each AMSU-A footprint used to

estimate Rclr

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N. Hemisphere 500 hPa AC Z 20N - 80N Waves 1-20

1 Jan - 24 Feb '04

0.85

0.87

0.89

0.91

0.93

0.95

0.97

0.99

0 1 2 3 4 5

Forecast [days]

An

om

aly

Co

rrela

tio

n

Control AIRS (cloudy fovs)

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N. Hemisphere 500 hPa AC Z 20N - 80N Waves 1-20

1 Jan - 24 Feb '07

0.85

0.87

0.89

0.91

0.93

0.95

0.97

0.99

0 1 2 3 4 5

Forecast [days]

An

om

aly

Co

rrela

tio

n

Control AIRS (cloudy fovs)

S. Hemisphere 500 hPa AC Z 20S - 80S Waves 1-20

1 Jan - 24 Feb '07

0.8

0.82

0.84

0.86

0.88

0.9

0.92

0.94

0.96

0.98

1

0 1 2 3 4 5

Forecast [day]

An

om

aly

Co

rrela

tio

n

Control AIRS(cloudy fovs)

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Day 5 Average Anomaly Correlation

Waves 1- 20

10 Jan - 24 Feb 2007

0.73

0.78

0.83

0.88

nh 500 sh 500 nh 1000 sh 1000

Control AIRS(cloudy fovs)

Day 5 Average Anomaly Correlation

Waves 1 - 20

1 Aug - 31 Aug 2008

0.74

0.76

0.78

0.8

0.82

0.84

nh 500 sh 500 nh 1000 sh 1000

Control AIRS

Figure 6 : The impact of AIRS data on GFS forecasts at 500hPa (20°N - 80°N), 1 Jan. – 24 Feb. 2007; The pink curve denotes use of clear radiances from clear and cloudy AIRS fovs (see text) and the blue curve denotes use of non cloud effected radiances (Control).

Figure 7 ): The impact of AIRS data on GFS forecasts at 500hPa (20°S - 80°S), 1 Jan. – 24 Feb. 2007; The pink curve denotes use of clear radiances from clear and cloudy AIRS fovs (see text) and the blue curve denotes use of non cloud effected radiances (Control).

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AIRS Data AssimilationAIRS Data AssimilationAIRS Data AssimilationAIRS Data Assimilation

MOISTURE MOISTURE MOISTURE MOISTURE Forecast Impact evaluates which forecast (with or without

AIRS) is closer to the analysis valid at the same time.

Forecast Impact = 100* [Err(Cntl) – Err(AIRS)]/Err(Cntl)

Where the first term on the right is the error in the Cntl

forecast. The second term is the error in the AIRS forecast.

Dividing by the error in the control forecast and multiplying

by 100 normalizes the results and provides a percent

improvement/degradation. A positive Forecast Impact means

the forecast is better with AIRS included.

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Page 30: Benefits from Advances in the Data Assimilation Earth Observations from Space · 2016. 12. 12. · Earth observations From Space Fig. 8(c). SH 500hPa height anomaly correlation for

AIRS /IASI Data AssimilationAIRS /IASI Data AssimilationAIRS /IASI Data AssimilationAIRS /IASI Data Assimilation

Using Moisture ChannelsUsing Moisture ChannelsUsing Moisture ChannelsUsing Moisture Channels

Adding 80 AIRS and IASI Tropospheric Water Vapour

channels

Adding 40 AIRS and IASI Stratospheric Water Vapour

channels

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The AIRS and IASI water vapour channels added to the

operational data base for the water vapour experimental

runs.

Tropospher

ic

Channels

AIRS tropospheric channels (2378 channel set): 1301,

1304, 1449, 1455, 1477, 1500, 1519, ….27AIRS

Channels

IASI tropospheric channels (8461 channel set): 2701,

2741, 2819, 2889, 2907, 2910, 2939, …53 IASI

Channels

Stratosphe

ric

Channels

AIRS Channels: AIRS stratospheric channels (2378

channel set):

1466, 1614, …..9 AIRS Channels

IASI Channels: IASI stratospheric channels (8461

channel set):

3168, 3248, …31 IASI Channels

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Figure 2: Water Vapor Jacobians for IASI channel 3168

(black), which is sensitive to moisture in the Stratosphere,

similar CrIS channels half (red) and full (dark blue) spectral

resolution and the HIRS channel 12(light blue).

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control experiment

Analysing Tropospheric Moisture by Assimilating

Hyperspectral Infrared Water Vapor Channels

Figure 3: Specific humidity fits to rawinsondes humidity data during the time period March to May 2010 for the analysis, 6(Ges)- , 12- , 24- , 36- and 48-hour forecasts. Note the considerable improvement in the 6-hour and 12-hour forecasts.

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Figure 11: Emissivity near 10.85 or µm computed from IASI observations over South Central Australia on the 17th of June 2008.The image is from MTSaT-1R. (Emissivity greater than 0.984 yellow, emissivity between 0.92 and 0.984 magenta).

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HimawariHimawariHimawariHimawari----6,7 and 86,7 and 86,7 and 86,7 and 8

THE GENERATION THE GENERATION THE GENERATION THE GENERATION

AND ASSIMILATION AND ASSIMILATION AND ASSIMILATION AND ASSIMILATION

OF OF OF OF

CONTINUOUS CONTINUOUS CONTINUOUS CONTINUOUS

ATMOSPHERIC ATMOSPHERIC ATMOSPHERIC ATMOSPHERIC

MOTION VECTORS MOTION VECTORS MOTION VECTORS MOTION VECTORS

WITH WITH WITH WITH

4DVAR4DVAR4DVAR4DVAR

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Specification of “Himawari-8/9” Imager(AHI)

Band Central Wavelength

[μm] Spatial

Resolution

1 0.43 -0.48 1Km

2 0.50 -0.52 1Km

3 0.63 -0.66 0.5Km

4 0.85 -0.87 1Km

5 1.60 -1.62 2Km

6 2.25 -2.27 2Km

7 3.74 -3.96 2Km

8 6.06 -6.43 2Km

9 6.89 -7.01 2Km

10 7.26 -7.43 2Km

11 8.44 -8.76 2Km

12 9.54 -9.72 2Km

13 10.3 -10.6 2Km

14 11.1-11.3 2Km

15 12.2 -12.5 2Km

16 13.2 -13.4 2Km

X

X

X

X

X

X

X

X

X

X

X

Band Central Wavelength

[µm] SpatialResolution1 0.55 –0.90 1Km2 3.50 –4.00 4Km3 6.50-7.00 4Km4 10.3 –11.3 4Km5 11.5 –12.5 4Km

as of MTSAT-1R/2

Full Disk Imageevery 10 minutes

RGBCompositedTrue Color Image

1.3 µm for GOES-R

Water

Vapour

SO2

O3

Atmospheric

WindowsCO2

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H – 7 AMVS

MTSAT 2

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27 January – 23 February 2011

Used

■ Real Time Local Satellite Winds MTSAT-2 (EE, hourly

since 96, TB)

● 2 sets of quarter hourly motion vectors every six

hours.

● Hourly motion Vectors

■ Operational Regional

Forecast Model (ACCESS-R) and

Data Base ( Inc JMA AMVs)

OPERATIONAL SYSTEMOPERATIONAL SYSTEMOPERATIONAL SYSTEMOPERATIONAL SYSTEM

NEAR RT TRIALNEAR RT TRIALNEAR RT TRIALNEAR RT TRIAL

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Fig.6(a). The RMS difference between

forecast and verifying analysis geopotential

height(m) at 24 hours for ACCESS-R (green)

and ACCESS-R with hourly AMVs (red) for

the period 27 January to 23 February 2011.

Fig.6(b). The RMS difference between

forecast and verifying analysis geopotential

height(m) at 48 hours for ACCESS-R (green)

and ACCESS-R with hourly AMVs (red) for

the period 27 January to 23 February 2011.

HIMAWARIHIMAWARIHIMAWARIHIMAWARI----7 NEAR RT TRIAL7 NEAR RT TRIAL7 NEAR RT TRIAL7 NEAR RT TRIAL

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GENERATION AND GENERATION AND GENERATION AND GENERATION AND

ASSIMILATION ASSIMILATION ASSIMILATION ASSIMILATION

OF OF OF OF

CONTINUOUS CONTINUOUS CONTINUOUS CONTINUOUS

(10 Minute) (10 Minute) (10 Minute) (10 Minute)

ATMOSPHERIC ATMOSPHERIC ATMOSPHERIC ATMOSPHERIC

MOTION VECTORS MOTION VECTORS MOTION VECTORS MOTION VECTORS

FROM MTSATFROM MTSATFROM MTSATFROM MTSAT----1R1R1R1R

USINGUSINGUSINGUSING

4DVAR4DVAR4DVAR4DVAR

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Fig. 13 Bureau of Meteorology Analysis for 12 UTC on 27 January 2014. Fig. 14. Bureau of Meteorology Analysis for 12 UTC on 30 January 2014

Fig.15 The Bureau of Meteorology operational three-day MSLP (hPa) forecast valid 1200 UTC 30 January

2014, shown remapped over an MTSat infrared image, valid at the same time.

Fig.16 The Bureau of Meteorology three-day MSLP (hPa) forecast valid, 1200 UTC 30 January 2014 using

the next generation operational regional forecasting system with ten, fifteen and sixty minute AMV data from

MTSat-1R and MTSat-2. The forecast remapped over the 1200 UTC MTSat image.

First Results –

MTSAT-1R

APS-2 APS-1

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RECENT GENERATION RECENT GENERATION RECENT GENERATION RECENT GENERATION

AND ASSIMILATION AND ASSIMILATION AND ASSIMILATION AND ASSIMILATION

OF OF OF OF

CONTINUOUS CONTINUOUS CONTINUOUS CONTINUOUS

(10 Minute) (10 Minute) (10 Minute) (10 Minute)

HHHH----8 ATMOSPHERIC 8 ATMOSPHERIC 8 ATMOSPHERIC 8 ATMOSPHERIC

MOTION VECTORS ,MOTION VECTORS ,MOTION VECTORS ,MOTION VECTORS ,

GEOCAT GEOCAT GEOCAT GEOCAT

ANDANDANDAND

4DVAR4DVAR4DVAR4DVAR

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HimawariHimawariHimawariHimawari----8 Operational AMV Generation8 Operational AMV Generation8 Operational AMV Generation8 Operational AMV Generation

Uses 3 images separated by 10 min in HSF format.

Employs modified GEOCAT (Geostationary Cloud Algorithm Testbed) software in initial processing.

Height assignment methods similar to GOES-R ABI ATBD For Cloud Height (Heidinger, A. 2010)

AMV estimation is similar to GOES-R ABI ATBD for Derived Motion Winds (Daniels, 2010) / BoM system

Error characterization, data selection, QC via EE, QI, ERR etc. (Le Marshall et al., 2004, 2015)

Height assignment verification Cloudsat/Calipso, RAOBS

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H – 8 AMVS

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).

Fig.3 Himawari-8 AMVs tracked using IR (11 µm) channel

14 tracers at 00 UTC 16 January 2016 using the next generation operational system

Fig. 4. Measured error (m/ s) vs Expected Error (m/s) for low-level Himawari-8 IR winds (1 31 August –29 2016).

Fig. 5 Coverage of AMVs from Himawari-8 in the tropics to the north

of Australia 0600 UTC 6 September 2015

Fig. 6 Himawari-8 level of best fit height assignment statistics for CH.14

AMVs for September 2015 (see text)

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Fig. 7 Himawari-7 AMVs tracked using the IR and VIS channels at 00 UTC on 20 August 2015 from the operational system

Fig.8 Himawari-8 AMVs tracked using the IR (11 µm) channel at 00 UTC on 20 August 2015 using the next generation operational AMV system

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Fig.7 AMVs generated around Australia 0000UTC 29 April 2015 – Note box around Australia. Fig.8 AMVs generated around Australia 0000UTC 29 April 2015 – View from the south.

Fig.9AMVs generated around Australia 0000UTC 29 April 2015 – View from the west. Fig.10AMVs generated around Australia 0000UTC 29 April 2015 – Slant view from southwest.

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Verification for real time vectors

from Himawari-7 and Himawari-8

Table 2 Verification Table for Himawari-8

IR (channel 14) AMVs compared to

radiosondes 1 March – 31 March 2016

AMV

Type

Category m/s NOBS

Low

Sep.

<50 km

MMVD

RMSVD

BIAS

2.4

2.8

0.3

358

High

Sep.

<50 km

MMVD

RMSVD

BIAS

3.3

3.9

-0.6

1460

Table 3 Verification Table for Himawari-7 IR

(channel 14) AMVs compared to radiosondes

1 March – 20 March 2016

AMV

Type

Category m/s NOBS

Low

Sep.

<50 km

MMVD

RMSVD

BIAS

2.5

2.9

-0.6

57

High

Sep.

<50 km

MMVD

RMSVD

BIAS

3.5

3.9

-1.4

291

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geographical area. After March only 2 datasets were available.

Fig.13 MSLP anomaly correlation coefficients for the Northern Hemisphere Annulus for

the operational system (blue) and for the operational test system for 4 – 26 March 2016.

Change-over Month – Triply Redundant system

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Summary and Conclusions10-minute winds are being continuously generated and assimilated operationally in the Australian region with 4D Var – First country to do so.

H-8 10 minute DMVs provide an improved spatial and temporal resolution database for analysis and forecasting.

The quality of these higher spatial, temporal and spectral density data is of a level which renders them beneficial for NWP.

If the data is thinned to equal spatial density, the quality of the H-8 data exceeds that of the operational H7 data.

Data assimilation tests showed successful transfer of data into operations and successful use of the data by the NWP system.

Further quantification of the impact of these data in our current operational prediction system is underway. This involves use of all 10 minute data in the prediction of TC activity and severe weather.

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GPS/COSMIC RADIO OCCULTATION

24 transmitters

6 receivers3000 occultations/day

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1 November – 30 November 2010

Used

■ Bending Angle data from

● the COSMIC Constellation

● GRACE and METOP

■ Operational Global

Forecast Model (ACCESS-G) and

Operational Data Base

OPERATIONAL FORECAST SYSTEM ACCESSOPERATIONAL FORECAST SYSTEM ACCESSOPERATIONAL FORECAST SYSTEM ACCESSOPERATIONAL FORECAST SYSTEM ACCESS----GGGG

OPERATIONAL TRIALOPERATIONAL TRIALOPERATIONAL TRIALOPERATIONAL TRIAL

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Figure 10(a). RMS Errors and anomaly

correlations for ACCESS-G MSLP

forecasts to five days, for the Australian

region. Shown are results for Control

(black), and with GPS RO data (red) for

the period 1 November to 30 November

2010.

Figure 10(b). RMS errors and anomaly

correlations for ACCESS-G 500hPa

forecasts to five days, for the Australian

region. Shown are results for Control

(black) and with GPS RO data (red) for

the period 1 November to 30 November

2010.

Figure 10(c). RMS errors and anomaly

correlations for ACCESS-G 200hPa

forecasts to five days, for the Australian

region. Shown are results for Control

(black) and with GPS RO data (red) for the

period 1 November to 30 November 2010.

OPERATIONAL TRIAL - AUSTRALIAN REGION

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Command and acquisition groundstation for the new COSMIC-2 Constellation

RecentlyAnomalous GNSS Radio Occultation COSMIC 2 Ground Station

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The FutureThe FutureThe FutureThe FutureDistribution of simulated daily COSMIC II RO events in the Australasian region with GPS, Galileo, Glonass and QZS-1

…..

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Summary• The great benefit of current RO data in the Australian

Region and Southern Hemisphere have been recorded using data impact studies

• COSMIC, GRACE and METOP data have been successfully assimilated into the current ACCESS system and the data are now being used in the BoMs operational forecast system

• The data are important for climate quality analyses

• The data are important for climate monitoring

• The BoM is providing a command and acquisition Ground-station for the new COSMIC-2 Constellation

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ADM (Atmospheric Dynamics Mission) - Aeolus

ADM-Aeolus Doppler wind lidar Observing System Simulation ExperimentBy A. STOFFELEN1∗∗∗∗, G. J. MARSEILLE1, F. BOUTTIER2,D. VASILJEVIC3, S. de HAAN1 and C. CARDINALI3

Q. J. R. Meteorol. Soc. (2006), 132, pp. 1927–1947

Satellite built by the European Space Agency that is due for launch in 2017.

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DOPPLER WIND LIDAR OSSE

Forecast skill, as represented by the wind vector RMSE (m s−1) at 500 hPa of the forecast fields forthe NoDWL (dashed) and DWL (solid) experiments (both with respect to the nature run), as a function of forecastrange and for six regions: (a) the northern hemisphere, (b) the southern hemisphere, (c) the tropics, (d) Europe,(e) the North Atlantic and (f) North America. Forecasts are initialized with analyses at 12 UTC each day in theperiod 6 to 20 February 1993. The mean is taken over all 15 cases.

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Future ProspectsEnvironmental analysis /prediction using current and future satellite systems have been examined.

The great benefits from recent advances using current Earth Observations from Space have been noted.

The potential for greatly increased benefit from current and future satellite and assimilation systems has been noted and some of the planning related to gaining these benefits summarised.

Increasing benefits will continue to accrue from current and next generation advanced instruments, which represent an investment of billions of dollars by the international community. (eg.CrIS, ATMS, VIIRS,ABI,AHI, ADM, …ASCENDS….). This will need some local co-investment in infrastructure, research and trained staff.

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Looking DownLooking DownLooking DownLooking Down

IsIsIsIs

Looking UpLooking UpLooking UpLooking Up

TC LAURENCE - Dec. 2009

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