practical exchange of atovs direct broadcast data in asia pacific region akihiko nakazono office of...

Practical Exchange of ATOVS Direct Broadcast Data

in Asia Pacific Region

Akihiko Nakazono

Office of International Communications,

Forecast Department, JMA

APSDEU-6, 1-3 June 2005, Seoul, Republic of Korea

© NOAA/NESDIS

PART 1PART 1

Status of ATOVS-DB Data Related Status of ATOVS-DB Data Related Activities in JMAActivities in JMA

Topic-1ATOVS-DB Data at Syowa StationATOVS-DB Data at Syowa Station

• Syowa Station, belongs to the National Institute of Polar Research (NIPR) , was established in 1957 at 69.00S and 39.58E Antarctica.

• Showa Station has been receiving NOAA HRPT data for research and operation.

• The HRPT data are relayed to the NIPR in Tokyo near real-time through 1Mbps satellite communication circuits since 2004.

ATOVS-DB Data at Syowa StationATOVS-DB Data at Syowa Station(cont.)

• JMA started to negotiate with the NIPR on acquisition and utilization of the data, including dissemination to WMO Members.

• The NIPR seems to allow dissemination to WMO members under the their data policy, i.e., inclusion of the originator name in the data.

• The Meteorological Satellite Centre is experimentally getting the data from the NIPR, and studying for applying the AAPP package effectively.

Sample ATOVS Data Received at Sample ATOVS Data Received at Syowa StationSyowa Station

Topic-2

Replacement Plan of HRPT EquipReplacement Plan of HRPT Equipment at the Meteorological Satellitment at the Meteorological Satellit

e Centre (MSC), Kiyosee Centre (MSC), Kiyose

Reception of NOAA DB DataReception of NOAA DB Dataat MSC (current system)at MSC (current system)

• JMA has been receiving the NOAA satellite data since 1968 at the MSC, Kiyose

• Currently, JMA receives HRPT data from NOAA-16 and 17 around 10 orbits a day

(c)Nojima

NNew Reception Systemew Reception System

• The MSC is procuring a new POS receiving system which replaces current one.

• Capability of direct reception of the forthcoming AHRPT from METOP as well as HRPT from NOAA satellites

• In addition to the L-band, antenna has a capability of receiving X-band for the reception of HRD from NPP/NPOESS

• New system start to work in March 2006

Diagram of new reception system

INTFINTF

DRIVERCIRCUIT

DRIVERCIRCUIT

LAN

3mΦParabolicantenna Time

Server

TimeServer

ＮＯＡＡRx

ＮＯＡＡRx

ＭＥＴＯＰRx

ＭＥＴＯＰRx

INTFINTFSignal Processing

& Control Unit

Optical Cable

SAPS

HRPT, AHRPT

Antenna Tower Operation Room

SAPS:Satellite Data

Advanced Processing

System

LNALNA

D/CD/C

Future plan of polar orbit satellite data receptionFuture plan of polar orbit satellite data reception

METOP-2

METOP-1

NOAA-N’

NOAA-18

NOAA-17

NOAA-16

201320122011201020092008200720062005

： PM Satellite ： AM Satellite

As of May 2005

Status of AAPP InstallationStatus of AAPP Installation

• JMA has already utilized the AAPP ver.4.4 operationally for ATOVS DB data at MSC/JMA and for global ATOVS data at NPD/JMA.

• The AAPP processing time for DB HRPT data is less than two minutes per orbit.

PART 2PART 2

Practical Exchange of ATOVS-DB Practical Exchange of ATOVS-DB Data in Asia PacificData in Asia Pacific

CONTENTS CONTENTS

• BackgroundBackground• Analysis & Estimation for exchangeAnalysis & Estimation for exchange• ProposalProposal

BackgroundBackground

• The importance of ATOVS DB data for NWPs has been confirmed and therefore the exchange of ATOVS DB data have been discussed in the APSDEU since its fourth meeting in March 2002.

• APSDEU-4: Recommendation 8– The meeting noted the importance of real time data exchange

of locally received ATOVS data. – KMA and CMA agreed to explore the possibility of real time AT

OVS data exchange.– BoM will investigate the possibility of distributing locally receiv

ed ATOVS data.

BackgroundBackground(cont.)

• Action Item 2004-5-15 （ Beijing,2004)– The meeting noted the importance of real time data exchange

of locally received ATOVS L1B or L1C data processed by AAPP.

– KMA, CMA and JMA agreed to investigate the possibility of real time ATOVS data exchange.

– The Australian Bureau of Meteorology also agreed to investigate the possibility of distributing real time ATOVS data.

– These countries agreed to explore the EUMETSAT EARS approach as one possible strategy to achieve implementation.

BackgroundBackground (cont.)

• EARS has been established for collecting and disseminating ATOVS data in Europe and North America since 2001

• CGMS has been discussing the exchange of ATOVS DB Data within the framework of WMO Space Program

• WMO , hosted by EUMETSAT, held the 1-st RARS Workshop in Dec 2004

In the 1-st RARS Workshop,In the 1-st RARS Workshop,• Three Areas are Focused and Discussed for RARS in the Asi

a Pacific Region– Data Collection

• Potential HRPT Stations - at least, 19 stations are identified• Communication means - FTP over GTS, Internet ….

– Data Distribution• Communication means - FTP over GTS, Internet ,...

– Standardization• The data should only be processed to AAPP L1A at the various

HRPT station sites• Further processing to AAPP L1C at the distribution centres to en

sure better calibration on the data

Potential HRPT Stations in the Asia PacificPotential HRPT Stations in the Asia Pacific

• Existing National Stations: in Australia, China - including Hong Kong, Japan, Korea, and New Zealand

• Singapore, Guam, Tahiti, Fiji, (La Reunion) • Antarctic Stations:

– McMurdo, Dumont d’Urville , Casey, Syowa

Coverage by the 19 stations above

CONTENTS CONTENTS

• BackgroundBackground• Analysis & Estimation for exchangeAnalysis & Estimation for exchange• ConclusionConclusion

HRPT Stations in BoM, CMA, HKO, HRPT Stations in BoM, CMA, HKO, KMA, and JMAKMA, and JMA

• BoM– Darwin, Melbourne, Perth, Casey (Antarctica)

• CMA– Beijing, Guangzhou , Urumuqi, Lasha

• HKO– Hong Kong

• KMA– Seoul

• JMA– Kiyose, Syowa (Antarctica)

There are 12 candidates

Coverage by 12 HRPT Stations

Coverage by the 12 HRPT Stations (Northern Hemisphere)

EARS (DEC 2003)

Coverage by the 12 HRPT Stations (Southern Hemisphere)

Duration and Completion of reception

A coverage of the station (depends on conditions)

Orbit NOrbit N+1Orbit N+2

Completion

Completion

Duration

A Receiving Station

0:00

2:00

4:00

6:00

8:00

10:0

0

12:0

0

14:0

0

16:0

0

18:0

0

20:0

0

22:0

0

0:00

Completion Time (UTC)

1st May

2nd May

3rd May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations HRPT Receiving Stations (NOAA-16, 1(NOAA-16, 1stst-3-3rdrd May) May)

Origin of each circle indicates completion time.

Diameter of each circle is relative to the duration of reception (max. 15-minutes)

Estimated Completion Time of HRPT Estimated Completion Time of HRPT Receiving Stations (superposition in May)Receiving Stations (superposition in May)

0:00

2:00

4:00

6:00

8:00

10:0

0

12:0

0

14:0

0

16:0

0

18:0

0

20:0

0

22:0

0

0:00

Completion Time (UTC)

NOAA-16,Superpositionin May

NOAA-17,Superpositionin May

DarwinMelbourn

PerthCaseyKiyoseSyowaSeoul

BeijingGuangzhUrumuqi

LashaHong

Statio

0:00

2:00

4:00

6:00

8:00

10:0

0

12:0

0

14:0

0

16:0

0

18:0

0

20:0

0

22:0

0

0:00

Completion Time (UTC)

NOAA- 16,Superposition

NOAA- 17,Superposition

NOAA- 16,1st May

NOAA- 17,1st May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations (1HRPT Receiving Stations (1stst May) May)

1 2 3 4 Congestion Times

2:00

3:00

4:00

5:00

Completion Time (UTC)

NOAA- 16,1st May

NOAA- 17,1st May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations (congestion time1)HRPT Receiving Stations (congestion time1)

5:00

6:00

7:00

8:00

Completion Time (UTC)

NOAA- 16,1st May

NOAA- 17,1st May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations (congestion time2)HRPT Receiving Stations (congestion time2)

13:0

0

14:0

0

15:0

0

16:0

0

Completion Time (UTC)

NOAA- 16,1st May

NOAA- 17,1st May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations (congestion time3)HRPT Receiving Stations (congestion time3)

18:0

0

19:0

0

20:0

0

21:0

0

Completion Time (UTC)

NOAA- 16,1st May

NOAA- 17,1st May

Darwin

Melbourne

Perth

Casey

Kiyose

Syowa

Seoul

Beijing

Guangzhou

Urumuqi

Lasha

Hong Kong

Station

Estimated Duration and Completion Time at Estimated Duration and Completion Time at HRPT Receiving Stations (congestion time4)HRPT Receiving Stations (congestion time4)

Characteristics of ATOVS DB reception in view of exchange

• Rush hour of ATOVS data are foreseen around six to eight times a day in the East Asia

• In a rush hour, most of HRPT stations in CMA, HKO, KMA and JMA complete reception in a short period (within 10 minutes )

• In view of traffic, the degree of rushing depends on orbit position, data processing time at stations and centers, and national and international communications…should be examined

Amount of ATOVS Data Unit to be Transferred

• AAPP Level 1A/1B– Maximum Size = 1.2MB / Pass / Satellite in gzip compressed

file• AAPP Level 1C

– Typical Size = 1.1MB / Pass / Satellite in BUFR form• Roughly, 1.2MB is a index of data transfer• A 1.2MB file is transferable within 5 minutes

through a 32Kbps circuit with 100% efficiency

BoMMelbourne

BoMMelbourne

HKOHong Kong

HKOHong Kong

KMASeoul

KMASeoul

JMATokyo

JMATokyo

F/R

F/R

F/R

MSS TokyoMSS Tokyo

NOAA

ATOVS

256Kbps 1.5Mbps

64Kbps

192Kbps

64Kbps

128Kbps 128Kbps

CMABeijing

CMABeijing

CIR=16 CIR=32

CIR=48 CIR=48

CIR=16

CIR=16

CIR=16 UNIX Workstation4 processors

CIR=16

FTP File exchange

GTS Socket Message, FAX exchange

F/R : Frame Relay CIR : Committed Information Rate

（ RMDCN）

GTS links for exchange of ATOVS dataGTS links for exchange of ATOVS data FTP can be used for ATOVS data exchange over GTS among these centres

MSS TokyoMSS Tokyo

FTP File exchange

GTS Socket Message, FAX exchange

F/R : Frame Relay CIR : Committed Information Rate

Use of GTS links for exchange of ATOVS Use of GTS links for exchange of ATOVS datadata

FTP can be used for ATOVS data exchange over GTS among these centers In the Rush Hour

BoMMelbourne

BoMMelbourne

HKOHong Kong

HKOHong Kong

KMASeoul

KMASeoul

JMATokyo

JMATokyo

F/R

F/R

F/R

NOAA

ATOVS

256Kbps 1.5Mbps

64Kbps

192Kbps

64Kbps

128Kbps 128Kbps

CMABeijing

CMABeijing

CIR=16 CIR=32

CIR=48 CIR=48

CIR=16

CIR=16

CIR=16 UNIX Workstation4 processors

CIR=16

（ RMDCN）64Kbps

96Kbps

96Kbps

96Kbps

Rough Estimation To complete file transfer

around 5 minutes

• These five centers are connected by TCP/IP links in GTS directly or via Tokyo

• FTP can be used for ATOVS data exchange over GTS among these centers

• FTP server at Tokyo is accessible through GTS and has capability to collect and distribute ATOVS data files

• Most of GTS links among these centers seem to have, or will have, enough spare capacity for ATOVS data, but some circuits have to be considered to widen the bandwidth to avoid delay in congestion hours

Use of GTS links for the exchange of ATOVS data among BoM, CMA, HKO,

KMA and JMA

Standardization/Coordination( for data handling and utilizing )

• Type of data to be exchanged– AAPP Level L1A/L1B/L1C– AAPP Version?

• Names and Codes– Name (Code) of the HRPT Stations and Processing Centre

s required in the AAPP and applied to output data, should be coordinated globally

• Format of data– AAPP Specific file, or– BUFR form(L3C) (TBD)

• Descriptors and codes to be used(Is it enough with 3-10-008, 3-10-009, 3-10-010 for L1C?)

• Any additional descriptors and/or codes to be defined?– Common encoder is expected for BUFR encoding

To Exchange ATOVS Data, some rules are required and shall to be coordinated

Standardization/Coordination( for data transfer )

• Data compression– gzip, bzip2 ?

• File naming convention for transfer– For WMO code: WMO PUB 386, AII-15– For other type: TBD (WMO has not defined yet)

• FTP procedure – WMO PUB 386, AII-15– Get/Put? (needs bilateral agreement between centres)

• Anything else ?

CONTENTS CONTENTS

• BackgroundBackground• Analysis & Estimation for exchangeAnalysis & Estimation for exchange• ConclusionConclusion

The Time Has Come

• JMA already has capability of receiving HRPT, pre-processing by AAPP, and exchanging ATOVS data through the GTS, and is willing to perform our part of the retransmission functions through the GTS in cooperation with other Centers concerned

• JMA propose: – to start to exchange ATOVS AAPP data– among BoM, CMA, HKO, KMA , and JMA– through the GTS– by the end of 2005

The Time Has Come (Cont.)

• APSDEU is expected to start discussion and coordination on the exchange of ATOV DB data

• Then, examine the exchange and make reviews to the next step=> The next meeting is expected to be held in early 2006

Thank you for your attention!!Thank you for your attention!!

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