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Welcome to HDF Workshop V
“Selected” ESDIS Status
What is HDF/HDF-EOS
Richard Ullman
ESDIS
Outline
Welcome
“Selected” ESDIS Status
What is HDF/HDF-EOS
HDF & HDF-EOS Workshop 5
This is the fifth “annual” HDF workshop sponsored by ESDIS and NCSA.
Combined this year with the Science Data Processing (SDP) workshop after our
September meeting was canceled.
We use this workshop to help guide our priorities for HDF and HDF-EOS
development over the next year. Please make it a “workshop” by asking
questions and expressing opinions.
Consulting opportunities with NCSA and with ECS
2 lunches
After hours
Please sign up

Panel discussion tomorrow afternoon.
Presentations from this workshop will be posted on the web on the HDF–EOS tools
and information web site:
http://hdfeos.gsfc.nasa.gov
Also on the Science Data Processing workshop page:
http://that.gsfc.nasa.gov/gss/workshop2002/workshop.html
Outline
Welcome
“Selected” ESDIS Status
What is HDF/HDF-EOS
Data Availability
Since Terra launch, the EOSDIS science systems (ECS, DAACs, and SIPS) have
processed and made available over 750 Terabytes Terra and Landsat 7 products.
In many cases, validation of Terra products is continuing and care should be
taken when using these data for science research.
ASTER data, CERES data, and some MODIS products are at the “validated” state

ASTER
Validated: Radiance at sensor, AST06 Decorrelation stretch, AST04 Brightness temperature
Provisional: AST09 Surface radiance-VNIR,SWIR, AST09T Surface radiance-TIR, AST07 Surface
reflectance-VNIR,SWIR , AST08 Surface kinetic temperature, AST05 Surface emissivity

CERES “Edition 1” validated data released. “Edition 2” reprocessing expected to
be completed June ‘02.
MISR products upgraded from “beta” to “provisional”:
Geometric Parameters (from MISR PGE7)
L1B2 Terrain Radiance(a.k.a. GRP_TERRAIN_GM, MI1B2T)
L1B2 Ellipsoid Radiance

(from MISR PGE1)

MODIS data reprocessing is in process, many datasets in “provisional status”
MOPITT
Limited amounts of Beta quality data are available from the LaRC DAAC.
Terra Archive Volume Against “Baseline Volumes”
Total L0-4 Archive Volume for All Terra Instruments (w/o CERES): 8-Day Average
March 2000 - September 2001
Archive Volume Average - 930.4 GB/day
2,500

Baseline Volumes (GB/day)
03/00 - 856
03/01 - 1,758
09/01 - 2,361

1,500

1,000

Date

09/01/01

08/01/01

07/01/01

06/01/01

05/01/01

04/01/01

03/01/01

02/01/01

01/01/01

12/01/00

11/01/00

10/01/00

09/01/00

08/01/00

07/01/00

06/01/00

05/01/00

0

04/01/00

500

03/01/00

Volume (GB/day)

2,000
EOS Data Distributed to End-Users (via EDG)
Future Planning – Data Pools
ECS DAACs are being augmented with a new delivery capability – Data Pools
Data Pools are large, on-line, smart disk farms attached to ECS that allow users to
quickly download key, popular data sets
The Data Pool hardware and software will be installed at the DAACs in first quarter of FY02.
Data pools have metadata inventories to enable data location and filtering including
personalized data view and to support DAAC controlled data residency.
Special services, including search and subsetting, will be available to users through the data
pool interface (different from EDG).
User interface is via a “navigation” client based on GSFC DAAC-developed WHOM interface

Data pools are being procured using funds from the ECS “Synergy” earmark managed by
NASA HQ/YO.
Operations concept for the data pools is being coordinated with YO (Gubbels) to ensure adequate
support for YO applications requirements
DAAC Managers will work with their UWGs and YO to establish a data management plan for their Data
Pool
Future Planning - EMD Contract
The ESDIS Project is preparing to procure an ESDIS Maintenance and Operations
contractor
ECS Maintenance and Development (EMD) Contract will be an Indefinite Delivery
Indefinite Quantity (IDIQ) procurement
Broad scope of potential work provides flexibility with minimum commitment
Specific work added by multiple Task Orders
5 year overall period of performance; specific tasks define their own periods of performance
(e.g., Task 1 will be 3 years)

Extended transition period between ECS and EMD designed to ensure transfer of
knowledge of developed operational ECS to EMD winner.
Target RFP release is Mid-March 2002.
Community Advisory Process – DAAC UWG
The DAACs and the ESDIS Project continue to receive critical assessment and
recommendations from the DAAC User Working Groups (UWGs)
The UWGs are comprised of discipline and cross-discipline scientists and by applications
researchers and data users.
The UWG Chairs have met through telecons to exchange ideas and lessons learned regarding
the UWG process.
Initiated and chaired by the ESDIS Project Scientist

UWGs meet every 6-9 months and are always looking for new members to augment their
panels.
Community Advisory Process – DAWG
The ESDIS Project has formed a special Data Access Working Group (DAWG)
The DAWG is comprised of representatives from the DAACs, the Science Working Group on
Data (SWGD), the instrument science teams, the SIPSs, and the general user community
The DAWG is addressing operations concepts and system inefficiencies that may be limiting
access to EOS data at the DAACs
Key problem areas have been identified and prioritized for work off.
Where problems are already known (through existing NCRs) the priority for work off of those NCRs has
been raised.
Other, new NCRs, have been written against the system to improve access throughput.
Identifying new capabilities that would support refined data access operations concepts

The DAWG process has been very effective, due in large part to the “targeted” focus of the
working group
Need and effectiveness of focused “tiger teams” is a key lesson learned for NewDISS
Community Advisory Process – SWGD
The Science Working Group on Data (SWGD) is comprised of representatives from
the EOS instrument teams (primarily Terra), the DAACs, and technical experts
from the ESDIS project.
The SWGD is an advocate for EOS science processing in an advisory role in helping
ESDIS prioritize use of enhancement resources
The SWGD has been looking at throughput requirements for the EOS science data processing
and distribution based on measured performance of systems and algorithm software.
SWGD has made numerous recommendations to the Project for hardware enhancement to
improve throughput in key, target areas.
The SWGD as begun looking at other data center issues including distribution and tool
availability.
Outline
Welcome
“Selected” ESDIS Status
What is HDF/HDF-EOS
What is HDF?
A container for storing scientific data
A portable format and a portable library

Stores images, multidimensional arrays, tables, etc.
Emphasis on storage and I/O efficiency
Free and commercial software support
Emphasis on standards
Users from many engineering and scientific fields
What is HDF5?
New format(s) and library (c.1998)
Format is not compatible with HDF4
library
Primary Objects:
Groups
Datasets

Secondary Objects:
Datatypes
Dataspaces

Additional means to organize data
Attributes
Sharable objects
Storage and access properties

New Demands
Bigger, faster machines and storage
systems
massive parallelism, teraflop speeds
parallel file systems, terabyte storage

Greater complexity
complex data structures
complex subsetting

Emphasis on remote & distributed access

New HDF5 Features
More scalable
Larger arrays and files
More objects

Improved data model
New datatypes
Single comprehensive dataset object

Improved software
More flexible, robust library
More flexible API
More I/O options
What is HDF-EOS?
To share files, users must organize them similarly.
HDF user groups create standard profiles
Ways to organize data in HDF files.
Metadata
API and library

HDF-EOS is the standard profile of HDF for EOS standard products
Swath
Grid
Point
Profile (Atmospheric profile)
HDF-EOS lessons learned
Ten years since first “trade study” for Earth Systems Science data format
standard.
“Baseline standard” decision September 1993(nine years)
First library was released June 1996 (six years)
HDF-EOS 5 released spring 2001 (one year)

The concept of a “profile” for interchange of files among members of a
producer/user community is reasonable.
It has been difficult for HDF-EOS development to quickly respond to community
feedback.
Standard still allows a great deal of flexibility.
This flexibility permits mission or instrument science teams to create products with the
subtlety that they require.
Flexibility also means that general purpose (cross-product) end-user tools are difficult to
support.

“Standards are difficult to negotiate but essential for success.”
- Dolly Perkins (SDP Workshop 2/27/02)

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Welcome to HDF Workshop V

  • 1. Welcome to HDF Workshop V “Selected” ESDIS Status What is HDF/HDF-EOS Richard Ullman ESDIS
  • 3. HDF & HDF-EOS Workshop 5 This is the fifth “annual” HDF workshop sponsored by ESDIS and NCSA. Combined this year with the Science Data Processing (SDP) workshop after our September meeting was canceled. We use this workshop to help guide our priorities for HDF and HDF-EOS development over the next year. Please make it a “workshop” by asking questions and expressing opinions. Consulting opportunities with NCSA and with ECS 2 lunches After hours Please sign up Panel discussion tomorrow afternoon. Presentations from this workshop will be posted on the web on the HDF–EOS tools and information web site: http://hdfeos.gsfc.nasa.gov Also on the Science Data Processing workshop page: http://that.gsfc.nasa.gov/gss/workshop2002/workshop.html
  • 5. Data Availability Since Terra launch, the EOSDIS science systems (ECS, DAACs, and SIPS) have processed and made available over 750 Terabytes Terra and Landsat 7 products. In many cases, validation of Terra products is continuing and care should be taken when using these data for science research. ASTER data, CERES data, and some MODIS products are at the “validated” state ASTER Validated: Radiance at sensor, AST06 Decorrelation stretch, AST04 Brightness temperature Provisional: AST09 Surface radiance-VNIR,SWIR, AST09T Surface radiance-TIR, AST07 Surface reflectance-VNIR,SWIR , AST08 Surface kinetic temperature, AST05 Surface emissivity CERES “Edition 1” validated data released. “Edition 2” reprocessing expected to be completed June ‘02. MISR products upgraded from “beta” to “provisional”: Geometric Parameters (from MISR PGE7) L1B2 Terrain Radiance(a.k.a. GRP_TERRAIN_GM, MI1B2T) L1B2 Ellipsoid Radiance (from MISR PGE1) MODIS data reprocessing is in process, many datasets in “provisional status” MOPITT Limited amounts of Beta quality data are available from the LaRC DAAC.
  • 6. Terra Archive Volume Against “Baseline Volumes” Total L0-4 Archive Volume for All Terra Instruments (w/o CERES): 8-Day Average March 2000 - September 2001 Archive Volume Average - 930.4 GB/day 2,500 Baseline Volumes (GB/day) 03/00 - 856 03/01 - 1,758 09/01 - 2,361 1,500 1,000 Date 09/01/01 08/01/01 07/01/01 06/01/01 05/01/01 04/01/01 03/01/01 02/01/01 01/01/01 12/01/00 11/01/00 10/01/00 09/01/00 08/01/00 07/01/00 06/01/00 05/01/00 0 04/01/00 500 03/01/00 Volume (GB/day) 2,000
  • 7. EOS Data Distributed to End-Users (via EDG)
  • 8. Future Planning – Data Pools ECS DAACs are being augmented with a new delivery capability – Data Pools Data Pools are large, on-line, smart disk farms attached to ECS that allow users to quickly download key, popular data sets The Data Pool hardware and software will be installed at the DAACs in first quarter of FY02. Data pools have metadata inventories to enable data location and filtering including personalized data view and to support DAAC controlled data residency. Special services, including search and subsetting, will be available to users through the data pool interface (different from EDG). User interface is via a “navigation” client based on GSFC DAAC-developed WHOM interface Data pools are being procured using funds from the ECS “Synergy” earmark managed by NASA HQ/YO. Operations concept for the data pools is being coordinated with YO (Gubbels) to ensure adequate support for YO applications requirements DAAC Managers will work with their UWGs and YO to establish a data management plan for their Data Pool
  • 9. Future Planning - EMD Contract The ESDIS Project is preparing to procure an ESDIS Maintenance and Operations contractor ECS Maintenance and Development (EMD) Contract will be an Indefinite Delivery Indefinite Quantity (IDIQ) procurement Broad scope of potential work provides flexibility with minimum commitment Specific work added by multiple Task Orders 5 year overall period of performance; specific tasks define their own periods of performance (e.g., Task 1 will be 3 years) Extended transition period between ECS and EMD designed to ensure transfer of knowledge of developed operational ECS to EMD winner. Target RFP release is Mid-March 2002.
  • 10. Community Advisory Process – DAAC UWG The DAACs and the ESDIS Project continue to receive critical assessment and recommendations from the DAAC User Working Groups (UWGs) The UWGs are comprised of discipline and cross-discipline scientists and by applications researchers and data users. The UWG Chairs have met through telecons to exchange ideas and lessons learned regarding the UWG process. Initiated and chaired by the ESDIS Project Scientist UWGs meet every 6-9 months and are always looking for new members to augment their panels.
  • 11. Community Advisory Process – DAWG The ESDIS Project has formed a special Data Access Working Group (DAWG) The DAWG is comprised of representatives from the DAACs, the Science Working Group on Data (SWGD), the instrument science teams, the SIPSs, and the general user community The DAWG is addressing operations concepts and system inefficiencies that may be limiting access to EOS data at the DAACs Key problem areas have been identified and prioritized for work off. Where problems are already known (through existing NCRs) the priority for work off of those NCRs has been raised. Other, new NCRs, have been written against the system to improve access throughput. Identifying new capabilities that would support refined data access operations concepts The DAWG process has been very effective, due in large part to the “targeted” focus of the working group Need and effectiveness of focused “tiger teams” is a key lesson learned for NewDISS
  • 12. Community Advisory Process – SWGD The Science Working Group on Data (SWGD) is comprised of representatives from the EOS instrument teams (primarily Terra), the DAACs, and technical experts from the ESDIS project. The SWGD is an advocate for EOS science processing in an advisory role in helping ESDIS prioritize use of enhancement resources The SWGD has been looking at throughput requirements for the EOS science data processing and distribution based on measured performance of systems and algorithm software. SWGD has made numerous recommendations to the Project for hardware enhancement to improve throughput in key, target areas. The SWGD as begun looking at other data center issues including distribution and tool availability.
  • 14. What is HDF? A container for storing scientific data A portable format and a portable library Stores images, multidimensional arrays, tables, etc. Emphasis on storage and I/O efficiency Free and commercial software support Emphasis on standards Users from many engineering and scientific fields
  • 15. What is HDF5? New format(s) and library (c.1998) Format is not compatible with HDF4 library Primary Objects: Groups Datasets Secondary Objects: Datatypes Dataspaces Additional means to organize data Attributes Sharable objects Storage and access properties New Demands Bigger, faster machines and storage systems massive parallelism, teraflop speeds parallel file systems, terabyte storage Greater complexity complex data structures complex subsetting Emphasis on remote & distributed access New HDF5 Features More scalable Larger arrays and files More objects Improved data model New datatypes Single comprehensive dataset object Improved software More flexible, robust library More flexible API More I/O options
  • 16. What is HDF-EOS? To share files, users must organize them similarly. HDF user groups create standard profiles Ways to organize data in HDF files. Metadata API and library HDF-EOS is the standard profile of HDF for EOS standard products Swath Grid Point Profile (Atmospheric profile)
  • 17. HDF-EOS lessons learned Ten years since first “trade study” for Earth Systems Science data format standard. “Baseline standard” decision September 1993(nine years) First library was released June 1996 (six years) HDF-EOS 5 released spring 2001 (one year) The concept of a “profile” for interchange of files among members of a producer/user community is reasonable. It has been difficult for HDF-EOS development to quickly respond to community feedback. Standard still allows a great deal of flexibility. This flexibility permits mission or instrument science teams to create products with the subtlety that they require. Flexibility also means that general purpose (cross-product) end-user tools are difficult to support. “Standards are difficult to negotiate but essential for success.” - Dolly Perkins (SDP Workshop 2/27/02)