Data Handling: EOSDIS


Every satellite has a mission control unit and normally a data handling center. That developed for the ESE program, designed so far to handle Terra data, is known as the EOSDIS. The volume of data received from Terra will exceed 3 terabytes daily, a huge load that will require dedicated and efficient facilities. Its main components are diagrammed. On this page also are comments and two diagrams that review what is known about the Earth�s energy budget and how physical climate and biogeochemical systems are intertwined. The page ends with a simplified table of some of the satellites of relevance to the ESE that have been put into orbit or will soon.


Data Handling: EOSDIS

Availability of data is critical to the success of NASA’s ESE. The EOS Data and Information System (EOSDIS) must be responsive to this requirement. EOSDIS manages data from NASA’s past and current Earth science research satellites and field measurement programs. During the coming EOS era, EOSDIS will allow command and control of satellites and instruments, and will generate data products based on orbital observations. In addition, EOSDIS will generate data sets made by assimilation of satellite and in situ observations into global climate models.

EOSDIS’s services will include:

  • User Support

  • Data Archive Management and Distribution

  • Information Management

  • Product Generation

  • Spacecraft Command and Control

  • Data Capture and Telemetry Processing

NASA planners base the present plans for EOSDIS on an open system, with distributed architecture. This permits data controllers to allocate EOSDIS elements to various locations to take best advantage of different institutional capabilities and science expertise.

Flow diagram showing the functions of the EOSDIS Network and its interactions with other data receiving and handling components.

EOSDIS consists of several components including:

  1. A core system (ECS), which provides the Science Data Processing Segment (SDPS), the Flight Operation Segment (FOS), and the Communications and System Management Segment (CSMS).

  2. Eight Distributed Active Archive Centers (DAACs);

  3. Scientific Computing Facilities (SCFs);

  4. the EOS Data and Operations System (EDOS); and EOS Networks

Together, these components will address all command and control; data acquisition, transport, reduction, storage, and visualization; and user access needs.

` <>`__16-20: As was noted in the answer to question 16-15, the daily load on EOSDIS will be the largest yet faced by any NASA or other space agency mission - on the order of 3 terabytes, Can you think of some way to ease or lighten that load? `ANSWER <Sect16_answers.html#16-20>`__

Further Comments

As we noted earlier, the basic impetus for the kinds of studies we described is to provide input to planners and policy makers. Having access to raw (or even processed) data is of little use to such groups. What they need is information for making decisions about allocating and, perhaps, regulating resources. This information answers questions, such as, “If we do not curb automobile pollution, what may be its effect on atmospheric composition and temperatures over the next 5-10 years?” Or, “If we continue to deforest the Pacific northwest, what may be the effect on biodiversity, land cover, land use, and water run-off patterns?”

No one can actually predict the future accurately, but we can create mathematical models that generate useful predictive functions. Such models can be as simple as that shown in the first figure, which describes the distribution of incoming solar energy through major portions of the Earth’s systems. It’s similar to balancing the books: The sum of all components that use solar energy must equal the amount of incoming solar radiation. If they don’t add up, our model is wrong, or we’re missing something.

The general energy budget of the Earth�s outer shells, with principal input from the Sun.

Christopherson, R.W., GEOSYSTEMS: An Introduction to Physical Geography, 2nd Ed. © 1994. Reproduced by permission of Prentice Hall, Upper Saddle River, New Jersey)

` <>`__16-21: This diagram, while not constructed to explain or support the EOS program, does suggest that the various sensors in the EOS missions are all measuring aspects of the same phenomenon. What might that be? `ANSWER <Sect16_answers.html#16-21>`__

But the models we need for an Earth-system, predictive capability are much more complex than what we show here. Such models must account for energy budgets, sources and sinks of carbon and other biogeochemically related materials, effects of temperature on wind speed and direction, precipitation patterns, land use patterns, speed and direction of oceanic currents, increases in so-called greenhouse gases, and more. A full understanding of how these components interact with each other supports our willingness to trust the output from such models. We show an example of the complexity of these models, along with a color-coded indication of how EOS and other MTPE platforms contribute to a better understanding, in the figure below, which we based on the Bretherton diagram:

|Interactions between the terrestrial physical climate systems and biogeochemical systems. |

Because of the complexity of such models, we must accumulate multitudes of timely data from many different sources, over a relatively long period, by a highly advanced data and information system that ingests, processes, and distributes those data to interested parties around the world.

Based on the predictive models described above, we must make decisions based on our understanding of the potential magnitude of global change, in order for planners and policy-makers to define strategies for mitigation or adaptation. These strategies may have widely different economic and societal impact, involving health, standard of living, and quality of life. EOS studies address how climate changes affect water resources, agriculture and ecosystems, and provide fundamental data sets on land-cover change, and measures of sea level change. These EOS measurements and the resulting predictive models address such topics as marine productivity, ozone depletion, air quality, and resources monitoring. These activities give us the tools we need to understand our Earth system and its many subsystems, and to understand the role we play in modifying such systems, and the roles they play in our daily lives.

We bring to your attention another related program that will rely on a variety of satellites and sensors, and the participation of many nations, to monitor and assess aspects of the environmental that relate to natural and manmade disasters. This program is an outgrowth of agreements worked out during a May 1996 Workshop on International Cooperation in Space. We summarize the results of their recommendation to use remote sensing for this purpose in the table shown here. We’ve since added other satellites to the list, and EOS will contribute to the monitoring capabilities. (See also, the summary of satellite programs planned over the next ten years given in Section 21 [page 21-1]).

System

Status

Observation capabilities

Types of applications

Weather satellites

many existing

global day and night observations

prediction/monitoring of hurricanes, typhoons, tornadoes, volcanic eruptions

Landsat-7

operational

visual 30 m and multispectral 80 meter land observations

land use, flood extent, environmental monitoring

SPOT 1-4

operational

visual 10 to 30 m land observations

3 dimensional mapping, flood extent, damage assessment, crop identification

IRS-1C

operational

visual 6-30 m land and sea observations

3 dimensional mapping, oil spill detection, flood extent, damage assessment

RESURS-O1

operational

visual and multispectral 160-600 meter land and sea observations

regional environmental mapping, monitoring of coastal zones, crop development, drought, flood areas and fires

ERS

operational

all weather 25-500 m land and sea observations

3 dimensional mapping, oil spill detection, flood extent, damage assessment, night coverage

Radarsat

operational

all weather 10-100 m land and sea radar observations

3 dimensional mapping, oil spill detection, flood extent, damage assessment, night coverage

JERS

operational

all weather 18 m land and sea observations

3 dimensional mapping, oil spill detection, flood extent, damage assessment, night coverage

SeaWiFS

launched in 1997

multispectral 1 & 4 km sea observations

oil spill detection, ocean pollution monitoring, algae detection

Cosmos, KVR-1000

operational

visual 2 m land observations (not near-real-time)

high-resolution mapping, infrastructure identification, terrain analysis

Space Imaging IKONOS-2)

first launched in 1999

visual 1 m and multispectral 4 m land observations

high-resolution mapping, infrastructure identification, terrain analysis, crop identification

OrbView-2

launched in 1999

visual 1 & 2 m and multispectral 4 m land observations

high-resolution mapping, infrastructure identification, terrain analysis, crop identification

QuickBird-2

launched in 2001

visual 1 m land observations

high-resolution mapping, infrastructure identification, terrain analysis

SPOT 5A

launched in 2002

visual 5 m land observations

high-resolution mapping, infrastructure identification, terrain analysis, crop identification

OrbView-3

launched in 2003

visual <1 m and multispectral 4 m land observations

high-resolution mapping, infrastructure identification, terrain analysis, crop identification

Examples of images from several of the above systems are presented on page 21-2.

Now, with these eight pages of background, we can now actually see in the next two pages the first, and most impressive indeed, results from the flagship EOS satellite, Terra.


Primary Contact: Nicholas M. Short, Sr. email: nmshort@nationi.net

Dr. Mitchell K. Hobish, Consultant (mkh@sciential.com)