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Our Earth is unique among the planets with an abundance of water and highly diversified life. Its land, atmosphere, oceans, and all forms of life interact in many complex ways to form a complex Earth system. NASA provides a unique vantage point from space that is the only way to effectively study global scale phenomena and to understand local, regional and global-scale changes in their larger context. The mission of NASAs Earth Science Enterprise (ESE) is to develop a scientific understanding of the Earth system and its response to natural and human-induced changes to enable improved prediction of climate, weather, and natural hazards for present and future generations. ESE has three major goals:
ESE Research Strategy How is the Earth changing and what are the consequences for life on Earth? In and of itself, this question is very difficult to answer, so NASAs ESE has come up with five more specific questions designed to look at different aspects of the broader question:
Undergirding each of these are even more specific questions (totaling 23) that drive requirements for new research tasks and new remote sensing and in-situ observations to be satisfied by satellites, suborbital and surface-based observing systems. |
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![]() The Advanced Land Imager (ALI) on board the EO-1 spacecraft obtained this image of South Africas Kruger National Park. ALI produces images comparable to Landsat, continuing its long-standing data record at a fraction of the cost. | |||
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ESE Applications Strategy next: Missions |
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ESE Mission Programs The Earth Observing System (EOS) was created primarily to meet the need for systematic measurements, and is the largest component of the ESE. It aims to carry NASAs legacy of focused Earth Science measurements into a new era of comprehensive data sets, leading to an improved understanding of the Earth as a complete global system. EOS is managed by the Goddard Space Flight Center, with important contributions from other NASA centers: Jet Propulsion Laboratory, Langley Research Center, Marshall Space Flight Center, Wallops Flight Facility, and Stennis Space Center. In addition, NASA works in conjunction with many other partners from government, industry, academia, and with international space agencies.
Twelve missions are planned as part of the EOS program and already NASA has launched six EOS spacecraft. These include the Quik Scatterometer (QuikScat), the Active Cavity Radiometer Irradiance Monitor Satellite (ACRIMSAT), the third Stratospheric Aerosol and Gas Experiment (SAGE III - Meteor 3M), Landsat 7, Jason-1, Terra and Aqua. Terra launched in December 1999 and is the flagship of the EOS program. It is a joint mission with Japan and Canada that carried five advanced instruments into orbit to study land and ocean surfaces, sea surface temperature, cloud patterns, small atmospheric particles called aerosols, and the balance of solar energy absorbed and reflected by Earth. The most recent launch was that of Aqua, in May 2002. Aqua carries a synergistic instrument payload and is designed to observe how moisture cycles between Earth's lithosphere (land), hydrosphere (water), atmosphere (air), and cryosphere (ice). This is a very busy year for the EOS program with two additional launches planned. The Solar Radiance and Climate Experiment (SORCE) will make daily measurements of total solar irradiance and spectral solar irradiance between wavelengths of 1 nm and 2000 nm, and the Ice, Clouds and Land Elevation Satellite (ICESat) will measure precisely the elevations of Earth's ice sheets and cloud and aerosol layers in the atmosphere. Aura, the third major EOS mission, is scheduled to launch in 2004 and will carry a suite of instruments that will study the complex chemistry of the atmosphere. The Earth System Science Pathfinder (ESSP) program is the primary source of exploratory missions to complement EOS. These are smaller and cheaper missions proposed by the scientific community to address specific research questions and they are developed and implemented on a faster schedule. They are competitively selected and led from development through data distribution by a Principal Investigator.
The first ESSP mission is the Gravity Recovery and Climate Experiment (GRACE) launched in March 2002. Two satellites fly in formation, linked by a microwave ranging instrument and obtain the most precise measurements of the gravity field that have been obtained to date. Many scientific disciplines eagerly await advances that should derive from these data. A second launch in 2004 will deploy two more ESSP satellites CloudSat and CALIPSO. CloudSat is a satellite experiment designed to measure the vertical structure of clouds from space, which will contribute to better predictions of clouds and effects of clouds on Earth radiation. The Cloud Aerosol Lidar and Infrared Pathfinder Satellite Observer (CALIPSO) will profile the atmosphere using lidar and provide a global set of data on aerosol and cloud properties, radiative fluxes, and atmospheric state. These two spacecraft will fly in formation with Aqua and Aura; the resulting measurements will be intercomparable and will greatly improve our ability to predict future climate change. The Vegetation Canopy Lidar (VCL) whose principal mission is the characterization of the three-dimensional structure of the Earths forest canopy and a global reference data set of topographic heights and transects is currently being pursued as a technology demonstration. A decision is pending on whether to proceed with a satellite mission.
The New Millennium Program (NMP) is the principal source of technology demonstration/operational precursor missions. NMP serves as a testbed for the development of cutting edge technology for future Earth science instruments and spacecraft. The first NMP mission, Earth Observing-1 (EO-1), was launched in November 2000. EO-1 carries an Advanced Land Imager designed to continue the measurements made by the Landsat series at a much lower cost and using an instrument that is four to five times smaller than the Enhanced Thematic Mapper Plus (ETM+) instrument on Landsat. Meanwhile, the Hyperion instrument onboard EO-1 tests hyperspectral imaging techniques that can split the signal returned from the surface into hundreds of separate wavelength bands, an order of magnitude improvement in resolution over Landsat. EO-1 is flying in formation with Landsat and Terra so that their observations can easily be compared, making them a physical emblem of the best in remote sensing satellites of today, tomorrow and for decades to come. Another planned NMP mission is the Geosynchronous Imaging Fourier Transform Spectrometer (GIFTS) developed at NASA Langley Research Center. GIFTS will allow tracking of the movement of water vapor through the atmosphere in all three spatial dimensions. GIFTS is scheduled to launch in 2005 and will give scientists the ability to observe the space and time distribution of temperature, water vapor, and wind, which will improve weather forecasting. next: Data and Information System |
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ESE Data and Information System Services The Earth Observing System Data and Information System (EOSDIS) has been handling existing data sets since 1994. It began working with raw satellite data following the launch of the Tropical Rainfall Monitoring Mission (TRMM) in November 1997. The system also manages data from other satellites such as Landsat 7 and Terra and provides command and control functions for Terra. EOSDIS works in tandem with NASAs primary satellite network, the Tracking and Data Relay Satellite System (TDRSS), and eight major remote sites called Distributed Active Archive Centers (DAACs), each of which specializes in serving a particular scientific discipline. Scientific products for Terra are being generated in partnership with the missions principal investigators and their home institutions. This trend will grow with future EOS missions and competitive selections of creative data processing proposals from universities and commercial providers. EOSDIS is accessible to scientists as well as the general public. It is based on an open architecture that can be updated as computer technology improves and research questions evolve over the coming decades.
The Federation of Earth Science Information Partners (ESIPs) was created in 1998 as an experiment in developing a federated system for data management. The notion was that this should be a decentralized, heterogeneous and distributed data and information system taking EOSDIS data to the next step by generating products tailored by and for specific uses in society. The ESIPs combine their collective resources (data, technology, knowledge and education) to increase the quality and widen the usage of Earth science data and create new interoperability tools for Earth data resources. They work to make it increasingly practical for end-users of Earth Science data to access information without having to navigate through a maze of data and cataloging issues. NASA hopes to incorporate many of the lessons learned and technologies developed through the ESIP Federation as it begins to plan the Strategic Evolution of ESE Data Systems a project known as SEEDS. Capitalizing on the assets developed by EOSDIS and the ESIP Federation, as well as emerging information technology, ESE will evolve its data and information system and services both to handle data from future missions and to involve and serve a broader range of information suppliers and users. ESE Advanced Technology Program next: Partnerships |
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ESE Partnerships ESE Education Programs
NASA also has a vested interest in training the next generation of scientists. The Graduate Student Fellowship Program sponsors 50 new graduate students each year to conduct new research. The New Investigator Program does the same for those who recently received their doctoral degrees. ESE is working on professional education projects to help meet the growing demand in the workforce for people capable of using remote sensing data and geographic information systems. next: Introduction |
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