4
Opportunities to Improve Alignment with Decadal Survey Priorities
The inefficiencies associated with budget instability and continuing shifts in administration and congressional priorities warrant a more dynamic and robust approach to making progress on the 2007 Earth science and applications from space decadal survey vision and recommendations.1 NASA’s Earth Observing System (EOS), conceived in the 1980s and implemented in the 1990s,2 benefited from structures that existed within the NASA program that enabled senior principal investigators and engineers associated with missions and instruments to meet frequently and provide day-to-day advice to NASA managers about, for example, changes in scope and plans, new technology options, and new mission architectures. The EOS Payload Panel and Interdisciplinary Science Principal Investigators were the most visible of such groups, and their experience was built on an overall philosophy of engaging the science community and mission and instrument engineers in a coordinated way, and then using their input as a major contribution to difficult operational decisions about missions and instruments. These working groups were outside the formal broad advisory structure of the NASA Advisory Committees and the National Academies but had the benefit that they were intimately familiar with the details and overall goals of the NASA program. This committee does not see that such management structures currently exist to provide an ongoing source of broad Earth science community involvement. As a result, difficult decisions are made largely without coordinated community input, because infrequent meetings with existing high-level oversight committees cannot delve into issues at the needed level of detail.
1 The 2007 decadal survey recommended that NASA “[i]mplement a system-wide independent review process that permits decisions regarding technical capabilities, cost, and schedule to be made in the context of the overarching science objectives. Programmatic decisions on potential delays or reductions in the capabilities of a particular mission would be evaluated in light of the overall mission set and integrated requirements” (p. 11). This statement is reiterated here in the form of a recommendation. See National Research Council, Earth Science and Applications from Space: National Imperatives for the Next Decade and Beyond (The National Academies Press, Washington, D.C., 2007), which included guidance in Box 3.4 for the case of budget shortfalls.
2 See CIESIN, “EOS Program Chronology,” available at http://www.ciesin.org/docs/005-089/005-089art2.html, reproduced from NASA, Earth Observing System (EOS) Reference Handbook, G. Asrar and D.J. Dokken, eds., NASA Earth Science Support Office, Document Resource Facility, Washington, D.C., 1993.
Below are the first 10 and last 10 pages of uncorrected machine-read text (when available) of this chapter, followed by the top 30 algorithmically extracted key phrases from the chapter as a whole.
Intended to provide our own search engines and external engines with highly rich, chapter-representative searchable text on the opening pages of each chapter.
Because it is UNCORRECTED material, please consider the following text as a useful but insufficient proxy for the authoritative book pages.
Do not use for reproduction, copying, pasting, or reading; exclusively for search engines.
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4
Opportunities to Improve Alignment
with Decadal Survey Priorities
The inefficiencies associated with budget instability and continuing shifts in administration and con-
gressional priorities warrant a more dynamic and robust approach to making progress on the 2007 Earth
science and applications from space decadal survey vision and recommendations.1 NASA’s Earth Observ-
ing System (EOS), conceived in the 1980s and implemented in the 1990s,2 benefited from structures that
existed within the NASA program that enabled senior principal investigators and engineers associated with
missions and instruments to meet frequently and provide day-to-day advice to NASA managers about, for
example, changes in scope and plans, new technology options, and new mission architectures. The EOS
Payload Panel and Interdisciplinary Science Principal Investigators were the most visible of such groups,
and their experience was built on an overall philosophy of engaging the science community and mis-
sion and instrument engineers in a coordinated way, and then using their input as a major contribution
to difficult operational decisions about missions and instruments. These working groups were outside the
formal broad advisory structure of the NASA Advisory Committees and the National Academies but had
the benefit that they were intimately familiar with the details and overall goals of the NASA program. This
committee does not see that such management structures currently exist to provide an ongoing source
of broad Earth science community involvement. As a result, difficult decisions are made largely without
coordinated community input, because infrequent meetings with existing high-level oversight committees
cannot delve into issues at the needed level of detail.
The 2007 decadal survey recommended that NASA “[i]mplement a system-wide independent review process that permits decisions
1
regarding technical capabilities, cost, and schedule to be made in the context of the overarching science objectives. Programmatic
decisions on potential delays or reductions in the capabilities of a particular mission would be evaluated in light of the overall mission
set and integrated requirements” (p. 11). This statement is reiterated here in the form of a recommendation. See National Research
Council, Earth Science and Applications from Space: National Imperatives for the Next Decade and Beyond (The National Academies
Press, Washington, D.C., 2007), which included guidance in Box 3.4 for the case of budget shortfalls.
See CIESIN, “EOS Program Chronology,” available at http://www.ciesin.org/docs/005-089/005-089art2.html, reproduced from
2
NASA, Earth Observing System (EOS) Reference Handbook, G. Asrar and D.J. Dokken, eds., NASA Earth Science Support Office,
Document Resource Facility, Washington, D.C., 1993.
56
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OPPORTUNITIES TO IMPROVE ALIGNMENT WITH DECADAL SURVEY PRIORITIES 57
An overarching cross-mission science and applications coordination effort would help ensure that
programmatic decisions on potential delays or augmentations/reductions in the capabilities of a particular
mission would be evaluated in light of the overall mission set and integrated requirements rather than as
“one off” decisions.3 The science and applications coordination effort should include appropriate interac-
tion with the already-established system engineering working group4 and mission system engineering teams
to stay apprised of cross-mission areas of mutual interest5 and should be conducted in an ongoing manner
as science requirements and mission designs and costs evolve—with the participation of other agencies
and international partners/stakeholders when appropriate.
ESTABLISHING AND MANAGING MISSION COSTS
As discussed in Chapter 3, the 2007 decadal survey report put forth mission concept descriptions and
notional costs that were intended mainly to set targets for each mission that are consistent with an overall
program that is affordable while denoting the relative cost of one mission with respect to another, which
factored into mission priority and phasing.6 After release of the survey, teams were formed by NASA to
further develop each of the recommended mission concepts. Based on discussions with the director of
the Earth Science Division (ESD) and individual mission team members, the committee learned that teams
operated primarily in a “requirements-gathering” mode, unconstrained by even notional cost targets.7
Unfortunately, this approach created an atmosphere in which science requirements and scope tended to
grow, as did cost estimates.8 Furthermore, there was apparently insufficient consideration given to the ef-
fect of individual mission cost growth on the entire queue of recommended missions.
This cross-mission science and applications coordination effort could, for example, encourage studies and trades across missions
3
where synergies anticipated in the survey report might not be readily realized in the mission concepts as presented, or within avail-
able resources. Indeed, the need for further optimization was recognized by the survey authors, who stated, “The selected missions
reflect the panels’ prioritization of scientific observations but are not the result of an exhaustive examination of the trade-offs across
the entire range of potential missions. Clearly, more detailed cost estimates are needed that examine the full range of mission trade-
offs….” (National Research Council, Earth Science and Applications from Space: National Imperatives for the Next Decade and
Beyond, 2007, p. 43.)
The Earth Systematic Missions Program Office has established a systems engineering working group with representatives from
4
each center.
Science stakeholder participation in the A-Train Constellation Mission Operations Working Group is an example of such effective
5
interaction.
The decadal survey cost estimation process and purpose are described further in Box 2.3 in the 2007 report: “Nevertheless, the
6
estimates provided in this study set targets for each mission that are consistent with an overall program that is also affordable. The
panels recognize that the missions afforded under the estimated costs will be ones that respond to the main scientific requirements
articulated by the panels in Chapters 5 through 11, but not necessarily all of the desired requirements. The selected missions reflect
the panels’ prioritization of scientific observations but are not the result of an exhaustive examination of the trade-offs across the
entire range of potential missions. Clearly, more detailed cost estimates are needed that examine the full range of mission trade-offs.
Where possible within budget constraints, augmentation of the specified set of science observations with additional desired observ-
ables should be considered; however, NASA and the scientific community must avoid ‘requirements creep’ and the consequent
damaging cost growth” (National Research Council, Earth Science and Applications from Space: National Imperatives for the Next
Decade and Beyond, 2007, p. 43).
The discussion between the ESD director and the committee took place on April 28, 2011, during the committee’s first meeting
7
in Washington, D.C. Discussions with mission team members took place during the committee’s first and second meetings, the latter
of which was held on July 6-8, 2011.
The bulk of early formulation funding went directly to the science community to support “requirements gathering.” Without
8
pushback from engineering or cost experts, requirements can accumulate with minimal challenges or controversy. The sense is that
the science is paramount and, as long as the mission is far in the future, anything is considered possible. However, this approach
nurtures the development and maintenance of sometimes inappropriately high expectations and can result in untenably high costs
and high cost risk.
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58 EARTH SCIENCE AND APPLICATIONS FROM SPACE
The success of all missions is ultimately critically dependent on an end-to-end partnership between
the science team and the engineering team to ensure that an iterative process emerges that continu-
ously balances all of a mission’s constraints, both technical and programmatic. Instead of a process that
starts with gathering science requirements and then determining the resulting cost of a derived mission,
those with science, engineering, systems engineering, and cost expertise should all be involved from
the beginning. By understanding the source of various requirements, their relative priorities, and the
consequences of designing to satisfy the requirements, engineers are better able to push back if incre-
mental science requirements will drive up a mission design’s cost or risk, identifying the “knees in the
curves,” and interacting with the science stakeholder community in a productive and iterative fashion
toward development of a truly optimized design.9 By fully sensitizing all involved to the factors associ-
ated with implementing and costing a mission, this interaction can help minimize the “sticker shock”
associated with individual missions when they are handed off from the broader science community to
the mission implementers.
Early establishment of cost and schedule constraints would allow an iterative process to emerge that
could continuously balance all of the mission constraints within a known and achievable funding envelope,
leading to a more robust yet affordable implementation. This way, the team can be focused on maximiz-
ing science return on investment rather than attempting to craft a “perfect” yet unaffordable mission. The
committee found that process transparency is essential to ensure that the implementation of the decadal
survey is regarded as a community-driven effort and not one driven by local or vested interests, and thus
offers the following recommendation:
Recommendation:
• NASA’s Earth Science Division (ESD) should implement its missions via a cost-constrained ap-
proach, requiring that cost partially or fully constrain the scope of each mission such that realistic
science and applications objectives can be accomplished within a reasonable and achievable
future budget scenario.
Further, recognizing that survey-derived cost estimates are by necessity very approximate and that
subsequent, more detailed analyses may determine that all of the desired science objectives of a par-
ticular mission cannot be achieved at the estimated cost,
• NASA’s ESD should interpret the 2007 decadal survey’s estimates of mission costs as an expression
of the relative level of investment that the survey’s authoring committee believed appropriate to
advance the intended science and should apportion funds accordingly, even if all desired science
objectives for the mission might not be achieved.
To coordinate decisions regarding mission technical capabilities, cost, and schedule in the context of
overarching Earth system science and applications objectives, the committee also recommends that
• NASA’s ESD should establish a cross-mission Earth system science and engineering team to advise
NASA on execution of the broad suite of decadal survey missions within the interdisciplinary
context advocated by the decadal survey. The advisory team would assist NASA in coordinating
End-to-end system simulations performed prior to Preliminary Design Review can help to quantitatively identify the cost/benefit
9
ratios for the baseline design, as well as a range of alternatives.
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OPPORTUNITIES TO IMPROVE ALIGNMENT WITH DECADAL SURVEY PRIORITIES 59
decisions regarding mission technical capabilities, cost, and schedule in the context of overarch-
ing Earth system science and applications objectives.10,11
INTERNATIONAL PARTNERSHIPS
The roots of international partnerships and joint missions to observe Earth from space come from the
International Geophysical Year in the late 1950s. Throughout the 1960s and 1970s and peaking with the
Global Weather Experiment (GWE) and the World Weather Watch in 1979, both bilateral and multina-
tional space missions for weather, climate, and ocean observations became the norm. These international
activities are fostered by the International Council of Scientific Unions (ICSU), the World Meteorological
Organization of the United Nations, and others. NASA and other national space agencies, as well as the
National Oceanic and Atmospheric Administration (NOAA) and other national weather/climate agencies,
have decades of experience with joint space missions as well as hosting another nation’s instruments on
their spacecraft.
On June 28, 2010, President Obama issued the new National Space Policy. One of the policy’s goals
is expanded “international cooperation on mutually beneficial space activities to: broaden and extend the
benefits of space; further the peaceful use of space; and enhance collection and partnership in sharing of
space-derived information.”12 The policy further calls on departments and agencies to “identify potential
areas for international cooperation that may include … Earth science and observation; environmental
monitoring; … geospatial information products and services … disaster mitigation and relief ….”; and
other areas, as well. It further looked to “promote appropriate cost- and risk-sharing among participating
nations in international partnerships; and augment U.S. capabilities by leveraging existing and planned
space capabilities of allies and space partners.” Clearly, this policy seeks to mitigate U.S. budget shortfalls
through a non-zero-sum game, enabling increased accomplishment through international cooperation.
International joint missions, hosted instruments, shared data, and coordinated satellite constellations are
all becoming new realities. As such international cooperation spreads into all areas of Earth science it
becomes natural and essential to include significant specific international partnerships in the planning
and implementation of any Earth science and applications from space decadal survey. Several examples
of international collaborations are provided below to illustrate the variety of scopes and scales such col-
laborations can involve.
• The successful June 10, 2011, launch and orbital insertion of the Aquarius/Satélite de Aplicaciones
Científicas (SAC)-D mission to globally measure sea-surface salinity features an international partnership
between NASA and Argentina’s space agency, Comision Nacional de Actividades Espaciales (CONAE).13
The 3-year mission (the fourth of this collaboration) includes a NASA instrument, an Argentine spacecraft,
and a launch from Vandenberg Air Force Base on a Delta II launch vehicle.
The team, similar to the Payload Advisory Panel established by NASA to assist in implementation of its Earth Observing System
10
(EOS), would draw its membership from the scientists and engineers involved in the definition and execution of survey missions as
well as the nation’s scientific and engineering talent more broadly. (The Payload Advisory Panel was composed of the EOS Interdis-
ciplinary Science Investigation principal investigators and was formally charged with examining and recommending EOS payloads
to NASA based on the science requirements and priorities established by the Earth science community at large.) See NASA, Earth
Observing System (EOS) Reference Handbook, G. Asrar and D.J. Dokken, eds., NASA Earth Science Support Office, Document
Resource Facility, Washington, D.C., 1993.
The committee believes that NASA is best positioned to determine whether this advisory panel should be constituted as a Federal
11
Advisory Committee Act-compliant advisory body.
See http://www.whitehouse.gov/sites/default/files/national_space_policy_6-28-10.pdf.
12
See http://aquarius.nasa.gov/overview.html.
13
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60 EARTH SCIENCE AND APPLICATIONS FROM SPACE
• FORMOSAT-3/COSMIC, the joint Taiwan/U.S. science mission for weather, climate, space weather,
and geodetic research, was launched on April 14, 2006. The mission, which includes six identical micro-
satellites launched together on a Minotaur vehicle, currently provides thousands of daily radio occultation
profiles that yield accurate and precise information on temperature, water vapor, and electron density.14
COSMIC (Constellation Observing System for Meteorology, Ionosphere and Climate) has contributed sig-
nificantly to ionospheric, stratospheric, and tropospheric sciences and to applications for space weather,
weather prediction, and climate science.15 The FORMOSAT-7/COSMIC-2 planned joint mission (Appendix
D), however, is at risk because of a lack of NOAA funding commitment to match Taiwan’s $160 million
commitment and a similar level of support from the U.S. Air Force.
• The joint Japanese-U.S. Global Precipitation Mission (GPM)—a joint NASA/JAXA mission—is to
be launched in 2013 (Figure 4.1). For this mission Japan provides the Dual-frequency Precipitation Radar
(DPR) instrument and HII-A launch vehicle, and the United States provides the GPM Microwave Imager
(GMI) instrument, the spacecraft, and other system components. Major international partners also include
France and Canada.
• NASA and the German Aerospace Center (DLR) jointly developed the twin-satellite Gravity Recov-
ery and Climate Experiment (GRACE) mission (launched in March 2002) and are continuing to cooperate
throughout its operational phase. NASA and DLR plan to fly a GRACE follow-on continuity mission to
extend the measurement of changes in microgravity due to variability (e.g., depletion, recovery) in conti-
nental aquifers, polar ice mass changes, and so on.16
• The Initial Joint Polar System Agreement,17 made between NOAA/National Environmental Satellite,
Data, and Information Service (NESDIS) and the European Organisation for the Exploitation of Meteoro-
logical Satellites (EUMETSAT) in 1998, created the framework for two polar-orbiting satellite systems and
their respective ground systems. This agreement—whereby EUMETSAT flies the mid-morning weather and
environmental platform, and NOAA flies in the early afternoon—continues to work exceedingly well to
provide meteorological and environmental forecasting and global climate monitoring services worldwide.18
It is sustained through ongoing working groups, cross-participation in satellite meteorology, oceanography,
and climate conferences, and the dedication of a small number of individuals in the United States and
Europe. NOAA/NESDIS and EUMETSAT are working to establish the renewed Joint Polar System by 2018.19
Recent developments in bilateral and multilateral sharing of Earth remote sensing data have been
encouraging. In a continuation of its policy of open access to science data, the United States has made
Landsat data widely available, and the number of data downloads, users, and applications has increased
from thousands to millions.20 Working through the Global Climate Observing System (GCOS) and the
Committee on Earth Observations Satellites (CEOS), NASA and NOAA coordinate activities to ensure in-
ternational coordination of long-term mission planning activities and progress on issues of mutual interest.
Several agreements between NASA and NOAA with international groups will bring Japanese Global Change
See http://www.cosmic.ucar.edu/index.html.
14
See http://www.atmos-meas-tech.net/4/1077/2011/amt-4-1077-2011.html.
15
See http://www.csr.utexas.edu/grace/. The GRACE follow-on mission is a climate continuity mission called for in NASA, Respond-
16
ing to the Challenge of Climate and Environmental Change: NASA’s Plan for a Climate-Centric Architecture for Earth Observations
and Applications from Space, June 2010, available at http://science.nasa.gov/media/medialibrary/2010/07/01/Climate_Architec-
ture_Final.pdf.
See http://www.eumetsat.int/Home/Main/AboutEUMETSAT/InternationalRelations/KeyPartners/ SP_1225965119191.
17
See http://projects.osd.noaa.gov/IJPS/.
18
See http://www.eumetsat.int/Home/Main/AboutEUMETSAT/InternationalRelations/KeyPartners/ SP_1225965119191.
19
U.S. Geological Survey, “Free Landsat Scenes Go Public by the Million,” USGS Newsroom, August 20, 2009, available at http://
20
www.usgs.gov/newsroom/article.asp?ID=2293&from=rss_home.
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OPPORTUNITIES TO IMPROVE ALIGNMENT WITH DECADAL SURVEY PRIORITIES 61
FIGURE 4.1 The Dual Frequency Precipitation Radar instrument that will fly on the Global Precipitation Measurement
mission. SOURCE: Copyright © Japan Aerospace Exploration Agency.
Observation Mission-Climate (GCOM-C) and GCOM-W (water) data to the United States as well as the
EUMETSAT MetOp data. In addition, the 2007 survey’s Surface Water and Ocean Topography (SWOT) mis-
sion is being considered as a multidisciplinary cooperative international effort that builds on a long-lived
and successful U.S. and French partnership. The SWOT satellite mission will expand on previous altimetry
flights (e.g., TOPEX/Poseidon) through wide-swath altimetry technology to achieve complete coverage of
the world’s oceans and freshwater bodies with repeated high-resolution elevation measurements.21
International collaborations are well aligned with the first recommendation of the 2007 decadal survey
that “the U.S. government, working in concert with … international partners, should renew its investment
in Earth-observing systems and restore its leadership in Earth science and applications” (p. 2). As noted in
the 2011 National Research Council (NRC) report Assessment of Impediments to Interagency Collaboration
on Space and Earth Science Missions:22
See http://swot.jpl.nasa.gov/mission/.
21
National Research Council, Assessment of Impediments to Interagency Collaboration on Space and Earth Science Missions, The
22
National Academies Press, Washington, D.C., 2011.
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62 EARTH SCIENCE AND APPLICATIONS FROM SPACE
A prerequisite for a successful international collaboration is that all parties believe the collaboration is of
mutual benefit.… agreements should not be entered into lightly and should be undertaken only with a full
assessment of the inherent complexities and risks. (p. 2)
Current opportunities for new partnerships might be found, among others, with the European EarthCARE
joint European-Japanese mission that observes the climate-related interactions among cloud, radiative, and
aerosol processes; the Atmospheric Laser Doppler-Lidar Instrument (Aladin) on the Atmospheric Dynamics
Mission-Aeolus (ADM-Aeolus), with DLR for a Tandem-L InSAR mission.
Finding: NASA has made considerable efforts to secure international partnerships to meet its science
goals and operational requirements.
ALTERNATIVE PLATFORMS AND FLIGHT FORMATIONS
In addition to traditional launches on dedicated, large spacecraft, a number of promising alternative
platforms and observing strategies are emerging and being proven. These include flights on piloted23 and/
or unpiloted aircraft, hosted payloads on commercial satellites,24 small satellites, the International Space
Station, and the flight of multiple sensors in formations rather on a single bus.25 These alternative mission
concepts can offer considerable implementation flexibility.
Suborbital Campaigns
Instrument accommodation on balloons, piloted aircraft, and unpiloted aerial vehicles (UAVs) provides
a rapid and cost-effective means for proof-of-concept studies, technology maturation, or actual research/
operational use. Their utility was recognized by NASA in the first Earth Venture (EV-1) announcement of
opportunity, from which a diverse portfolio of five science investigations was selected.26
Hosted Payloads
Also referred to as secondary payloads, hosted payloads take advantage of available capacity on com-
mercial (e.g., communications) satellites to accommodate communications or science instruments. The De -
partment of Defense (DOD) has been successful in using hosted payload concepts to lower program costs.
NASA’s recently released draft solicitation for the first Earth Venture-Instruments (EV-I) calls for principal
investigators to propose instruments for hosting on platforms of opportunity, which can include commer-
cial satellites, opening the door to leveraging hosted payload capacity to advance NASA Earth science.27
Small Satellites
Small satellites, notionally those with spacecraft masses less than 500 kg,28 can enable rapid develop-
ment strategies (less than 36 months) that lower development costs. A 2000 NRC report, The Role of Small
Satellites in NASA and NOAA Earth Observation Programs, provides an analysis of the role of small satel-
See http://www.nasa.gov/mission_pages/icebridge/index.html.
23
See http://hostedpayloadalliance.org/.
24
See http://www.nasa.gov/mission_pages/a-train/a-train.html.
25
See http://www.nasa.gov/home/hqnews/2010/may/Hq_10-127_Venture_Program.html.
26
See http://essp.larc.nasa.gov/EV-I/.
27
The ~450 kg OCO (and OCO-2) and the 70 kg COSMIC satellites are examples of small satellites.
28
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OPPORTUNITIES TO IMPROVE ALIGNMENT WITH DECADAL SURVEY PRIORITIES 63
lites in Earth observation, particularly in the context of complementing (not replacing) larger missions.29
Especially when configured with single sensors, small satellite missions can add significantly to architectural
and programmatic flexibility. An emphasis on smaller platforms also potentially reduces cost through the
use of smaller and cheaper launch vehicles, including opportunities for launching multiple payloads on a
single launch vehicle, and “piggyback” launches, using excess capacity on larger launch vehicles.
International Space Station
In 2007, the Hyperspectral Imager for the Coastal Ocean (HICO) was manifested for the Japanese
Experiment Module-Exposed Facility (JEM-EF) on the International Space Station (ISS), and installed on
orbit on September 24, 2009. HICO was sponsored by the Office of Naval Research (ONR) to “develop
and operate the first Maritime Hyperspectral Imaging from space.”30 HICO was integrated and flown under
the direction of DOD’s Space Test Program. One of the HICO mission requirements was to “demonstrate
new and innovative ways to develop and build the imaging payload (reduce cost, reduce schedule).”31 The
sensor was delivered 16 months after project start and was installed within a total time of 3 years of its
proposal. HICO has since met its demonstration requirement. HICO’s implementation demonstrated that
the ISS is a viable platform for demonstrations of Earth observing technologies and Earth observations.32
(See Figure 4.2.) Another instrument scheduled for manifestation on the ISS is NASA’s Stratospheric Aerosol
and Gas Experiment III-ISS (SAGE III-ISS) to measure atmospheric ozone, water vapor, and aerosols. SAGE
III is scheduled for launch in 2014 on a SpaceX rocket from NASA Kennedy Space Center.33
Flight Formations
Formation flying can deliver multiple benefits, not the least of which is the ability to flexibly combine
(and maintain over time) multiple, synergistic, and multisensor measurement types.34 Advances in both
station-keeping ability and coordination protocols now make it possible to achieve formation flight with a
diverse set of spacecraft, whether launched simultaneously or years apart, including the large EOS observa-
tories, small satellites, and co-manifested satellites. Constellations may remain in place beyond the lifetime
of individual satellites if appropriate planning and funding remain in place. The Afternoon Constellation
(A-Train) continues to exemplify the best of international scientific cooperation and coordination35 and can
provide valuable experience, best practices, and lessons learned for future constellation efforts (e.g., poten-
tial establishment of a constellation based on the Joint Polar Satellite System, JPSS). Coordinated formation
flight efficiencies can include the synergies of complementary measurements, where the assigned degree
National Research Council, The Role of Small Satellites in NASA and NOAA Earth Observation Programs, National Academy
29
Press, Washington, D.C., 2000.
M.R. Corson (Naval Research Laboratory) and C.O. Davis, (Oregon State University), “HICO Science Mission Overview,” avail-
30
able at http://hico.coas.oregonstate.edu/publications/Davis_HICO_for%20IGARSS.pdf, p. 22.
Corson and Davis, “HICO Science Mission Overview,” p. 7.
31
See http://www.ioccg.org/sensors/Davis_HICO_IOCCG-15.pdf.
32
See http://www.nasa.gov/topics/earth/features/sage3.html.
33
Formation flight can provide a much clearer way of quantifying errors in parameter estimation and identifying major biases/flaws
34
in past data derived from single sensors. For example, the combined cloud information from CALIPSO and CloudSat has exposed
significant biases in interpretation of ISCCP (International Satellite Cloud Climatology Project) global cloudiness, the combination
of CALIPSO and CloudSat has led to a new and more accurate way of retrieving aerosol optical depth, and CALIPSO has yielded
powerful new information about polar stratospheric clouds, and so on.
See http://atrain.nasa.gov/, http://www.nasa.gov/mission_pages/a-train/a-train.html, and http://eospso.gsfc.nasa.gov/eos_observ/
35
pdf/Jan-Feb_2011_color_508.pdf.
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64 EARTH SCIENCE AND APPLICATIONS FROM SPACE
FIGURE 4.2 HICO image of the Straits of Gibraltar, December 5, 2009. SOURCE: Naval Research
Laboratory; available at http://hico.coas.oregonstate.edu/gallery/gallery-scenes.shtml.
of simultaneity is based on position within the train; train permanence (with its composition changing over
time);36 a ready mechanism for international cooperation; technology insertion, with research and opera-
tional technologies operating side by side; the avoidance of engineering complexities and management
difficulties associated with integration on a common bus; and a more agile and cost-effective replacement
of individual sensors. Also important is the role of formation flight in enabling Earth system science by
moving away from a single parameter and sensor-centric approach toward a systems approach that ties
observations together to study processes important to understanding Earth-system feedbacks.37
Finding: Alternative platforms and flight formations offer programmatic flexibility. In some cases, they
may be employed to lower the cost of meeting science objectives and/or maturing remote sensing and
in situ observing technologies.
S.W. Boland, M.D. Garcia, M. Vincent, S. Hu, P.J. Guske, and D. Crisp, “Ground Track Selection for the Orbiting Carbon Ob-
36
servatory-2 Mission,” American Geophysical Union Fall Meeting 2011, abstract #A33C-0242, American Geophysical Union, 2011.
For example, the combination of water vapor and temperature from AIRS, together with proper cloud screening tested with other
37
data, has provided insight on the strength of water vapor feedback; the combination of MODIS, AMSR-E, and CloudSat has revealed
new insights on rain-forming processes, thus exposing major biases in climate model parameterizations; and the combination of
AIRS, CloudSat, and CERES is being used to understand the sources of seasonal loss of sea ice in the Arctic.