THE VEGETATION CANOPY LIDAR MISSION

Ralph Dubayah, Bryan Blair, Jack Bufton, David Clark, Joseph JáJá, Robert Knox, Scott Luthcke, Stephen Prince, and John Weishampel

Contents:

Introduction

Scientific Rationale

Mission Description

Data Processing and Description

VCL Institutional Partners and Science Team Membership

Abstract

The Vegetation Canopy Lidar (VCL) is the first selected mission of NASA's new Earth System Science Pathfinder program. The principle goal of VCL is the characterization of the three-dimensional structure of the earth: in particular, canopy vertical and horizontal structure and land surface topography. Its primary science objectives are: landcover characterization for terrestrial ecosystem modeling, monitoring and prediction; landcover characterization for climate modeling and prediction; and, production of a global reference data set of topographic spot heights and transects. VCL will provide unique data sets for understanding important environmental issues including climatic change and variability, biotic erosion and sustainable landuse, and will dramtically improve our estimation of global biomass and carbon stocks, fractional forest cover, forest extent and condition, and provide canopy data critical for biodiversity studies. as well as for natural hazard and climate studies. Scheduled for launch in early 2000, VCL is an active lidar remote ensing system consisting of a five-beam instrument with 25 m contiguous along track resolution. The five beams are in a circular configuration 8 km across and each beam traces a separate ground track spaced 2 km apart, eventually producing 2 km coverage between 65° N and S, VCL's core measurement objectives are: (1) canopy top heights; (2) vertical distribution of intercepted surfaces (e.g. leaves and branches); (3) ground surface topographic elevations. These measurements are used to derive a variety science data products including canopy heights, canopy vertical distribution, and ground elevations gridded monthly at 1 resolution and and every 6 months at 2 km resolution, as well as a 2 km fractional forest cover product.

INTRODUCTION

The National Aeronautics and Space Administration has established the Earth System Science Pathfinder (ESSP) Program within the Office of Mission to Planet Earth (MTPE) to provide a means by which small, scientific space missions can be proposed and developed by individual investigators and their teams in response to research priorities not adequately addressed by current space missions such as those in EOS. The ESSP philosophy is to identify low-cost (less than $90M), quick-turnaround missions of limited duration that will provide data required to answer focused questions of importance to earth system science. As such, the ESSP program has been described as another tool among those in the existing NASA observational tool kit for improved understanding and comprehension of the components and interactions of the Earth system. The ESSP program is on-going and anticipates yearly mission launches.

In response to this opportunity, the Vegetation Canopy Lidar (VCL) mission was proposed by the University of Maryland, College Park, NASA Goddard Space Flight Center, and other university and industrial collaborators, to collect canopy and topography landcover data critical for terrestrial ecology and climate studies. In spring of 1997, VCL was selected as the first ESSP mission at a total cost of $59.8 M to NASA, along with the second mission, the Gravity Recovery and Climate Experiment (GRACE).

Mission Overview

The priniciple goal of the Vegetation Canopy Lidar is the characterization of the three-dimensional structure of the earth: in particular, canopy vertical and horizontal structure and land surface topography. The VCL mission has two main science objectives:

I. Landcover characterization for:
(a) terrestrial ecosystem modeling and prediction; and,
(b) climate modeling and prediction.
II. Global reference data set of topographic spot heights and transects.

The datasets derived from the laser altimetry instrument will make a unique and catalytic contribution to pressing environmental issues -- climatic change and variability, biotic erosion and sustainable landuse, and should dramtically improve our estimation of global biomass and carbon stocks, fractional forest cover, forest extent and condition, and provide canopy data critical for biodiversity studies. In addition, through its characterization of land surface canopy and topographic structure, VCL provides new knowledge of biophyscial parameters critical for climate, hydrologic, and other global modeling activities, activities that are essential for our ability to plan and predict for global change in the next century. Lastly, VCL provides a dense, global network of accurate topographic heights, including sub-canopy topography, data which are invaluable for future topographic missions, as well as for natural hazard and climate studies.

VCL is an active remote sensing system built around the Multi-Beam Laser Altimeter (MBLA), a five-beam instrument with 25 m contiguous along track resolution. The five beams are in a circular configuration 8 km across and each beam traces a separate ground track spaced 2 km apart, eventually producing 2 km coverage between 65° N and S, with orbit crossovers producing a denser grid away from the equator.

VCL's core measurement objectives are:
(1) canopy top heights;
(2) vertical distribution of intercepted surfaces (e.g. leaves and branches);
(3) ground surface topographic elevations.
VCL measurements are used to derive a variety science data products including canopy heights, canopy vertical distribution, and ground elevations gridded monthly at 1° resolution and and every 6 months at 2 km resolution, as well as a 2 km fractional forest cover product. These products are created at the VCL Data Center at the University of Maryland and archived and distributed through a collaboration with the EROS Data Center.

Motivation

The primary focus of the VCL mission is to provide quantitative description of landcover and global productivity, one of five science priorities of MTPE (Harris et al., 1996). Landcover change or dynamics is directly linked to several important environmental issues, including climatic change and variability, biotic erosion (loss of biodiversity), and sustainable landuse. Landcover is a first order component of general circulation models. Its status and dynamics have a direct feedbacck on the climate system by determining the boundary conditions of the exchange of momentum, energy and mass between the atmosphere and the land. Landcover also exerts an indirect or trace gas feedback because it represents a significant and dynamic pool in the carbon cycle. Similarly, landcover dynamics are the principal driver of biotic erosion. It is changes in landcover structure and composition that in turn, determines changes in habitat suitability. Any predictive understanding of biotic erosion, a necessary prerequisite for slowing and reversing that loss, will be underpinned by a quantitative comprehension and representation of current landcover status and the regime of disturbance by landuse.

For understanding and managing these environmental issues, there is a prerequisite for describing landcover status and dynamics to initialize, parameterize and validate modeling efforts. This description is required in many forms. To represent landcover in models of the climate system, it must be first be parameterized with respect to albedo, aerodynamic roughness, and surface resistance to evaporation, among others; these parameters being functions of vegetation structure, e.g. height, canopy closure, and leaf-area index (LAI), and composition (annual/ perennial, etc.). Similarly, for biogeochemical modeling, biotic erosion, and land degradation, the vegetation component of landcover must be represented in structural terms (biomass) and by composition (annual/perennial, woody/non-woody, and their age structures).

These arguments are not new. Indeed, they have justified the significant efforts by the global remote sensing community to better characterize the global land surface. The principal data source thus far for these efforts has been that from the AVHRR instrument of the NOAA spacecraft series, e.g. the NASA AVHRR Pathfinder Program. The ISLSCP Initiative (Sellers et al. 1995) is one example of the intensive use of existing data to parameterize landcover for modeling purposes. While these AVHRR-derived datasets represent a significant contribution, there remains considerable uncertainty associated with the estimated parameters. For example, important parameters such as height, LAI, woody biomass, aerodynamic roughness, and surface resistance are poorly estimated by existing methods using AVHRR data alone. Nor will any of the EOS-suite of instruments provide the requisite observations of these variables. However, given an independent and systematic sampling of vegetation based on laser returns, global data sets can be developed that will provide much improved estimates of critical variables such as canopy height, aerodnamic roughness and biomass. Furthermore, the recovery of explicit vegetation structure should provide new insight into traditional measures of surface reflectance and structure, obtained from passive remote sensing instruments, such as NDVI, LAI, BRDF, thereby extending the usefulness of the existing and planned remote sensing archive.

VCL also provides a near-global dense reference network of height transects including sub-canopy topography. The importance of accurate topographic data for global change and earth system science is increasingly being recognized, as evidenced by efforts to assimilate global topographic data, declassify defense digital elevation data, and the creation of new technologies for accurate mapping (such as GPS and interferometric SAR). This data set should prove invaluable for calibration and registration of data from future topographic missions, such as the Shuttle Radar Topography Mapper (SRTM), as well as providing detailed information on topographic roughness and scaling.

SCIENTIFIC RATIONALE

Forests comprise 29% of the world's terrestrial sruface and, as indication by the seasonal changes in atmospheric CO2 (Denning et al. 1995), these systems represent key dynamic components in the global carbon cycle. Besides harboring the bulk of the Earth's biodiversity (Erwin 1995), forest canopies are the primary interfce between terrestrial ecosystems and the atmosphere, accounting for greater than 50% of the annual CO2 flux (Potter et al 1993). Knowledge of canopy structure is required for modeling processes such as photosynthesis, energy transfer, and evapotranspiration at local to global scales.

Heretofore, the lack of broad scale data on vegetation morphology has limited the implementation of canopy-related processes into earth system models (Asrar and Dozier 1994), and is a priority for earth system science. Our crude knowledge about fundamental landcover characteristics, especially their vertical and horizontal structure and gradients, is remarkable given the level of sophistication and complexity of many global modeling activities that rely on this data. DeFries et al. (1995) have outlined the weaknesses of current landcover schemes in their discreet mapping of the land surface characteristics required to calculate land surface parameters such as absorbed radiation, albedo, canopy conductance, roughness, photsynthesis, transpiration, net primary production, carbon and nutrient dynamics. Although further development and refinement of the passive remote sensing techniques generally used for such characterization may provide some improvement, truly dramatic gains may be realized only with the advent of active remote sensing systems, such as laser altimetry, which directly measure surface structure

Landcover characterization for terrestrial ecosystem modeling and prediction

Landcover characterization for climate modeling

Direct measurements of canopy height, canopy vertical and spatial structure, and ground topography would allow determination of landcover properties critical to GCMs, SVATs and mesoscale models, whether used for climate modeling or numerical weather forecasting. There have been efforts to include complex land surface parameterization schemes both on-line and off-line in these models, as well as to understand the effects of various schemes on model outputs (e.g. see the Project for Intercomparison of Landsurface Parameterization Schemes - PILPS - activities). The determination of bulk aerodynamic parameters that control the transfer of energy, mass and momentum between the atmosphere and the surface, roughness length, zero-plane displacement, and canopy and ground resistances, is generally regarded as a major source of uncertainty. For example, in SiB2 (Sellers et al. 1996) 1 @times@ 1 maps of the bulk aerodynamic parameters are found by first using a global landcover classification. Mean values of eight canopy and ground morphological and physical parameters (canopy top height, canopy base height, ground roughness length, leaf-area density inflection height, leaf width and length, leaf-angle distribution factor and leaf area index) are assigned from the literature based on landcover type. These variables are then used with estimates of LAI from satellite data to derive the bulk parameters at 1 @times@ 1 spatial resolution. This procedure can only be seen as inadequate given the sparsity of literature values for canopy variables and their gross spatial and categorical generalization.

In contrast VCL would provide direct measurements of canopy top height, canopy base height, sub-canopy ground roughness length, and vertical density of interceptors (woody and non-woody). Maps of these variables would then be available globally, and gridded to a resolution as fine as 2 km @times@ 2 km. These can then be used to derive the bulk aerodynamic parameters at accuracies and spatial extents never before possible, with a resultant improvement in our ability to model momentum, water vapor and sensible heat fluxes. In addition, a global data base of canopy structure, especially when combined with other remote sensing data, such as greeness indices from MODIS, should enhance our ability to model the interaction of energy with the surface via better estimates of LAI and FPAR (fractional absorbed photosynthetically active radiation), as well as the interaction of precipitation with the surface through interception and retention, with resulting improvements in model photosynthesis, net primary production, trace gas and hydrologic fluxes.

Globally distributed topographic control points

The strong scientifc need for accurate, global topographic data bases has led to recent progress in limited release of portions of the Defense Mapping Agency Digital Terrain Elevation Data (DTED) Level 1 data that has 90 spatial (horizontal) pixel resolution and 16 m vertical accuracy. Despite this progress the scientific benefit for global MTPE studies is not nearly realized. The existing DTED Level 1 data will not be released for the entire Earth and space-based imaging sensors now in orbit and planned in the EOS-AM1 era (1998-2003) require global topography at DTED Level 2 (30 m spatial, 16 m vertical) for full realization of their science potential in land cover/global productivity, short-term climate modeling, and natural hazard studies. The Shuttle Radar Topography Mission (SRTM) has been announced to address these needs. Since IFSAR data, or the conventional photogrammetric data sets, are only relative in their measurement of surface elevation, direct measurements are needed to "control" the vertical dimension of the topographic image. Estimates of TCPs needed for a global DTED Level 2 are well in excess of 100,000,000. Only a limited number of these TCPs can be provided by ground-based radar targets and GPS receivers, the remainder will have to be estimated from existing maps and digital elevation models that do not routinely achieve the 1 meter level of vertical accuracy and do not have a common reference frame. The VCL surface elevation measurements will have a common, global reference frame and are "direct" rather than inferred. Furthermore, only VCL will address the vegetation cover issues that limit all present mapping techniques to tens-of-meters rms in forested areas. The VCL Mission, by virtue of its primary vegetation canopy measurements, will provide billions of sub-canopy surface elevation points.

MISSION DESCRIPTION

VCL is scheduled for launch in early 2000 on board a Pegasus XL launch vehicle. The VCL mission will be conducted by means of a small satellite carrying the MBLA instrument in a 400 km orbit of 65° inclination with a two-year nominal lifetime. This will provide sufficient coverage of the Earth to characterize the vegetation canopy structure on a global basis during two complete growing seasons and produce a global reference grid of land topography. Because of increased atmospheric drag caused by the solar maximum during the mission, monthly reboosts are required to maintain nominal orbital altitude. Command and control of the spacecraft during operation, as well as data processing will take place at the University of Maryland. Distribution and archiving of VCL data products will be performed by the EROS Data Center. Table 1 lists VCL data characteristics and quality.

VCL visits, on average, the same 1 cell at the equator every two weeks, with more frequent revisits away from the equator. The exact ground track through any cell is essentially random, being a function of orbital drag and the monthly reboost required to keep the satellite at altitude. The number of visits to a 2 km cell, globally averaged over all cells, is approximately 10 during the two-year mission (with more frequent visits away from the equator, and less frequent visits at the equator).

Measurement Objectives and Requirements

To address its major science goals, the VCL mission has 3 direct measurement objectives listed above, all at sub-meter vertical accuracies: (1) canopy top height; (2) the vertical distribution of nadir intercepted surfaces; and, (3) surface topography elevation, including sub-canopy topography.

VCL science goals place further constraints on the measurements, achieved through sensor design, orbit configuration and mission lifetime. Among these constraints are: laser footprint of 25 m to adequately resolve vegetation height and structure; continuous along track returns to adequately characterize horizontal spatial variability and vertical height distributions; 5 beams separated by 2 km across-track spacing to achieve sufficient global sampling and exact positioning and pointing; precessing, inclined orbital configuration such that the sensor passes within the same 1 @times@ 1 block along the equator every two weeks, allowing for (a) seasonal refresh of canopy structure and, (b) global 2 km coverage every 6 months, minimizing the effects of clouds.

Canopy measurements are achieved through analysis of laser pulse returns (waveforms) and require that return signals include the canopy top, adjacent structural elements and, eventually, the underlying ground. Waveform analyses based on extensive airborne and spaceborne laser altimetry have revealed the need for footprint sizes on the order of 1 to 2 canopy diameters. This guarantees a resulting reflection from the very top of each canopy within the sampled area as well as sufficient intra- and inter-tree gaps required to image the underlying ground. Dynamic range in the receiver as well as sufficient laser output energy are required to detect small ( < 1%) weighted returns from the canopy top and, in dense canopies, the underlying ground. So, potentially, even the most dense canopies still reveal their heights and sub-canopy topography. Smaller footprints under-represent the canopy structure especially with respect to true height. This results from the reduced probability of sampling the top of the canopy: smaller footprints most often hit the shoulders of the canopy. Conversely, with larger footprints (beyond a few tens of meters), similar to those proposed for space-borne missions of the future, such as the Geoscience Laser Altimeter Sensor (GLAS) and Shuttle Laser Altimeter (SLA) series, the precent of the total return that is contributed by the canopy top is greatly reduced making height measurement inaccurate.

The footprint size selected for VCL will be especially suitable for high biomass tropical forests where canopy diameters can reach 10 to 25 m. The medium size footprint of VCL also reduces any surface slope spreading of the ground return, most notably in the case where the surface slope, canopy height, and canopy thickness combine to convolve the canopy return with the ground return.

A 65° orbital inclination was selected to provide near-complete coverage of vegetation areas of interest. Such an inclination samples 98% of closed canopy forest, and gives at least 92% coverage for all the major types of close-canopy forest, and at least 89% for all but one type of open woodland.

The orbit and 2 km beam spacing allows VCL to cover the entire earth between 65 N and S in less than 6 months, so that over an 18 month mission VCL will visit the same general 2 km @times@ 2 km area 3-4 times near the equator (with higher repeats at higher latitudes). Cloud probability studies have shown that this leads to a 85-90% chance of obtaining at least one clear pass through the area.

VCL acquires data 10 times over an average 2 km @times@ 2 km cell during a 2 year mission, accumulating 19.1 km lf laser ground tracks. This samples 9.4% of an average cell's area, or after adjusting for cloud cover, 4.7% of the land area between 65° N and S. VCL's mission duration is driven by requirements for coverage in the tropics, where there are the greatest uncertainties in present land cover data. The more frequent coverage where orbital paths converge at higher latitudes yields measurements of canopy heights and median intercepts during the summer growing season, even where deciduous trees are in leaf for but a few months a year.

Baseline Instrumentation

The MBLA is comprised of five laser transmitters in a single altimeter instrument. Each laser beam operates at the 1064 nm fundamental wavelength of the neodymium-doped yttrium aluminum garnet (Nd:YAG) solid-state laser, are arranged in a pentagon inside a 20 mrad telescope circular field-of-view that is centered on nadir as illustrated in Figure 3.

Figure 3 . VCL mission concept.

The optical telescope is 0.9 m in diameter composed of beryllium. For the VCL orbital altitude of 400 km the across-track separation between adjacent tracks is 2 km. VCL makes simultaneous measurements of range to the surface by synchronous triggering of the 5 laser pulse transmitters and detection with a single telescope that is staring at nadir and is equipped with multiple silicon avalanche photo diode detectors in its focal plane. Individual laser footprints are 25 m in diameter and are contiguous along-track, commensurate with the best DTED Level 2 topography mapping resolution and LANDSAT Thematic Mapper pixel resolution. Surface echoes from the 5 beams are digitized in the MBLA electronics at 250 Megasamples per sec to achieve the required sub-meter vertical resolution in the vegetation canopy and permit pulse centroid correction of the range measurement.

The MBLA pulsed laser transmitter modules are based on high power Nd:YAG and employ the Q-switching technique to concentrate laser energy in a short pulse. Each of these laser modules produces a laser pulse of 5 nsec duration at the rate of 290 pps. Laser pulse energy of 10 mJ per pulse will be sufficient to establish a link performance for the MBLA instrument that results in 95% probability of detection of the Earth's surface under clear atmospheric conditions and permits surface lidar investigations.

DATA PROCESSING AND DISTRIBUTION

The ultimate goal of the VCL project is to produce quality data products that the science community may use to answer the scientific questions posed earlier. The VCL data processing and distribution plan assures the quality of final data products and their timely release. There are several pre-launch elements of this plan including: calibration and validation activities to assist in algorithm development and data quality evaluation; precision orbit determination strategy for VCL; laser waveform processing algorithm development; in partnership with EROS data center, development of web sites, interfaces, distribution, archiving, data and metadata structures and other protocols. Post-launch, all data processing is done at the VCL Data Processing Center (VDC) and the University of Maryland. During the first 6 months after on-orbit check-out, calibration and validation activities confirm data quality, after which the frist Level 1B through Level 3 data products will be available on-line from VDC and transferred to EDC for archiving and distribution.

VCL Data Products

There are two basic types of data products delivered by VCL: gridded and ungridded (Table 2). The ungridded data products are the along-track, contiguous footprint observations. The ungridded data products consist of calibrated waveforms and ranges, should users wish to derive their own parameters from the lidar measurements (Level 1B), and data products derived from these (Level 2), but using VCL developed algorithms. These Level 2 products consist of geolocated measurements of canopy top heights, ground height, and the vertical distribution of intercepted surfaces.

VCL will provide products gridded at two different spatial and temporal resolutions: 1 , monthly products and 2 km, 6 monthly products, these time periods a function of the revisit times to any particular cell for the given spatial resolution. During a one month period, VCL will visit a 1 grid cell at the equator twice (with more frequent visits away from the equator). Every month the derived Level 2 parameters accumulated for a cell will be gridded and released as Level 3 products (see Table 1). Similarly, every 6 months the accumulated Level 2 data for a particular 2 km grid cell will be gridded and released as a Level 3 product, the longer time period being needed to accumulate enough returns for the smaller area. An additional Level 3 data set, 2 km fractional forest cover. will also be derived from these observations. Every 6 months these 2 km grids will be updated with the accumulated returns.

Table 1.
VCL Data Characteristics and Quality
Swath width8 km
Number of beam tracks5
Footprint (at 400 km)25 m (60 @ mu @rad)
Footprint spacingcontiguous over land (approx)
Track spacing2 km
Pulses per second290 over land (approx.)
Wavelength1064 nanometer
Coveragebetween 65 eg N and S
Elevation accuracy< 1 m in low slope terrain
Waveform digitization 250 Megasamples/sec
Samples per waveform10-200, average=50
Sample precision10 bits
Pulse detection dynamic range100:1

Table 2.
VCL Data Set Levels and Descriptions


LevelDescriptionEstimated Data Volume
0Uncompressed instrument data 5.0 Gb/day
1AOrbital, calibration and time parameters inserted 5.0 Gb/day
1BCalibrated waveforms and ranges6.0 Gb/day
2Geolocated canopy top heights0.5 Gb/day
Geolocated vertical distribution of intercepted surfaces6.0 Gb/day
Geolocated ground heights (including sub-canopy) 0.5 Gb/day
3Gridded mean canopy top height and variances (1 deg by 1 deg) 0.4 MB/month
Gridded median height of intercepted surfaces (1 deg by 1 deg)0.2 MB/month
Gridded mean ground height and variances (1 deg by 1 deg) 0.4 MB/month
Gridded mean canopy top height and variances (2 km)130 MB/6 months
Gridded median height of intercepted surfaces (2 km) 65 MB/6 months
Gridded mean ground height and variances (2 km)130 MB/6 months
Gridded fractional forest cover (2 km)32 MB/6 months

Calbration and Validation Activities

The VCL science team (see below) has primary responsibility for calibration of algorithms for extracting geophysical fields, for validation of the results, and for assuring the accuracy and quality of the science data products.

Calibration.
Calibration of ground height measurements requires on-orbit bias and drift retrievals. These are obtained through comparisons with results from the TOPEX/POSEIDON altimeter at ocean orbital crossover points between VCL and TOPEX/POSEIDON, as well as comparisons of VCL ocean altimetry with high resolution mean sea surface elevation maps.

Calibrating canopy top heights.
Before launch, the science team will develop and unambiguous calibration relating an extreme percentile fo the canopy return (e.g. the first 2%) and the most widely encuntered definition of stand height (the average of top heights for plants forming the canopy, i.e. the dominant and codominant tress in forests). We will test whether the same percentile and calibration coefficient can be used for canopies with markedly different crown forms. To help with this assessment ee will acquire aircraft data with the Laser Vegetation Imaging Sensor (LVIS) instrument (Blair et al. 1996), configured as a VCL simulator over a variety of forest types including moist tropical forests, deciduous and mixed conifer, and open woodland, among others.

Validation.
Validation has three components: comparing results from aircraft data with localized ground data, comparing VCL data products with aricraft data for the same areas, and comparing gridded products with data from global site networks. The combination allows us to scale from small field plot data to landscape-level estimates, an then to gridded products from VCL. Alogrithms for Level 2 products are validated by compariso with groudn data. Level 1 and Level 3 products are validated by comparing them with aircraft data and landscape estimates from aircraft data, respectively. Global Level 3 products are cehced against several distributed data sources.

VCL Institutional Partners and Science Team Membership

VCL was conceived and executed as a collaboration among various university, federal agency, and private industrial partners. Such a collaboration is neccesitated through the "Principal Investigator" mode required by the ESSP program, where the PI and mission team are solely responsible for all aspects of the mission from engineering design, construction, launch, and ground systems, to processing, archiving and release of final data products. The VCL partners and their roles are given in Table 3. The great advantage of PI-mode is that allows a mission team great flexibility to design and implement a mission in efficient and novel ways with limited NASA direction, and thus represents a radically "new way of doing business" for the space agency. NASA provides oversight of the project through the valuable efforts of the ESSP project office.

Table 3.
VCL institutional partners.
InstitutionRole
University of Maryland, College Park PI institution and prime contractor, Science Team, data processing
Laboratory for Terrestrial Physics, NASA Goddard Space Flight Center Instrument, alogorithms, orbits, Science Team
CTA Space SystemsSpacecraft bus
Omitron, IncProject management, ground systems
Fibretek, IncInstrument lasers
University of Central FloridaScience Team
University of Missouri - St. LouisScience Team

As required by the ESSP program, a VCL Science team was formed prior to mission selection. The VCL Science Team is responsible for developing science requirements for the instrument, developing and implementing calibration and validation plans, developing science algorithms, implementing and monitoring science outreach, evaluating data products and ensuring their timely release. Table 4 lists science team members and their roles in the mission.

It is important to note that the VCL Science Team does not directly attempt to meet any of the science objectives of the mission, nor do they receive any funding to do so; rather, each member's participation is focused solely on some aspect of the production of VCL data sets. Through its Science Development and Analysis Program (SDAP), NASA plans to competitively fund research projects proposed by members of the scientific community that make use of data from ESSP missions to answer the questions posed by particular project(s). The use of VCL observations for estimating global biomass and carbon reserves would be one example of an investigation properly funded by the SDAP program.

Table 4.
Science team membership and responsibilities.
MemberInstitutionRole
Ralph DubayahUniversity of MarylandPrincipal Investigator, Cal/val
J. Bryan BlairNASA GSFCAlogrithm development, LVIS, cal/val
Jack L. BuftonNASA GSFCMBLA instrument
David B. ClarkUniversity of Missouri - St. LouisCal/val
Robert G. KnoxNASA GSFCCal/val coordinator
Scott LuthkeNASA GSFCPrecision orbit determination
Stephen PrinceUniversity of MarylandCal/val
John WeishampelUniversity of Central FloridaCal/val

SUMMARY

The Vegetation Canopy Lidar will be a key instrument in the EOS-era of earth observation. Its 5-beam, active remote sensing system will provide unprecedented information on the structure of the Earth's forests and land surfaces, directly observing vegetation canopy height, forest vertical and spatial distriubtion, and ground topography at high resolution. In its two year mission VCL will acquire billions of cloud-free observations that will prove invaluable for estimating the current status and dynamics of the earth's landcover and topography in structural terms never before possible, and the implications of these for biophysical and climatological processes. When fully integrated with observations expected from other EOS-era sensors, these data should revolutionize our perspective and understanding on the role of the land surface as part of the earth system, and the effects of human activites therein.

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