The Collier Report of U.S. Government Contracting

Sampling of Federal Government Funding Actions/Set Asides

In order by amount of set aside monies.

• $95,527 - Wednesday the 16th of September 2015
  National Aeronautics And Space Administration
  NASA SHARED SERVICES CENTER
  LOW-ALTITUDE ELECTRON DENSITIES ARE A KEY BOUNDARY CONDITION FOR SATURN IONOSPHERIC MODELS, AS THEY OCCUR IN A REGION OF COMPLEX CHEMISTRY AND POSSIBLY STRONG DYNAMICS. IN ADDITION, THE BULK OF IONOSPHERIC PEDERSEN CONDUCTIVITY - AN IMPORTANT PARAMETER FOR COUPLING TO THE SATURN MAGNETOSPHERE - IS GENERATED WITHIN THIS ALTITUDE REGION. NEVERTHELESS, DUE TO MULTIPATH PROPAGATION ISSUES THAT RESULT FROM THE HIGH DEGREE OF VERTICAL STRUCTURING IN SATURN'S IONOSPHERE, LOW-ALTITUDE ELECTRON DENSITIES REMAIN LARGELY UNREPORTED. DIURNAL VARIATIONS IN ELECTRON DENSITY WITHIN AN IONOSPHERE PROVIDE ANOTHER IMPORTANT CONSTRAINT FOR MODELERS, AS THEY LIMIT THE POSSIBLE CHEMICAL AND TRANSPORT TIMESCALES. RADIO OCCULTATION MEASUREMENTS PROVIDE PROFILES IN ALTITUDE OF ELECTRON DENSITY, BUT ARE LIMITED TO SATURN DAWN AND DUSK. CONVERSELY, SATURN ELECTROSTATIC DISCHARGE (SED) MEASUREMENTS REVEAL ONLY THE PEAK ELECTRON DENSITY, BUT ARE ABLE TO TRACK THE VARIATION OF PEAK ELECTRON DENSITY THROUGHOUT THE ENTIRE SATURN DAY. THEREFORE, COMBINING BOTH MEASUREMENTS IS VITAL TO UNDERSTANDING SATURN'S IONOSPHERE. WE PROPOSE TO BETTER CONSTRAIN THE SATURN IONOSPHERE THROUGH ADDITIONAL ANALYSES OF TWO CASSINI INSTRUMENT DATASETS: LOW-ALTITUDE RADIO OCCULTATION MEASUREMENTS FROM THE RADIO SCIENCE SUBSYSTEM (RSS), AND SED MEASUREMENTS FROM THE CASSINI RADIO AND PLASMA SCIENCE (RPWS). IN ADDITION, IN ORDER TO LINK OUR ANALYSES, WE WILL USE THE SATURN THERMOSPHERE-IONOSPHERE-MODEL (STIM), A STATE-OF-THE-ART GLOBAL CIRCULATION MODEL OF THE SATURN UPPER ATMOSPHERE DEVELOPED OVER THE PAST 7 YEARS. STIM CAN PROVIDE PREDICTIONS OF PARAMETERS THAT CAN NOT BE OR HAVE NOT BEEN MEASURED.

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• $827,000 - Thursday the 9th of February 2012
  Department Of Air Force
  FA8650 USAF AFMC AFRL/RQK
  INCREMENTAL FUNDING FOR YEAR 2 OF THE CAT PROGRAM

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• $72,701 - Friday the 10th of July 2015
  National Aeronautics And Space Administration
  NASA SHARED SERVICES CENTER
  PLASMA TURBULENCE IN THE IONOSPHERE OFTEN DISRUPTS AND DISTORTS GPS AND RADIO COMMUNICATION BETWEEN SPACE AND EARTH. TYPICALLY, THIS ARISES WHEN SOLAR-TERRESTRIAL INTERACTIONS CREATE STRONG DENSITY GRADIENTS OR WIND SHEARS THAT, IN TURN, DRIVE PLASMA INSTABILITIES. THE BOSTON UNIVERSITY (BU) RESEARCH GROUP PROPOSES TO CONTRIBUTE TO A FOCUS TEAM EFFORT BY EXPLORING THE DEVELOPMENT, EVOLUTION, AND EFFECTS OF IONOSPHERIC TURBULENCE ON SPATIAL SCALES RANGING FROM CENTIMETERS TO KILOMETERS AND TEMPORAL SCALES FROM MILLISECONDS TO MINUTES. THEY WILL DO THIS USING LARGE-SCALE KINETIC SIMULATIONS, THEORY AND MODELING. THIS WILL HELP SCIENTISTS AND ENGINEERS BETTER UNDERSTAND FUNDAMENTAL PHYSICAL PROCESSES OF THE SPACE ENVIRONMENT AND FURTHER ADAPT OUR SPACE-BASED TECHNOLOGICAL SYSTEMS. THE BU TEAM CAN MOST EASILY CONTRIBUTE TO THE FIRST TWO TYPES OF INVESTIGATIONS OUTLINED IN SECTION 1.2.1(A) OF THE ROSES "LIVING WITH A STAR TARGETED RESEARCH AND TECHNOLOGY SIMULATIONS:" 1. THEORETICAL STUDIES OF THE LINEAR AND NONLINEAR DEVELOPMENT OF IONOSPHERIC INSTABILITIES, 2. FIRST-PRINCIPLE MODELING OF IONOSPHERIC IRREGULARITIES AND TURBULENCE IN 2D AND 3D THEY CAN ALSO CONTRIBUTE TO "OBSERVATIONAL STUDIES IDENTIFYING REGIONS OF IONOSPHERIC IRREGULARITIES AND POSSIBLE CAUSAL MECHANISMS, "PARTICULARLY AS USERS OF JICAMARCA RADIO OBSERVATORY (JRO) DATA. THEIR RESEARCH SHOULD ADVANCE ALL OF THE MEASURES OF SUCCESS LISTED IN 1.2.1(A), BUT IN PARTICULAR THEIR RESEARCH WILL ENHANCE THE FOLLOWING: 1. DEVELOPMENT OF IMPROVED MODELS OF E AND F REGION PLASMA INSTABILITIES AND TURBULENCE; 2. UNDERSTANDING OF THE CONNECTION BETWEEN LARGE-SCALE IONOSPHERIC PROCESSES AND THE DEVELOPMENT OF ELECTRON DENSITY IRREGULARITIES (E.G., EQUATORIAL SPREAD F); AND 3. DEVELOPMENT OF A PREDICTIVE CAPABILITY FOR IRREGULARITY ONSET AND EVOLUTION. THE RESEARCH GROUP AT BU HAS DEVELOPED AN ELECTROSTATIC, MASSIVELY PARALLEL, PARTICLE-IN-CELL (EPPIC) PLASMA SIMULATOR THAT ALSO HAS THE ABILITY TO APPLY HYBRID TECHNIQUES (E.G., PIC IONS&FLUID ELECTRONS). IT WORKS EQUALLY WELL IN 1D, 2D AND 3D AND HAS BEEN USED FOR A BROAD RANGE OF PLASMA PROBLEMS. THIS CODE RUNS EFFICIENTLY ON SOME OF THE WORLD S LARGEST SUPER-COMPUTERS, SCALING TO TENS OF THOUSANDS OF PROCESSORS. IT ALLOWS THEM TO SIMULATE IONOSPHERIC PLASMAS SPANNING A RANGE OF SCALES THAT WERE IMPOSSIBLE UNTIL THE CURRENT GENERATION OF SUPERCOMPUTERS CAME ON-LINE. DUE TO ITS EFFECTS ON COMMUNICATION AND GPS, EQUATORIAL SPREAD-F (ESF) IS THE MOST IMPORTANT OF THESE INSTABILITIES. WHILE THERE ARE CURRENTLY COMPUTER MODELS THAT SIMULATE THE EVOLUTION OF LARGE-SCALE SPREAD-F PHENOMENA (1000KM-TO-KILOMETER), NO SUCH MODELS EXIST FOR MEDIUM AND SHORT-SCALE IRREGULARITIES (KILOMETER-TO-METER). THESE SMALL IRREGULARITIES ARE WHAT RADARS AND SPACECRAFT INSTRUMENTS MEASURE, AND THEY HAVE A DIRECT IMPACT ON THE PROPAGATION OF RADIO WAVES. THIS PROJECT AIMS TO FILL THIS GAP BY SIMULATING ESF FROM THE SMALLEST PHYSICALLY IMPORTANT SCALE (~10 CM) TO KILOMETER SCALES AND DEVELOP A BETTER UNDERSTANDING OF HOW THESE IRREGULARITIES EVOLVE AND DISSIPATE. IN ORDER TO ACCURATELY MODEL SHORT WAVELENGTH DISSIPATION, SUCH COMPUTATIONS MUST BE KINETIC, AT LEAST FOR IONS. AS A SECONDARY INVESTIGATION, THE BU TEAM CAN ALSO EXPLORE E-REGION INSTABILITIES. IN PARTICULAR, THEY CAN STUDY THE EVOLUTION OF LARGE-SCALE GRADIENT-DRIFT WAVES AND ALSO AT HOW MID-LATITUDE SHEAR-DRIVEN SPORADIC-E IRREGULARITIES DEVELOP, EVOLVE, AND COUPLE TO THE F-REGION. FOR ALL INVESTIGATIONS, THEY WILL COMPARE SIMULATION AND MODEL RESULTS TO MEASUREMENTS, BOTH SPECTRALLY AND SPATIALLY. THIS WILL ALLOW THEM TO APPRAISE THE ACCURACY OF THEIR TECHNIQUES AND TO SUGGEST NEW APPROACHES AND MEASUREMENTS. THESE STUDIES WILL FURTHER SCIENTIST S ABILITY TO MODEL AND PREDICT THE ONSET, EVOLUTION, AND EFFECTS OF IONOSPHERIC IRREGULARITIES.

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• $69,538 - Friday the 10th of July 2015
  National Aeronautics And Space Administration
  NASA SHARED SERVICES CENTER
  PLASMA TURBULENCE IN THE IONOSPHERE OFTEN DISRUPTS AND DISTORTS GPS AND RADIO COMMUNICATION BETWEEN SPACE AND EARTH. TYPICALLY, THIS ARISES WHEN SOLAR-TERRESTRIAL INTERACTIONS CREATE STRONG DENSITY GRADIENTS OR WIND SHEARS THAT, IN TURN, DRIVE PLASMA INSTABILITIES. THE BOSTON UNIVERSITY (BU) RESEARCH GROUP PROPOSES TO CONTRIBUTE TO A FOCUS TEAM EFFORT BY EXPLORING THE DEVELOPMENT, EVOLUTION, AND EFFECTS OF IONOSPHERIC TURBULENCE ON SPATIAL SCALES RANGING FROM CENTIMETERS TO KILOMETERS AND TEMPORAL SCALES FROM MILLISECONDS TO MINUTES. THEY WILL DO THIS USING LARGE-SCALE KINETIC SIMULATIONS, THEORY AND MODELING. THIS WILL HELP SCIENTISTS AND ENGINEERS BETTER UNDERSTAND FUNDAMENTAL PHYSICAL PROCESSES OF THE SPACE ENVIRONMENT AND FURTHER ADAPT OUR SPACE-BASED TECHNOLOGICAL SYSTEMS. THE BU TEAM CAN MOST EASILY CONTRIBUTE TO THE FIRST TWO TYPES OF INVESTIGATIONS OUTLINED IN SECTION 1.2.1(A) OF THE ROSES "LIVING WITH A STAR TARGETED RESEARCH AND TECHNOLOGY SIMULATIONS:" 1. THEORETICAL STUDIES OF THE LINEAR AND NONLINEAR DEVELOPMENT OF IONOSPHERIC INSTABILITIES, 2. FIRST-PRINCIPLE MODELING OF IONOSPHERIC IRREGULARITIES AND TURBULENCE IN 2D AND 3D THEY CAN ALSO CONTRIBUTE TO "OBSERVATIONAL STUDIES IDENTIFYING REGIONS OF IONOSPHERIC IRREGULARITIES AND POSSIBLE CAUSAL MECHANISMS, "PARTICULARLY AS USERS OF JICAMARCA RADIO OBSERVATORY (JRO) DATA. THEIR RESEARCH SHOULD ADVANCE ALL OF THE MEASURES OF SUCCESS LISTED IN 1.2.1(A), BUT IN PARTICULAR THEIR RESEARCH WILL ENHANCE THE FOLLOWING: 1. DEVELOPMENT OF IMPROVED MODELS OF E AND F REGION PLASMA INSTABILITIES AND TURBULENCE; 2. UNDERSTANDING OF THE CONNECTION BETWEEN LARGE-SCALE IONOSPHERIC PROCESSES AND THE DEVELOPMENT OF ELECTRON DENSITY IRREGULARITIES (E.G., EQUATORIAL SPREAD F); AND 3. DEVELOPMENT OF A PREDICTIVE CAPABILITY FOR IRREGULARITY ONSET AND EVOLUTION. THE RESEARCH GROUP AT BU HAS DEVELOPED AN ELECTROSTATIC, MASSIVELY PARALLEL, PARTICLE-IN-CELL (EPPIC) PLASMA SIMULATOR THAT ALSO HAS THE ABILITY TO APPLY HYBRID TECHNIQUES (E.G., PIC IONS&FLUID ELECTRONS). IT WORKS EQUALLY WELL IN 1D, 2D AND 3D AND HAS BEEN USED FOR A BROAD RANGE OF PLASMA PROBLEMS. THIS CODE RUNS EFFICIENTLY ON SOME OF THE WORLD S LARGEST SUPER-COMPUTERS, SCALING TO TENS OF THOUSANDS OF PROCESSORS. IT ALLOWS THEM TO SIMULATE IONOSPHERIC PLASMAS SPANNING A RANGE OF SCALES THAT WERE IMPOSSIBLE UNTIL THE CURRENT GENERATION OF SUPERCOMPUTERS CAME ON-LINE. DUE TO ITS EFFECTS ON COMMUNICATION AND GPS, EQUATORIAL SPREAD-F (ESF) IS THE MOST IMPORTANT OF THESE INSTABILITIES. WHILE THERE ARE CURRENTLY COMPUTER MODELS THAT SIMULATE THE EVOLUTION OF LARGE-SCALE SPREAD-F PHENOMENA (1000KM-TO-KILOMETER), NO SUCH MODELS EXIST FOR MEDIUM AND SHORT-SCALE IRREGULARITIES (KILOMETER-TO-METER). THESE SMALL IRREGULARITIES ARE WHAT RADARS AND SPACECRAFT INSTRUMENTS MEASURE, AND THEY HAVE A DIRECT IMPACT ON THE PROPAGATION OF RADIO WAVES. THIS PROJECT AIMS TO FILL THIS GAP BY SIMULATING ESF FROM THE SMALLEST PHYSICALLY IMPORTANT SCALE (~10 CM) TO KILOMETER SCALES AND DEVELOP A BETTER UNDERSTANDING OF HOW THESE IRREGULARITIES EVOLVE AND DISSIPATE. IN ORDER TO ACCURATELY MODEL SHORT WAVELENGTH DISSIPATION, SUCH COMPUTATIONS MUST BE KINETIC, AT LEAST FOR IONS. AS A SECONDARY INVESTIGATION, THE BU TEAM CAN ALSO EXPLORE E-REGION INSTABILITIES. IN PARTICULAR, THEY CAN STUDY THE EVOLUTION OF LARGE-SCALE GRADIENT-DRIFT WAVES AND ALSO AT HOW MID-LATITUDE SHEAR-DRIVEN SPORADIC-E IRREGULARITIES DEVELOP, EVOLVE, AND COUPLE TO THE F-REGION. FOR ALL INVESTIGATIONS, THEY WILL COMPARE SIMULATION AND MODEL RESULTS TO MEASUREMENTS, BOTH SPECTRALLY AND SPATIALLY. THIS WILL ALLOW THEM TO APPRAISE THE ACCURACY OF THEIR TECHNIQUES AND TO SUGGEST NEW APPROACHES AND MEASUREMENTS. THESE STUDIES WILL FURTHER SCIENTIST S ABILITY TO MODEL AND PREDICT THE ONSET, EVOLUTION, AND EFFECTS OF IONOSPHERIC IRREGULARITIES.

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• $50,784 - Tuesday the 16th of August 2016
  National Aeronautics And Space Administration
  NASA SHARED SERVICES CENTER
  WE WILL USE TWO NEWLY-AVAILABLE DATASETS, EACH WITH UNIQUE STRENGTHS, TO EXPLORE THE IONOSPHERE OF MARS. THE FIRST DATASET IS THE COLLECTION OF IONOSPHERIC ELECTRON DENSITY PROFILES ACQUIRED BY THE MARINER 9 RADIO OCCULTATION EXPERIMENT IN 1971-2. WE HAVE REDISCOVERED THESE ON ARCHIVED MICROFILM AND ARE IN THE PROCESS OF CONVERTING THEM TO USABLE DIGITAL FILES. THESE PROFILES EXTEND TO 400 KM, MUCH HIGHER THAN THE CORRESPONDING MGS PROFILES, ENABLING STUDIES OF THE HIGH ALTITUDE IONOSPHERE, AND COVER A MASSIVE DUST STORM, ENABLING STUDIES OF LOWER-UPPER ATMOSPHERE COUPLING. THE SECOND DATASET CONTAINS IONOSPHERIC ELECTRON DENSITIES FROM MARSIS ON MARS EXPRESS, BOTH LOCAL DENSITIES AT THE SPACECRAFT (275-1250 KM) AND REMOTELY-SENSED DENSITIES AT LOWER ALTITUDES (120-275 KM). THESE DATA CROSS THE IONOPAUSE (TYPICALLY 400 KM, BUT HIGHLY VARIABLE) AND THEIR RAPID SAMPLING CADENCE REVEALS HORIZONTAL AND TEMPORAL GRADIENTS IN UNPRECEDENTED DETAIL. NEVERTHELESS, SEVERAL UNUSUAL FEATURES, PARTICULARLY AT THE 275 KM TRANSITION BETWEEN THE TWO DATA TYPES, DEMONSTRATE A CLEAR NEED FOR A CAREFUL COMPARISON OF MARSIS ELECTRON DENSITIES AGAINST THOSE MEASURED BY THE WELL-CHARACTERIZED TECHNIQUE OF RADIO OCCULTATIONS. WE SHALL FIRST MAKE THE MARINER 9 IONOSPHERIC DATASET PUBLICLY AVAILABLE (TASK A: ARCHIVING THE MARINER 9 ELECTRON DENSITY PROFILES). NEXT, WE SHALL STUDY THIS DATASET BEARING IN MIND THE MANY DISCOVERIES MADE AT MARS SINCE THE MARINER 9 INSTRUMENT TEAM LAST ANALYZED IT (TASK B: SCIENTIFIC INTERPRETATION OF THE MARINER 9 ELECTRON DENSITY PROFILES). FINALLY, WE SHALL COMPARE SEVERAL SYNTHESIZED REPRESENTATIONS OF IONOSPHERIC ELECTRON DENSITIES THAT HAVE BEEN PUBLISHED BY THE MARSIS TEAM TO MARINER 9 AND MGS RADIO OCCULTATION ELECTRON DENSITY PROFILES (TASK C: COMPARISON OF MARSIS AND RADIO OCCULTATION IONOSPHERIC MEASUREMENTS). AT THE CONCLUSION OF THIS PROJECT, WE EXPECT TO HAVE DEPOSITED A VALUABLE DATASET INTO NASA'S PERMANENT ARCHIVES, ENSURING ITS AVAILABILITY TO FUTURE GENERATIONS, TO HAVE USED IT TO STUDY FEATURES OF THE IONOSPHERE OF MARS THAT ARE NOT ACCESSIBLE TO CURRENT DATASETS, SUCH AS THE TOPSIDE IONOSPHERE AND THE RESPONSE TO A MASSIVE DUST STORM, AND TO HAVE COMPARED TWO TYPES OF MARSIS ELECTRON DENSITY MEASUREMENTS AGAINST INDEPENDENT RADIO OCCULTATION MEASUREMENTS, INCLUDING PROFILES THAT SPAN THE TRANSITION REGION BETWEEN MARSIS DATA TYPES.

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• $45,827 - Monday the 3rd of December 2012
  Veterans Affairs Department
  241-NETWORK CONTRACT OFFICE 01
  OTHER FUNCTIONS - HISTOLOGY STUDIES IN SUPPORT OF VA RETINAL PROSTHESIS RESEARCH OPTION EXERCISE

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• $413,507 - Friday the 10th of July 2015
  National Aeronautics And Space Administration
  NASA SHARED SERVICES CENTER
  A KEY CHALLENGE IN A CARBON MONITORING SYSTEM IS SCALING THEMATICALLY RICH BUT HIGHLY LOCALIZED INFORMATION TO THE BROAD SPATIAL SCALES NEEDED FOR CARBON ACCOUNTING AND MANAGEMENT. THIS IS PARTICULARLY TRUE FOR WOODED ECOSYSTEMS, WHERE CARBON STORAGE POTENTIAL IS HIGH, BUT ACTUAL CARBON STATUS IS HIGHLY DETERMINED BY LOCAL-SCALE ENVIRONMENTAL AND FOREST MANAGEMENT CONDITIONS. THROUGH A USDA-NIFA FUNDED PROJECT ENTITLED INTEGRATED, OBSERVATION-BASED CARBON MONITORING FOR WOODED LANDS OF WASHINGTON, OREGON AND CALIFORNIA , OUR TEAM IS DEVELOPING A SYSTEM TO INTEGRATE LANDSAT SATELLITE IMAGERY, MAPS OF ENVIRONMENTAL CHARACTERISTICS, FOREST INVENTORY AND ANALYSIS (FIA) PLOT DATA, SMALL-FOOTPRINT LIDAR DATA, AND AERIAL PHOTOS TO CHARACTERIZE KEY CARBON DYNAMICS IN FORESTED ECOSYSTEMS ACROSS ALL OWNERSHIPS IN THE STATES OF WASHINGTON, OREGON, AND CALIFORNIA FROM 1985 TO 2010. KEY CHARACTERISTICS OF OUR SYSTEM INCLUDE: OPERATIONAL SCALING OF LOCAL-SCALE DYNAMICS TO ALL FORESTS IN WASHINGTON, OREGON, AND CALIFORNIA YEARLY MAPPING OF FOREST BIOMASS AND CHANGE IN BIOMASS FROM 1990 TO 2010 EXPLICIT CHARACTERIZATION OF CAUSE OF CHANGE INTEGRATION OF USDA FOREST SERVICE FOREST INVENTORY AND ANALYSIS (FIA) PLOT DATA LINKAGE OF SMALL-FOOTPRINT LIDAR DATA WITH REGIONAL SCALE BIOMASS MAPS EXPLICIT QUANTIFICATION OF METHODOLOGICAL UNCERTAINTIES FOR ALL ESTIMATES BECAUSE OUR APPROACH ADDRESSES KEY CHALLENGES FACED BY THE CURRENT NASA CARBON MONITORING SYSTEM (CMS), WE BELIEVE IT HAS THE POTENTIAL TO COMPLEMENT AND AID NASA S MANDATE FOR OPERATIONAL CARBON MONITORING. TO HELP REACH THAT POTENTIAL, WE PROPOSE THREE ACTIVITIES. -- 1. WE WILL UTILIZE THE PRODUCTS FROM OUR OWN CARBON MONITORING PROGRAM IN FORESTS OF WASHINGTON, OREGON, AND CALIFORNIA TO EVALUATE, UNDERSTAND, AND IMPROVE PERFORMANCE OF THE NASA CMS PRODUCTS, AND COMPARE A VARIETY OF NATIONAL-SCALE PRODUCTS BOTH TO EACH OTHER AND TO FIA PLOT ESTIMATES. -- 2. WE WILL WORK WITH COLLABORATORS WITHIN THE USDA FIA TO EXTEND OUR APPROACHES TO A DIFFERENT FOREST SYSTEM, LINKING EXPLICITLY WITH THE LOCAL-SCALE NASA CMS EFFORTS IN EASTERN FORESTS. -- 3. FINALLY, WE WILL BRING OUR DATA, METHODS, AND LESSONS-LEARNED TO NASA CMS SCIENCE DEFINITION TEAM, AND WORK CLOSELY WITH OTHER SDT MEMBERS TO LINK OUR APPROACHES INTO THOSE ANALYTICAL AND MODELING FRAMEWORKS TO FURTHER THE OVERARCHING GOALS OF THE CMS. THE FOLLOWING CHARACTERISTICS OF OUR PROJECT ARE RELEVANT TO NASA S NEED TO EVALUATE AND IMPROVE ITS CMS: - EVALUATING THE UTILITY AND CHARACTERIZING UNCERTAINTIES IN CMS PRODUCTS - UNDERSTANDING SCALING ISSUES NEEDED TO LINK LOCAL TO NATIONAL SCALE PRODUCTS - DEVELOPING AND DEMONSTRATING FEASIBILITY OF ALTERNATIVE APPROACHES TO MONITORING - ILLUSTRATING CAPABILITIES OF SATELLITE-BASED MONITORING FOR SCIENCE AND MANAGEMENT

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• $36,015 - Thursday the 6th of March 2014
  Veterans Affairs Department
  241-NETWORK CONTRACT OFFICE 01
  IGF::OT::IGF RATIFICATION OF UNAUTHORIZED COMMITTMENT

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• $35,000 - Thursday the 18th of October 2012
  Department Of Air Force
  FA9453 DET 8 AFRL PKV8
  INCREMENTAL FUNDING $35K THRU 31 MAR 13

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• $331,000 - Tuesday the 7th of October 2014
  Veterans Affairs Department
  241-NETWORK CONTRACT OFFICE 01
  REVIEW OF RESEARCH STUDIES PER CHARTER

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