Documentation Revision Date: 2022-03-31
Dataset Version: 1
The MASTER instrument is a modified Daedalus Wildfire scanning spectrometer that flies on a variety of multi-altitude research aircraft and provides spectral information similar to that provided by the Moderate Resolution Imaging Spectroradiometer (MODIS) and the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), which are aboard two NASA Earth Observing System satellites: Terra and Aqua. The primary goal of this airborne campaign was to demonstrate important science and applications research that is uniquely enabled by HyspIRI-like data, taking advantage of the full suite of MASTER thermal infrared bands as well as the contiguous spectroscopic measurements of the AVIRIS (also flown in the HyspIRI campaign), or combinations of measurements from both instruments.
This dataset includes a total of 900 data files: 100 files in Hierarchical Data Format (HDF-4; *.hdf) format, 360 ENVI raster files (*.dat and *.hdr) that are compressed (*.zip), 190 files in Keyhole Markup Language Zipped (KMZ; *.kmz) format, 90 Portable Network Graphics (PNG; *.png) files that are compressed (*.zip), 40 text (*.txt) files, 10 archives of text files that are zipped (*.zip), 10 flight maps as GIF (*.gif) images, and 100 browse images in JPEG (*.jpg) format.
Green, R.O., S.J. Hook, B. Cairns, and D.J. Diner. 2022. MASTER: HyspIRI Airborne Campaign, California, Early Spring 2014. ORNL DAAC, Oak Ridge, Tennessee, USA. https://doi.org/10.3334/ORNLDAAC/1965
Table of Contents
- Dataset Overview
- Data Characteristics
- Application and Derivation
- Quality Assessment
- Data Acquisition, Materials, and Methods
- Data Access
This dataset includes Level 1B (L1B) and Level 2 (L2) data products from the MODIS/ASTER Airborne Simulator (MASTER) instrument. The spectral data were collected as part of the Hyperspectral Infrared Imager (HyspIRI) mission's preparatory airborne campaign during 10 flights aboard a NASA ER-2 aircraft over California and Nevada, U.S., from 2014-03-31 to 2014-05-07. Data products include L1B georeferenced multispectral imagery of calibrated radiance in 50 bands covering wavelengths of 0.460 to 12.879 micrometers at approximately 50-meter spatial resolution. Derived L2 data products are emissivity in 5 bands in thermal infrared range (8.58 to 12.13 micrometers) and land surface temperature. The L1B file format is HDF-4, and L2 products are provided in ENVI and KMZ formats. In addition, the dataset includes the flight path, spectral band information, instrument configuration, ancillary notes, and summary information for each flight, and browse images derived from each L1B data file.
he MASTER instrument is a modified Daedalus Wildfire scanning spectrometer that flies on a variety of multi-altitude research aircraft and provides spectral information similar to that provided by the Moderate Resolution Imaging Spectroradiometer (MODIS) and the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), which are aboard two NASA Earth Observing System satellites: Terra and Aqua. The primary goal of this airborne campaign was to demonstrate important science and applications research that is uniquely enabled by HyspIRI-like data, taking advantage of the full suite of MASTER thermal infrared bands as well as the contiguous spectroscopic measurements of the AVIRIS (also flown in the HyspIRI campaign), or combinations of measurements from both instruments.
Project: MODIS/ASTER Airborne Simulator
The MODIS/ASTER Airborne Simulator (MASTER) is a scanning spectrometer which flies on a variety of multi-altitude research aircraft and provides data similar to the Moderate Resolution Imaging Spectroradiometer (MODIS) and the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER). MASTER first flew in 1998 and has ongoing deployments as a Facility Instrument in the NASA Airborne Science Program (ASP). MASTER is a joint project involving the Airborne Sensor Facility (ASF) at the Ames Research Center, the Jet Propulsion Laboratory (JPL), and the Earth Resources Observation and Science Center (EROS).
Hook, S.J. Myers, J.J., Thome, K.J., Fitzgerald, M. and A.B. Kahle. 2001. The MODIS/ASTER airborne simulator (MASTER) - a new instrument for earth science studies. Remote Sensing of Environment 76:93–102. https://doi.org/10.1016/S0034-4257(00)00195-4
Additional MASTER datasets are available on the ORNL DAAC MASTER project page.
The MASTER instrument is maintained and operated by the Airborne Sensor Facility (ASF) at NASA Ames Research Center in Mountain View, California, under the oversight of the EOS Project Science Office at NASA Goddard. Data processing was conducted at NASA Ames Research Center and the Jet Propulsion Laboratory at the California Institute of Technology in Pasadena, California.
Spatial Coverage: southern California and western Nevada, U.S.
Spatial Resolution: 50 m
Temporal Coverage: 2015-04-28 to 2015-05-05
Temporal Resolution: One-time estimate
Study Area: All latitudes and longitudes given in decimal degrees.
|Site||Westernmost Longitude||Easternmost Longitude||Northernmost Latitude||Southernmost Latitude|
|southern California; western Nevada||-123.820||-112.500||40.980||31.952|
Data File Information
This dataset includes a total of 900 data files: 100 files in Hierarchical Data Format (HDF-4; *.hdf) format, 360 ENVI raster files (*.dat and *.hdr) that are compressed (*.zip), 190 files in Keyhole Markup Language Zipped (KMZ; *.kmz) format, 90 Portable Network Graphics (PNG; *.png) files that are compressed (*.zip), 40 text (*.txt) files, 10 archives of text files that are zipped (*.zip), 10 flight maps as GIF (*.gif) images, and 100 browse images in JPEG (*.jpg) format (Table 1).
There are different numbers of each type of file, which corresponds to the number of "flights" and "flight tracks". A "flight" is flown on a single day, and a "flight track" typically refers to a segment of a given flight. The number of flight tracks varies among flights (Table 2).
- There are 10 flights with 100 flight tracks (Table 2).
- For each of 100 flight tracks, there is one L1B data file in HDF format, one file in KMZ format, and one auxiliary browse image (*.jpg).
- L2 data are included for 90 of the 100 flight tracks. For each track, there is one L2 data file in KMZ format and five L2 data files in ZIP format.
- Four of the ZIP files contain L2 ENVI data for emissivity, land surface temperature, geographic coordinates, and quality assurance status. Each ZIP includes a binary data file (*.dat) and its header file (*.hdr).
- One ZIP file contains three L2 PNG files: RGB composite, single-band emissivity, and land surface temperature.
- For each flight, there is a collection of auxiliary files providing information about the flight and instrument configuration.
The primary data files are named MASTERLAA_BBBBBBBB_CC_YYYYMMDD_EEFF_GGHH_V0J-X.ext (e.g., MASTERL1B_1462900_01_20140331_1728_1732_V02.hdf).
The flight track-level browse images are named MASTERLAA_BBBBBBBB_CC_YYYYMMDD_EEFF_GGHH_V0J.jpg (e.g., MASTERL1B_1462900_01_20140331_1728_1732_V02.jpg).
The flight-level auxiliary files are named MASTER_BBBBBBBB_YYYYMMDD_X.ext (e.g., MASTER_1462900_20140331_config.txt).
Elements of file names are described as:
AA = ”1B” or “2”, indicating L1B or L2 data level,
BBBBBBBB = flight number (Table 2),
CC = flight track (Table 2),
YYYYMMDD = date of sampling,
EEFF = starting time at EE hour and FF minute,
GGHH = ending time at GG hour and HH minute,
J = version number for file,
X = the file content (see Table 1), and
ext = "hdf", "kmz", "gif", "jpg", "txt", or "zip", indicating the file extension.
Table 1. File names and descriptions.
|File Name||Level||File Type||Total Files||Description|
|Primary Data Files|
|MASTERL1B_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J.hdf||L1B||HDF-4||100||Multispectral radiance in 50 bands, pixel coordinates, sensor configuration, aircraft platform data, analysis parameters. The "CalibratedData" variable provides estimates of radiance in units of W m-2 sr-1 per micron.|
|MASTERL1B_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHHV0J-RGB.kmz||L1B||KMZ||100||RGB composite browse image (in KMZ format) derived from corresponding bands of RGB wavelengths of L1B data.|
|MASTERL2_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J-emissivity_tes.zip||L2||ENVI||90||Map of atmospheric corrected emissivity; Temperature and Emissivity Separation (TES) corrected data in 5 bands (wavelengths: 8.58, 9.02, 10.62, 11.32, and 12.13 µm).|
|MASTERL2_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J-images.zip||L2||PNG||90||Three non-georeferenced images depicting (a) RGB composite using selected bands, (b) emissivity from a single band, and (c) land surface temperature.|
|MASTERL2_BBBBBBBBB_CC_ YYYYmmDD_EEFF_GGHH_V0J-location.zip||L2||ENVI||90||Latitude and longitude coordinates for pixels in ENVI files.|
|MASTERL2_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J-LST.kmz||L2||KMZ||90||Map of land surface temperature in degrees Kelvin.|
|MASTERL2_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J-QAmap.zip||L2||ENVI||90||QA status for each pixel from TES algorithm, where 1 = divergence and 0 = convergence.|
|MASTERL2_BBBBBBBB_CC_YYYYmmDD_EEFF_GGHH_V0J-surface_temp.zip||L2||ENVI||90||Map of land surface temperature (TES LST) in degrees Kelvin.|
|MASTERLAA_BBBBBBBB_CC_YYYYMMDD_EEFF_GGHH_V0J.jpg||L1B||JPEG||100||Browse figures; one image per flight track; multiple tracks per flight.|
|MASTER_BBBBBBBB_YYYYMMDD_ancillary.txt||-||Text||10||Ancillary information about flight including notes on aircraft platform, mission objective, and data evaluation.|
|MASTER_BBBBBBBB_YYYYMMDD_config.txt||-||Text||10||Instrument configuration information for flight.|
|MASTER_BBBBBBBB_YYYYMMDD_flightpath.gif||-||GIF||10||Map showing flight paths.|
|MASTER_BBBBBBBB_YYYYMMDD_spectral_band_info.txt||-||Text||10||Spectral band information for flight.|
|MASTER_BBBBBBBB_YYYYMMDD_spectral_response_table.zip||-||Text||10||Spectral response tables by band (ZIP archive of 50 text files).|
|MASTER_BBBBBBBB_YYYYMMDD_summary.txt||-||Text||10||Time and coordinates for start and end of flight tracks along with the number of scan lines, solar and instrument angles, and aircraft altitude. FTLT = flight track number.|
Data File Details
The HDF and ENVI files contain swath trajectory data using longitude and latitude coordinates. The spatial resolution is 49 to 50 m and is a function of aircraft altitude.
Table 2. Number of flight tracks per file data level for each MASTER flight during this 2014 deployment over California and western Nevada.
|Date||Flight Number||Locations (U.S.)||Flight Tracks|
|2014-03-31||1462900||Ivanpah / Mtn. Pass / Salton Sea||8||8|
|2014-04-07||1463000||Yosemite N.P. / Rim Fire Scar / Soda Straw||14||13|
|2014-04-10||1463100||Lake Tahoe, CA||12||11|
|2014-04-14||1463200||Southern California / EcoHab||11||11|
|2014-04-16||1463300||Santa Barbara, CA||12||10|
|2014-04-18||1463400||San Francisco Bay Area, CA||6||4|
|2014-04-23||1463600||Monterey Bay, CA / Fresno Aeronet Site||6||6|
|2014-04-28||1463700||San Francisco Bay Area, CA||13||12|
|2014-05-07||1463800||San Francisco Bay Area, CA||12||11|
Application and Derivation
The primary objective of MASTER is to: (a) collect ASTER-like and MODIS-like land datasets to support the validation of the ASTER and MODIS geophysical retrieval algorithms; (b) collect these datasets at a higher resolution than the spaceborne datasets to permit scaling studies and comparisons with in situ measurements; and (c) under fly the EOS-AM1 ASTER and MODIS sensors to provide an additional radiometric calibration to assist with in-flight instrument performance characterization. Calibration is particularly important for ASTER where on-board calibration is dependent on a single black body in the TIR and only partial aperture illumination in the VNIR.
A secondary objective of MASTER is to: (a) provide both a backup instrument and backup modules for the current MODIS Airborne simulator, which is committed to a program of atmospheric and oceanic measurements; and (b) provide a wider spectral and dynamic range alternative to the use of the Thematic Mapper (TM) airborne simulator and Thermal Infrared Multispectral Scanner (TIMS) airborne scanners (JPL, 2021b).
MASTER imagery has been used for mapping wildfires and their impacts (Veraverbeke et al., 2011), land cover (Li and Moon, 2004), coral reefs (Capolsini et al., 2003), and urban heat islands (Zhao and Wentz, 2016).
The MASTER instrument channels are calibrated spectrally and radiometrically in the laboratory preflight and postflight. The mid-infrared and thermal infrared channels (26–50) are also radiometrically calibrated in-flight by viewing an internal hot and cold blackbody with each scanline (Hook et al., 2001). Three calibration and validation experiments were conducted in 1998–2001 (Hook et al., 2001; JPL, 2021a). Spectral response information for this deployment is included in the files named MASTER_BBBBBBBB_YYYYMMDD_spectral_response_table.zip.
Data Acquisition, Materials, and Methods
The MASTER instrument was developed by the NASA Ames Research Center in conjunction with the Jet Propulsion Laboratory. The instrument consists of three key components: the scanning spectrometer, the digitizer, and the storage system. The scanning unit was built by Sensys Technology (formerly Daedalus Enterprises) and the digitizer was a collaborative effort between Berkeley Camera Engineering and the Ames Airborne Sensor Facility (ASF, 2021). The data storage system and overall system integration were also provided by the ASF.
The MASTER instrument is similar to the MODIS Airborne Simulator (MAS) developed by the MODIS project (King et al., 1996). However, it has two key differences. First, MASTER supports a variety of scan speeds allowing it to acquire contiguous imagery from a variety of altitudes with different pixel sizes. Second, the channel positions are configured to closely match those of ASTER and MODIS. A detailed description of the instrument and optical system are provided by Hook et al. (2001) and King et al. (1996), respectively.
For this deployment, the MASTER instrument was flown on NASA's ER-2 aircraft at altitudes of 19,214–19,982 m above sea level. The study area included portions of southern California and western Nevada (Fig. 2, 3).
The L2 data are derived from the L1B files, and the primary L2 products are emissivity in five bands (wavelengths: 8.58, 9.02, 10.62, 11.32, and 12.13 µm) and land surface temperature (LST). Emissivity and LST were corrected using a Temperature and Emissivity Separation (TES) algorithm (Coll et al., 2001).
Figure 2. Flight tracks in this dataset represented as rectangular polygons. Map shows southern California and western Nevada, U.S. Basemap: © OpenStreetMap contributors.
Figure 3. Flight path for Flight 1462900, flown on 31 March 2014. Flight 1462900 and 8 flight tracks occurred over southern California and southwestern Nevada, U.S. Source: MASTER_1462900_20140331_flightpath.gif
These data are available through the Oak Ridge National Laboratory (ORNL) Distributed Active Archive Center (DAAC).
Contact for Data Center Access Information:
- E-mail: firstname.lastname@example.org
- Telephone: +1 (865) 241-3952
ASF. 2021. Campaign summary information: HyspIRI / WDTS Airborne Campaign. Airborne Sensor Facility, Airborne Science Program, NASA Ames Research Center, Moffett Field, California. https://asapdata.arc.nasa.gov/sensors/master/data/deploy_html/hyspiri_home.html
Capolsini, P., S. Andréfouët, C. Rion, and C. Payri. 2003. A comparison of Landsat ETM+, SPOT HRV, Ikonos, ASTER, and airborne MASTER data for coral reef habitat mapping in South Pacific islands. Canadian J. Remote Sensing 29:187-200. https://doi.org/10.5589/m02-088
Coll, C., V. Caselles, E. Rubio, F. Sospedra, and E. Valor. 2001. Temperature and emissivity separation from calibrated data of the Digital Airborne Imaging Spectrometer. Remote Sensing of Environment 76:250-259. https://doi.org/10.1016/S0034-4257(00)00207-8
Hook, S.J. Myers, J.J., Thome, K.J., Fitzgerald, M., and A. B. Kahle. 2001. The MODIS/ASTER airborne simulator (MASTER) - a new instrument for earth science studies. Remote Sensing of Environment 76:93-102. https://doi.org/10.1016/S0034-4257(00)00195-4
JPL. 2021a. Calibration and Validation, MASTER: MODIS/ASTER Airborne Simulator. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA. https://masterprojects.jpl.nasa.gov/cal-val
JPL. 2021b. Science objectives, MASTER: MODIS/ASTER Airborne Simulator. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA. https://masterprojects.jpl.nasa.gov/objectives
King, M.D., W.P. Menzel, P.S. Grant, J.S. Myers, G.T. Arnold, S.E. Platnick, L.E. Gumley, S.C. Tsay, C.C. Moeller, M. Fitzgerald, K.S. Brown, and F.G. Osterwisch. 1996. Airborne scanning spectrometer for remote sensing of cloud, aerosol, water vapor and surface properties. J. Atmospheric and Oceanic Technology 13:777-794. https://doi.org/10.1175/1520-0426(1996)013<0777:ASSFRS>2.0.CO;2
Li, P., and W.M. Moon. 2004. Land cover classification using MODIS-ASTER airborne simulator (MASTER) data and NDVI: A case study of the Kochang area, Korea. Canadian J. Remote Sensing 30:123-126. https://doi.org/10.5589/m03-061
Veraverbeke, S., S. Harris, and S. Hook. 2011. Evaluating spectral indices for burned area discrimination using MODIS/ASTER (MASTER) airborne simulator data. Remote Sensing of Environment 115:2702-2709. https://doi.org/10.1016/j.rse.2011.06.010
Zhao, Q., and E.A. Wentz. 2016. A MODIS/ASTER Airborne Simulator (MASTER) imagery for urban heat island research. Data 1:7. https://doi.org/10.3390/data1010007