This data set contains raw laser altimeter, Inertial Measurement Unit (IMU), Global Positioning System (GPS), and camera data over Greenland and Antarctica taken from the NASA Land, Vegetation, and Ice Sensor (LVIS). The data were collected as part of Operation IceBridge funded campaigns.
Operation IceBridge products may include test flight data that are not useful for research and scientific analysis. Test flights usually occur at the beginning of campaigns. Users should read flight reports for the flights that collected any of the data they intend to use. Check IceBridge campaign Flight Reports for dates and information about test flights.
The following example shows how to cite the use of this data set in a publication.
Blair, Bryan, and Michelle Hofton. 2011. IceBridge LVIS L0 Raw Ranges. Version 1.0. [indicate subset used]. Boulder, Colorado USA: NASA DAAC at NSIDC. Digital media. http://nsidc.org/data/ilvis0.html.
| NASA DC-8 | |
Land, Vegetation, and Ice Sensor (LVIS) |
|
Greenland, Antarctica |
|
| Nominally 20 meters |
|
14 April 2009 to the present. |
|
| Seasonal |
|
Altimeter measurements of terrain elevation |
|
Binary IMU files |
|
Metadata Access |
|
Data Access |
Bryan Blair
Laser Remote Sensing Laboratory, Code 694
NASA Goddard Space Flight Center
Greenbelt, MD 20771
Michelle Hofton
Department of Geography
2181 LeFrak Hall
University of Maryland
College Park, MD 20742
NSIDC User Services
National Snow and Ice Data Center
CIRES, 449 UCB
University of Colorado
Boulder, CO 80309-0449 USA
phone: +1 303.492.6199
fax: +1 303.492.2468
form: Contact NSIDC User Services
e-mail: nsidc@nsidc.org
This work was supported by NASA Grant Number NNX11AH69G, LVIS: A Topographic Mapping Capability for IceBridge.
Files in the LVIS Level-0 data set include binary laser altimeter, Inertial Measurement Unit and Global Positioning System data, binary JPEG images, and ASCII text files. All contain raw, unprocessed data.
Data are available on the FTP site in the following directory: ftp://n4ftl01u.ecs.nasa.gov/SAN2/ICEBRIDGE_FTP/ILVIS0_LVISraw_v01/.
Each directory contains data for one IceBridge campaign and is named with its year, location (AN = Antarctica, GR = Greenland), and NASA, for example: /2009_AN_NASA/.
Within each campaign, a directory is named for each Modified Julian Day (MJD) and contains the instrument data collected on that day, for example: /55117/. A tool for conversion between date and MJD is available at http://www.csgnetwork.com/julianmodifdateconv.html.
Within each MJD directory are sub-directories for instruments. These may include some or all of:
These directories may have subdirectories corresponding to separate individual instruments. Examples are:
LVIS L0 Raw Ranges data file names for each instrument follow different conventions as described below and in the following tables.
LVIS altimeter files found in /rtlvis/ are binary or ASCII text files with naming conventions as described in Table 1.
Examples:
fpga_20091013_15.47.48_00001.bin
galv_20091013_15.47.48.00001.bin
rtlvis_20091013_15.47.48_00001.bin
status_20091013_15.47.48_00001.bin
telem_20091013_15.47.48_00001.bin
applanix_raw_20091013.bin
log_rtlvis_20091013.txt
aaaaaa_YYYYMMDD_hh.mm.ss_NNNNN.bin
aaaaaa_YYYYMMDD.bin
aaaaaa_YYYYMMDD.txt
Where:
| Variable | Description |
|---|---|
| aaaaaa | fpga = Delphi digitizer / scanner code galv = time and galvanometer position rtlvis = LVIS digitizer / scanner data status = binary system status information telem = binary system status information applanix_raw = binary status packets from the Applanix IMU/GPS system log_rtlvis = records all user and real time ground tracking commands |
| YYYY | Four-digit year (GMT) at beginning of data collection |
| MM | Two-digit month (GMT) at beginning of data collection |
| DD | Two-digit day (GMT) at beginning of data collection |
| hh.mm.ss | hh = hour (GMT) at beginning of data collection mm = minute (GMT) at beginning of data collection ss = second (GMT) at beginning of data collection |
| NNNNN | sequential number, increments through the data collection period |
| .bin or .txt | indicates binary or ASCII text file |
Inertial Measurement Unit raw data files in /applanix/ or /gyro/ are binary or ASCII text files with naming conventions as described in Table 2. Note that normal LVIS operating conditions include two IMUs operating concurrently. Thus, two subdirectories are typically present.
Examples:
13Oct09.091
POSAV.001
AMES.015
LVIS.086
AAAAAA.NNN
Where:
| Variable | Description |
|---|---|
| AAAAAA | Combined with directory and subdirectory name, identifies the individual instrument. |
| .NNN | NNN = Sequential number. Data collected throughout the flight are separated into a sequence of smaller files according to instrument configuration or in order to limit file size. |
Some subdirectories contain the file md5deep.txt. This is an ASCII text file containing the MD5 hash numbers for each file in the subdirectory. It is provided for the user to check the integrity of a binary data file following download.
Unprocessed image files found in /camera/ are in standard binary JPEG format, and are named according to the following conventions and as described in Table 3. Note that these raw images are not georeferenced.
Examples:
IMG_5041.JPG
2009_10_16_0001.JPG
LVISCAM_2011_05_11_0001.JPG
Where:
| Variable | Description |
|---|---|
| IMG_XXXX.JPG | IMG = image XXXX = sequential number JPG = JPEG format |
| YYYY_MM_DD_XXXX.JPG | YYYY = four-digit year MM = two-digit month DD = two-digit day XXXX = sequential number JPG = JPEG format |
| LVISCAM_YYYY_MM_DD_XXXX.JPG | LVISCAM = LVIS camera YYYY = four-digit year MM = two-digit month DD = two-digit day XXXX = sequential number JPG = JPEG format |
Raw GPS files under directory /gps/ are named according to the following numerous conventions used by different receiver manufacturers. Files may be binary or ASCII. Multiple and various makes and models of ground based and airborne GPS receivers were in operation during the different LVIS IceBridge campaigns and may be identified by their name included in subdirectory and/or file names. Interested users are referred to those manufacturers for their proprietary file formats. Some file naming conventions are generally described in Table 4 below. The LVIS instrument team converted these proprietary formatted raw data into the standard RINEX format prior to processing with commercially available software. Please contact the LVIS data providers if more information is required.
Where:
| Examples | Description |
|---|---|
| J0080_101309.jps J078042a.jps 00790329a.jps 20101019_1.jps J0790508a |
.jps = proprietary binary format from Javad receivers, see www.javad.com (ASCII text file if '.jps' is absent) JXXX_YYYYYYZ: optional J = Javad XXX = receiver identification number YYYYYY = date as MMDD, MMDDYY, or YYYYMMDD Z = lower case a-z, or _N, indicating position in a sequence |
| 00443090.PDC | .PDC = proprietary binary format from NovAtel receivers (see www.novatel.com) |
| mgps_01_20091013a.gps | mgps*.gps = binary data from the IMU's internal GPS receiver |
| B1585A09.286 E1585A09.286 S1585A09.286 alm09.286 |
binary and ASCII files from Ashtec receivers (see www.ashtec.com) LMMMMNPP.XXX or almPP.XXX: L = B, E, or S, proprietary Ashtec binary format files alm = ASCII format almanac file MMMM = receiver identification number N = sequential letter PP = two-digit year .XXX = day of year |
Some subdirectories under /gps/ contain a file or files named similarly to md5deep.txt. These are ASCII text files containing the MD5 hash numbers for each file in the subdirectory. They are provided for the user to check the integrity of their downloaded binary data file(s).
Aircraft data files under /planedata/ contain aircraft position, attitude, and motion data and are in ASCII format. These are present for Operation IceBridge 2011 Antarctica data only, as they pertain to operations in the Gulfstream-V aircraft. The file naming convention is described in Table 5. No additional documentation is available to accompany these files.
Example:
OIBGVrf01.asc
Where:| Variable | Description |
|---|---|
| OIB | Operation IceBridge |
| GV | Gulfstream-V aircraft |
| rfxx | xx = sequential operational day number |
| .asc | Indicates ASCII text file |
Data volume for the full data set is approximately 5.5 TB.
Spatial coverage for the IceBridge LVIS campaigns includes the Arctic, Greenland, Antarctica, and surrounding ocean areas. In effect, this represents the coverage noted below.
Arctic / Greenland:
Southernmost Latitude: 60° N
Northernmost Latitude: 90° N
Westernmost Longitude: 180° W
Easternmost Longitude: 180° E
Antarctic:
Southernmost Latitude: 90° S
Northernmost Latitude: 53° S
Westernmost Longitude: 180° W
Easternmost Longitude: 180° E
Spatial resolution is nominally 20 meters, but varies with aircraft altitude. Laser spot size is a function of beam divergence and altitude. Nominal spot spacing is a function of scan rate and pulse repetition rate.
International Terrestrial Reference Frame (ITRF 2000), WGS-84 Ellipsoid.
These data were collected as part of Operation IceBridge funded campaigns from 14 April 2009 to the present.
IceBridge campaigns are conducted on an annual repeating basis. Arctic and Greenland campaigns are conducted during March, April, and May, and Antarctic campaigns are conducted during October and November.
The primary data parameter in this data set is raw laser altimeter measurement from the LVIS instrument. Additional supporting parameters include raw GPS and aircraft position, attitude, and motion readings. These files, provided for archival purposes, contain the raw data processed by the LVIS instrument team using proprietary software to create the data sets: IceBridge LVIS Level-1B Geolocated Return Energy Waveforms and IceBridge LVIS Level-2 Geolocated Surface Elevation Product.
Data are available via FTP.
No software or tools are provided for the L0 files.
As described on the NASA LVIS Web site, a laser altimeter is an instrument that measures range from the instrument to a target object or surface. The device sends a laser beam toward the target, and measures the time it takes for the signal to reflect back from the surface. Knowing the precise round-trip time it takes for the reflection to return yields the range to the target.
Figure 1 shows two examples of return energy waveforms. A simple waveform occurs where the ice surface is relatively smooth within the footprint of the laser pulse (approximately 20 meters in diameter). Mean noise level, provided with the Level-1B data product, provides the threshold relative to which the centroid and all modes are later computed for the Level-2 data product. A complex waveform might be returned from a rougher ice surface and could contain more than one mode, originating from different reflecting surfaces within the laser footprint such as crevasse sides and bottom, open water, large snowdrifts, and other steep or multiple slopes. A complex waveform would be more typically returned from multilevel vegetation landcover such as a forest.

Figure 1. Sample Level-1B Product Waveforms Illustrating Some Possible Distributions of Reflected Light
LVIS employs a signal digitizer, disciplined with a very precise oscillator, to measure both the transmitted and reflected laser pulse energies versus time. These digitized and captured photon histories are known as waveforms. For the outgoing pulse, it represents the profile of the individual laser shot, and for the return pulse it records the interaction of that transmitted pulse with the target surface.
Processing of these waveforms yields many products, but the primary is range from the instrument to the Earth's surface and the distribution of reflecting surfaces within the area of the laser footprint. For vegetated terrain these surfaces are tree canopies, branches, other forms of vegetation, and open ground. For cryospheric data these surfaces are snow, ice, crevasses, snowdrifts, sea ice possibly interspersed with open ocean, exposed rock, and water.
LVIS uses a waveform-based measurement technique to collect data instead of just timing detected returns of the laser pulse. The return signal is sampled rapidly, and stored completely for each laser shot. Retaining all waveform information allows post processing of the data to extract many different products. With the entire vertical extent of surface features recorded, metrics can be extracted about the sampled area. An advantage of saving all of the waveform data is that new techniques can be applied to these data long after collection to extract even more information. See the NASA LVIS Web site.
The LVIS L0 data are raw unprocessed data. No derivation techniques, algorithms, or processing steps are used.
As described on the NASA LVIS Web site the Land, Vegetation, and Ice Sensor is an airborne LIDAR scanning laser altimeter used by NASA for collecting surface topography and vegetation coverage data. LVIS uses a signal digitizer with oscillator to measure transmitted and reflected laser pulse energies versus time capturing photon histories as waveforms. The laser beam and telescope field of view scan a raster pattern along the surface perpendicular to aircraft heading as the aircraft travels over a target area. LVIS has a scan angle of approximately 12 degrees, and can cover 2 km swaths from an altitude of 10 km. Typical collection size is 10 to 25 meter spots. In addition to waveform data, GPS satellite data is recorded at ground tie locations and on the airborne platform to precisely reference aircraft position. An IMU is attached directly to the LVIS instrument and provides information required for coordinate determination.
Blair, J. B., D. L. Rabine., and M. A. Hofton. 1999. The Laser Vegetation Imaging Sensor: A Medium-Altitude, Digitisation-Only, Airborne Laser Altimeter for Mapping Vegetation and Topography, ISPRS Journal of Photogrammetry and Remote Sensing, 54: 115-122.
Hofton, M. A., J. B. Blair, J. B. Minster., J. R. Ridgway, N. P. Williams, J. L Bufton, and D. L. Rabine. 2000. An Airborne Scanning Laser Altimetry Survey of Long Valley, California, International Journal of Remote Sensing, 21(12): 2413-2437.
Hofton, M. A., J. B. Blair, S. B. Luthcke, and D. L. Rabine. 2008. Assessing the Performance of 20-25 m Footprint Waveform Lidar Data Collected in ICESat Data Corridors in Greenland, Geophysical Research Letters, 35: L24501, doi:10.1029/2008GL035774.
The acronyms used in this document are listed in Table 6.
| Acronym | Description |
|---|---|
| ASCII | American Standard Code for Information Interchange |
| CIRES | Cooperative Institute for Research in Environmental Science |
| ECS | NASA Earth Observing System Data and Information System (EOSDIS) Core System |
| FTP | File Transfer Protocol |
| GPS | Global Positioning System |
| IMU | Inertial Measurement Unit |
| INS | Inertial Navigation System |
| ITRF | International Terrestrial Reference Frame |
| JPEG | Joint Photographic Experts Group |
| L0 | Level-0 processing |
| LIDAR | LIght Detection And Ranging |
| LVIS | Land, Vegetation, and Ice Sensor |
| MD5 | Message-Digest Algorithm |
| MJD | Modified Julian Day |
| NASA | National Aeronautics and Space Administration |
| NSIDC | National Snow and Ice Data Center |
| URL | Uniform Resource Locator |
| WGS 84 | World Geodetic System 1984 |
02 October 2012
http://nsidc.org/data/docs/daac/icebridge/ilvis0/index.html