This data set is comprised of data collected by the Advanced Very High Resolution Radiometer (AVHRR) sensor. Depending on the model, the AVHRR sensor is a broad-band 4- or 5-channel scanning radiometer, sensing in the visible, near-infrared, and thermal infrared portions of the electromagnetic spectrum. Beginning in 1978, this sensor has been carried on the National Oceanic and Atmospheric Administration's (NOAA) Polar Orbiting Environmental Satellites (POES), otherwise known as the Television and Infrared Observation Satellites-N (TIROS-N) series.
The AVHRR data held in the U.S. Geological Survey's EROS Data Center archives are acquired in two formats:
The HRPT data are full resolution image data transmitted to a ground station as they are collected. The LAC data are also full resolution data, but are recorded with an onboard tape recorder for subsequent transmission during a station overpass.
AVHRR-LAC/HRPT
The normal operating mode of the satellite is for direct transmission of AVHRR data to Earth continuously in real time. This direct transmission is called High Resolution Picture Transmission (HRPT). In addition to the HRPT mode, about 11 minutes of data may be selectively recorded per orbit, by recorders on board the satellite for later playback. These recorded data are referred to as Local Area Coverage (LAC) data. The LAC data may be recorded over any portion of the world as selected by NOAA/National Environment Satellite, Data and Information Service (NESDIS) and played back on the same orbit as recorded or during a subsequent orbit.
AVHRR data are raw data as received by the satellite and archived as Level-0 data. Level-1B data are raw data that have been quality controlled, assembled into discrete data sets, and appended with Earth location and calibration information (but not applied). The HRPT and LAC data sets have been combined in this document since they have identical Level-1B formats and spatial resolutions.
The AVHRR Level-1B data represent a collection of data sets. Each data set contains one type of data for a discrete time period. Thus, there are separate AVHRR HRPT and LAC data sets. Time periods are arbitrary subsets of orbits and may cross orbits (i.e., may contain data along a portion of an orbital track that includes the ascending node, the reference point for counting orbits).
The objective of producing the AVHRR Data Set is to provide long term, global data of land surface parameters with high temporal frequency coarse resolution for studying the Earth as an integrated system.
Band # |
Satellites: NOAA-6,8,10 |
Satellites: NOAA-7,9,11,12,14 |
Instantaneous Field of View (IFOV) |
---|---|---|---|
1 | 0.58 - 0.68 | 0.58 - 0.68 | 1.39 |
2 | 0.725 - 1.10 | 0.725 - 1.10 | 1.41 |
3 | 3.55 - 3.93 | 3.55 - 3.93 | 1.51 |
4 | 10.30 - 11.50 | 10.30 - 11.30 | 1.41 |
5 | band 4 repeated | 11.5 - 12.50 | 1.30 |
(micrometers) | (micrometers) | (milliradians) |
The objective of the AVHRR instrument is to provide radiance data for investigation of clouds, land-water boundaries, snow and ice extent, ice or snow melt inception, day and night cloud distribution, temperatures of radiating surfaces, and sea surface temperature. It is an integral member of the payload on the advanced Television and Infrared Observation Satellite-N (TIROS-N) spacecraft and its successors in the NOAA series and, as such, contributes data required to meet a number of operational and research-oriented meteorological objectives.
EROS Data Center (EDC):
Land Processes Distributed Active Archive Center (LP DAAC):
Not applicable.. The AVHRR program is a worldwide data collection effort supporting programs and projects too great to be enumerated in this document.
Not applicable.
The AVHRR sensor is a scanning radiometer with either four or five channels, which is sensitive to visible, near infrared and thermal infrared radiation. The channels have been chosen to permit multispectral analyses, which provide improved determination of hydrologic, oceanographic, and meteorological parameters. The visible (0.5 micron) and near infrared (0.9 micron) channels are used to discern clouds; land-water boundaries; snow and ice extent; and, when the data from the two channels are compared, an indication of ice/snow melt inception. The IR window channels are used to measure cloud distribution and to determine temperature of the radiating surface (cloud or surface). Data from the two IR channels are incorporated into the computation of sea surface temperature.
On later instruments in the series, a third IR channel was added for the capability of removing radiant contributions from water vapor when determining surface temperatures. Prior to inclusion of this third channel, corrections for water vapor contributions were based on statistical means using climatological estimates of water vapor content.
Space, Low Earth Orbit.
TIROS-N and NOAA-6 through NOAA-14
In 1961, the Department of Commerce was directed by Congress to establish and operate a meteorological satellite system. This system was to provide for the continuous observation of worldwide meteorological conditions from space and to report and process the data obtained for use in weather forecasting. The main objectives established in the congressional mandate were:
Radiance and Imagery > Infrared Wavelengths
Radiance and Imagery > Visible Wavelengths
The EDC AVHRR processing flow begins with sensor data receipt by EDC's HRPT receiving station, receipt of data rebroadcast via communications satellite, or receipt of data from the AVHRR Global 1-km Project. All receipts of data are ingested and archived at the EDC. The processes to ingest the data include creating an archive tape; creating an inventory metadata file; creating a metadata file for information systems support; and building browse files.
As the spacecraft moves through its orbit, the expected angular distance between the nadir of adjacent LAC/HRPT scans is approximately 0.0296 degrees of arc, or 3.2914 kilometers, as measured from the center of the Earth. This actual value of the average angular distance can vary by up to about 0.1712 kilometer due to variations in satellite height, scan angle and other factors.
The instantaneous field of view (IFOV) for all channels is specified to be 1.3 +/- 0.1 milliradians.
The NOAA/TIROS radiometers have been designed to view cold space and one or more internal warm blackbodies as part of their normal scan sequences in orbit. This provides data in the microwave and infrared channels for determining signal-to-noise and radiometric slopes and intercepts. Unfortunately, there are no onboard calibration sources for the visible region; in the visible channels, the calibration used is the calibration determined before launch.
There are other coefficients necessary for in-orbit calibration that must be derived from prelaunch test data. These include the coefficients to account for the nonlinearity in the AVHRR's response and the coefficients for calibrating the temperature sensors in the internal blackbodies of the AVHRR sensor.
The following affect the calibration of the sensor:
IFOV ............ 1.4 mr Resolution ...... 1.1 km Altitude ........ 833 km Scan Rate ....... 360 scans/minute Samples/IFOV .... 1.362 samples Scan Range ...... -55.4 to 55.4 degrees Samples/Scan .... 2048 samples per channel per Earth scan
The AVHRR infrared channels were designed for an Noise Equivalent Differential Temperature (NEdT) of 0.12 degrees Kelvin (at 300 Kelvin), and a signal to noise ration of 3:1 at 0.5 percent albedo.
The AVHRR sensor was designed to view cold space and one or more internal warm blackbodies for each scan sequence while in orbit.
In general, radiometric calibration involves exposing a radiometer to sources of radiation that have been calibrated against primary or secondary standards and determining a relationship between the output of the radiometer and the intensity of the incident radiation (radiance).
All the radiometers flown on the NOAA/TIROS satellites undergo extensive prelaunch testing and calibration by their manufacturers to characterize their performance. The NESDIS independently analyzes the data from the prelaunch tests to determine the operating characteristics of the instruments, such as their signal-to-noise ratios, stability, linearity of response, and sensitivity. However, characteristics cannot be expected to be the same in orbit as they were before the launch. One reason is that the thermal environment varies with position in the orbit, causing sensitivities to vary orbitally. Also, instrument components age in the several years that usually elapse between the time of the prelaunch tests and launch, and the aging process continues during the two or more years the instrument typically operates in orbit. Therefore, the NOAA/TIROS radiometers have been designed to view cold space and one or more internal warm blackbodies as part of their normal scan sequences in orbit.
The AVHRR data are both broadcast continually in direct readout mode (HRPT) and recorded (LAC) on board the satellite for later playback. The EDC's AVHRR Data Acquisition and Processing System (ADAPS), which began operation in May 1987, receives approximately six daytime passes per day of HRPT data over the conterminous United States. Night acquisitions are acquired upon request only. As of March 1990, all data received at EDC are permanently archived. Prior to March 1990, approximately 40 percent of the data received were archived.
The NOAA receives both worldwide recorded and direct readout AVHRR data from the Wallops Island, Virginia, and Gilmore Creek, Alaska, stations. Those stations then redirect the data via a satellite relay to NOAA/NESDIS in Suitland, Maryland where the data are processed, archived, and reproduced.
On June 15, 1990, the EDC's ADAPS system was expanded to acquire data via the communications satellite relay used by NOAA. The data collected on a daily basis, consists of global coverage of the world's land masses.
Not applicable.
Not applicable.
The AVHRR sensor provides a global (pole-to-pole) onboard collection of data from all spectral channels. The 110.8-degree scan equates to a swath width of 27.2 degrees at the Equator centered on the subsatellite track. This swath width is greater than the 25.3-degree separation between successive orbital tracks, providing overlapping coverage (side-lap). The satellite orbits the Earth 14 times each day from 833 kilometers above its surface.
Global
The IFOV of each channel is approximately 1.4 milliradians leading to a resolution at the satellite subpoint of 1.1 kilometers for a nominal altitude of 833 kilometers. The scanning rate of the AVHRR sensor is 360 scans per minute. The time within each scan line of AVHRR data represents IFOV 1. These data provide continuous transmission for the HRPT data and selectively recorded LAC data.
Not applicable.
Not applicable.
The overall coverage of the archived AVHRR data base is shown in the following table. However, there may be short gaps in the time ranges and additional data coverage outside these dates associated with equipment malfunctions. Start and end dates indicate operational range.
SATELLITE: | START DATE: | END DATE: |
---|---|---|
TIROS-N | 10/19/78 | 01/30/80 |
NOAA-6 | 06/27/79 | 06/30/86* |
NOAA-7 | 08/24/81 | 06/07/86 |
NOAA-8 |
06/20/83 01/85 |
06/12/84* 10/31/85 |
NOAA-9 | 02/25/85 | 11/07/88 |
NOAA-10 | 11/17/86 | 09/16/91 |
NOAA-11 | 11/08/88 | 09/13/94 |
NOAA-12 | 09/01/91 | present |
NOAA-14 | 12/30/94 | present |
Not applicable.. The temporal coverage map will not be supplied due to the complexities of the acquisition schedules.
Each scan of the AVHRR views the Earth for a period of 51.282 milliseconds. The analog data output from the sensors is digitized onboard the satellite at a rate of 39,936 samples per second per channel. Each sample step corresponds to an angle of scanner rotation of 0.95 milliradian. At this sampling rate, there are 1.362 samples per IFOV. A total of 2,048 samples for the LAC/HRPT data are obtained per channel per Earth scan, which spans an angle of +/- 55.4 degrees from the nadir (subpoint view). Successive scans occur at the rate of six per second or at intervals of 167 milliseconds.
Because the satellite is Sun-synchronous, visible data revisit time is daily. Infrared imaging is accomplished twice daily with the second visit occurring during the pass over the dark side of the Earth. Instrument operation is continuous.
Depending on the instrument, there are four or five channels, which measure wavelengths, as outlined previously in the Summary of Parameters. Other parameters appended include calibration coefficients, Earth location, time code, quality indicators, solar zenith angles, and telemetry.
Each LAC data set contains an individual satellite recorder playback (up to 11 minutes of recorded HRPT data). Each HRPT data set contains the HRPT data from a CDA contact. Data within each LAC/HRPT data set are arranged in chronological order with one scan contained in two physical records. Each record contains 7,440 bytes written in binary format.
The time code consists of the year, day of year, and greenwich mean time (GMT) time of day in milliseconds. The year is contained in the first 7 bits of the first two bytes, the 9-bit day of year is right-justified in the first two bytes, and the 27-bit millisecond GMT time of day is right-justified in the last four bytes. All other bits are zero. The time code always has the same format for all Level-1B data sets.
The quality indicators are contained in four bytes. The first byte contains the status of detected conditions during processing and the last three bytes contain Data Acquisition and Control Subsystems (DACS) quality indicators. If the bit is set to one or the on position, then the condition is true.
The calibration coefficients consist of slope and intercept values for each of the five channels. The use of these coefficients is described in Section 3.3 of the "NOAA Polar Orbiter Data User's Guide". Each value is stored in four bytes in the following order:
Channel 1 slope coefficient, Channel 1 intercept coefficient
Channel 2 slope coefficient, Channel 2 intercept coefficient
Channel 3 slope coefficient, Channel 3 intercept coefficient
Channel 4 slope coefficient, Channel 4 intercept coefficient
Channel 5 slope coefficient, Channel 5 intercept coefficient
A fixed number of zenith angles and Earth location points are appended to each scan. However, only the first n zenith angles and the first n Earth location points have meaningful values (n is defined in byte 53). A maximum of 51 points is possible in a scan. There are 2,048 points in a LAC/HRPT scan line. However, the solar zenith angles and Earth location data (latitude and longitude) are sampled every 40 points starting at the twenty-fifth point (25, 65, 105, ..., 1945, 1985, 2025). There are 51 possible solar zenith angles and Earth location values for each scan line. Each zenith angle requires one byte (stored as degrees by 2). The latitude and longitude values are each stored in two-byte fields in 128ths of a degree (east positive).
The telemetry data contain information which may be used to compute calibration coefficients when these are not included in the data. The telemetry data are stored in 140-byte units. The first 103 10-bit words are packed three 10-bit words in four-bytes, right justified. The last four-byte group contains one 10-bit word with 20 trailing bits. All unused bits are set to zero. The contents of these 103 words are contained in Table 3.1.2.1-3 of the "NOAA Polar Orbiter Data User's Guide", which is the entire HRPT minor frame format. For more information, refer to NOAA Technical Memorandum NESS 107 entitled, "Data Extraction and Calibration of TIROS-N/NOAA Radiometers".
The LAC/HRPT video data consist of five readings (one for each channel) for each of the 2,048 points in a scan. They are packed as three 10-bit samples in four bytes, right-justified. The last four-byte group contains two 10-bit samples with 10 trailing zero bits. The first two bits of each four-byte group are zero. The 10,240 samples (2,048 points by 5 channels) are ordered scan point 1 (Channel 1, 2, 3, 4, 5), scan point 2 (Channel 1, 2, 3, 4, 5), and so forth. For TIROS-N, NOAA-6, NOAA-8, and NOAA-10, there is no sensor for Channel 5 so Channel 4 data are repeated in the Channel 5 position. The video data are stored in 2's complement form.
The 16-bit unpacked format for full copy LAC/HRPT data has the same format as the "packed" data described above except for the video data. The video data values for each channel are contained in the 10 least significant bits and the six most significant bits are zero filled.
Counts which can be converted to radiances.
AVHRR sensor
October 19, 1978, to present.
A general description of data granularity as it applies to the IMS appears in the eosdis Glossary.
LAC/HRPT (varies by scene).
Record structure of LAC/HRPT Level-1B data sets for each file:
Record 1 .... TBM (Terabit memory) Header record (122 bytes) Record 2 .... Data Set Header record (7400 bytes) Record 3 .... Dummy (7400 bytes) Record 4-n .. Data records (7400 bytes)
The TBM Header contains data type and selection parameters. All fields are in ASCII format except the Channels Selected field, which is binary. The overall format follows:
BYTE # |
# of Bytes in Field |
CONTENT |
---|---|---|
31-74 | 44 | Data Set Name** |
75 | 1 | Total/Selective Copy ("T" or "S") |
76-78 | 3 | Beginning Latitude |
79-81 | 3 | Ending Latitude |
82-85 | 4 | Beginning Longitude |
86-89 | 4 | Ending Longitude |
90-91 | 2 | Start Hour |
92-93 | 2 | Start Minute |
94-96 | 3 | Number of Minutes |
97 | 1 | Appended Data Selection ("Y" or "N") |
98-117 | 20 | Channels Selected (in binary) |
NSS.Data-type.Spacecraft-Unique-ID.Year-day.Start-time. Stop-time. Processing-block-ID.Source. The following screens detail this scheme.
Qualifier Valid Entry --------- ----------- Data-Type HRPT = HRPT GHRR = GAC (recorded) LHRR = LAC (recorded HRPT) Spacecraft- TIROS-N = TN Unique ID NOAA-A = NA = NOAA-6 NOAA-B = NB NOAA-C = NC = NOAA-7 NOAA-E = NE = NOAA-8 NOAA-F = NF = NOAA-9 NOAA-G = NG = NOAA-10 NOAA-H = NH = NOAA-11 NOAA-D = ND = NOAA-12 NOAA-I = NI = NOAA-13 NOAA-J = NJ = NOAA-14 Year-day D78141, where "D" identifies this section as a Julian day delimiter. The "78" identifies the year the spacecraft began recording data, and the "141" indicates the Julian day the satellite began recording. Start-time S1422, where "S" identifies this group as a start time delimiter. The "1422" indicates 14 hours and 22 minutes GMT to the nearest minute to when the spacecraft recording began. Stop-time E1555, where "E" identifies this group as a end time delimiter. The "1555" indicates 15 hours and 55 minutes GMT to the nearest minute of the spacecraft recording of the last usable data. Processing- B0017499, where "B" indicates this group is a Block-ID processing block ID delimiter. The "0017499" is a seven digit number identifying the spacecraft revolution number in which data recording began and the revolution in which the recording ended. The first five digits identify the beginning revolution and the last two being the least significant numbers of the ending revolution. The revolution number may be off by one or two digits. Source Gilmore Creek, Alaska = GC Western Europe CDA = WE SOCC (Satellite Operations Control Center) = SO Wallops Island, Virginia = WI EDC, Sioux Falls, SD = SD
Header Record Format
The binary Data Set Header record format follows:
BYTE # |
# of Bytes in Field |
CONTENT |
---|---|---|
1 | 1 | Spacecraft ID |
2 | 1 | Data Type |
3-8 | 6 | Start Time - time code from last data frame |
9-10 | 2 | Number of Scans |
11-16 | 6 | End Time - time code from last data frame |
17-23 | 7 | Processing Block ID (ASCII) |
24 | 1 | Ramp/auto Calibration |
25-26 | 2 | Number of Data Gaps |
27-32 | 6 | DACS Quality |
33-34 | 2 | Calibration Parameter ID |
35 | 1 | DACS Status |
36-40 | 5 | Zero-filled - spare |
41-84 | 44 | 44 Character data set (EBCDIC) |
85-end | variable | Spares - Zero-filled to size of data record (3220 or 14800) |
LAC Data Set Information
Each LAC data set contains two records per scan. The records are 7,400 bytes long and are written in binary format. A design detail follows:
To calculate the size in megabytes of an AVHRR scene, follow the formula listed below:
- Two records at 7400 bytes each .......... 14800 bytes - Six lines/second capture rate (6 x 60 seconds). 360 lines/minute - Using an average EROS pass of .................... 12 minutes - Formula: 14800 x 360 x 12 = 63.9 megabytes
LAC/HRPT Data Record Format
BYTE # | # of BYTES | CONTENTS |
---|---|---|
1-2 | 2 | Scan line number from 1 to n |
3-8 | 6 | Time code - year, julian day, milliseconds |
9-12 | 4 | Quality indicators |
13-52 | 40 | Calibrations coefficients |
53 | 1 | Number of meaningful zenith angles and Earth location points appended to scan (n) |
54-104 | 51 | Solar zenith angles |
105-308 | 204 | Earth Location |
309-448 | 140 | Telemetry (header) |
449-14104 | 13656 | LAC/HRPT video data |
14105-14800 | 696 | Spares |
Not applicable.
The EDC's ADAPS flow for acquisitions and archiving begins with either direct HRPT reception or with re-broadcast of DOMSAT LAC reception. Initial ingest of the data reformatting includes archive, and creation of browse quick looks and cartridge tapes.
The NOAA AVHRR processing flow begins with sensor data receipt by the CDA stations (Wallops Island, Virginia, and Gilmore Creek, Alaska) where the data are re-broadcast via communications satellites to NOAA/NESDIS in Suitland, Maryland. The ephemeris data are accessed through the Gridded Earth Location Determination System (GELDS) software for generation of Level-1B production.
The EDC ADAPS systematic georegistration process references AVHRR data to the Earth's surface. Through modeling the position and attitude of the TIROS satellite platforms and the canning geometry of the AVHRR sensor, geometric distortions can be minimized. The position of the satellite is determined by an orbital model updated by ephemeris data received daily from NAVY Space Surveillance. The AVHRR sensor model characterizes the non-linear scanning of the sensor mirror. A refinement to the sensor model accounts for the displacement in longitude due to the rotation of the Earth under the satellite. All modeling is referenced to the time of acquisition. As the satellite clock time drifts, a delta time adjustment is applied. Collectively, these models comprise the geometric correction model in ADAPS. The positional accuracy of a systematic georegistration is approximately 5,000 meter, root-mean-square-error (RMSE).
Precise georegistration positional accuracy of 1000 meter RMSE requires correlation of image features with accurately registered cartographic or image-based maps. A common practice is to use cartographic sources such as Digital Chart of the World (DCW) or hydrography data to extract easily identifiable features such as coastlines, water bodies, and rivers and to correlate them with the matching raw image locations using various techniques. The correlation process determines specific adjustments to be applied to the time, roll, and yaw parameters of the orbital model. The EDC ADAPS uses a variety of techniques depending upon the geographic location of the imagery and the volume of data to be processed.
See NOAA Polar Orbiter Data User's Guide, Appendix E.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not applicable.
Not Applicable.
Prior to June 1981, the Earth location data in the AVHRR Level-1B data may have been slightly inaccurate due to errors in the TIROS Information Processor (TIP) clock on board the spacecraft. The 6-byte time code in the Level-1B data is taken from the TIP clock, which routinely contained errors of 1.5 to 2.3 seconds.
Refer to the NOAA Polar Orbiter Data User's Guide.
As of September 8, 1992, the EDC implemented enhancements to the Level-1B format. These enhancements utilized some of the spare bytes appended to the end of the header record and the data records. The header record now includes Osculating Keplerian and Cartesian orbit parameters. The size of data records was increased in order to improve the accuracy of the solar zenith angle to one-tenth of a degree.
On November 15, 1994, the following Level-1B data set enhancements were implemented:
The AVHRR data provide opportunities for studying and monitoring vegetation conditions in ecosystems including forests, tundra, and grasslands. Applications include agricultural assessment, land cover mapping, producing large-area image maps (e.g., country maps, continental maps, world maps), and tracking regional and continental snow cover. The AVHRR data are also used to retrieve various geophysical parameters such as sea surface temperatures and energy budget data.
Not available.
Not available.
Not available
LP DAAC
Not available.
The LP DAAC provides standard AVHRR digital Level-1B products on 8 mm tape cassette and 3480 cartridge.
Kidwell, K.B., 1995, NOAA polar orbiter data user's guide: Washington, D.C., National Oceanic and Atmospheric Administration [variously paged].
Planet, W.G., ed., 1988, Data extraction and calibration of TIROS-N/NOAA radiometers, NOAA Technical Memorandum NESS 107--Rev. 1: Washington, D.C., National Oceanic and Atmospheric Administration, National Environmental Satellite, Data, and Information Service [variously paged].
Disclaimer: Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Government.
ADAPS -- AVHRR Data Acquisition and Processing System
ASCII -- American Standard Code for Information Interchange
AVHRR -- Advanced Very High Resolution Radiometer
CDA -- Command and Data Acquisition
DACS -- Data Acquisition and Control Subsystems
DCW -- Digital Chart of the World
DOMSAT -- DOMestic SATellite
EDC -- EROS Data Center
LP DAAC -- Land Processes Distributed Active Archive Center
eosdis -- Earth Observing System Data and Information System
GELDS -- Gridded Earth Location and Determination System
GMT -- Greenwich Mean Time
HRPT -- High Resolution Picture Transmission
IFOV -- Instantaneous Field of View
LAC -- Local Area Coverage
NEdT -- Noise Equivalent Differential Temperature
NESDIS -- National Environmental Satellite, Data and Information Service
NOAA -- National Oceanic and Atmospheric Administration
POES -- Polar Orbiting Environment Satellite
RMSE -- Root Mean Square Error
SBBC -- Solar Blackbody Contamination
TIP -- TIROS Information Processor
TIROS -- Television and Infrared Observation Satellite
URL -- Uniform Resource Locator
EOSDIS Acronym List
Document Revision Date: January 27, 2004
Document Review Date: May 28, 1997
Document Curator: EDC staff
Document URL:
http://eosims.cr.usgs.gov:5725/DATASET_DOCS/avhrr_dataset.html