This data set provides brightness temperature data, acquired during the Soil Moisture Experiment 2002 (SMEX02) by the Special Sensor Microwave/Imagery (SSM/I).
SMEX02 SSM/I Brightness Temperature Data, Iowa, Version 1
This is the most recent version of these data.
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Geographic Coverage |
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As a condition of using these data, you must cite the use of this data set using the following citation. For more information, see our Use and Copyright Web page.
Jackson, T. and J. Wen. 2003. SMEX02 SSM/I Brightness Temperature Data, Iowa, Version 1. [Indicate subset used]. Boulder, Colorado USA. NASA National Snow and Ice Data Center Distributed Active Archive Center. doi: https://doi.org/10.5067/WK4WA91H9B1Z. [Date Accessed].Detailed Data Description
Data are provided in ASCII text format.
The data files use the following convention:
TDmmddyysstttt.rr.txt
where:
mm=month
dd=day
yyyy=year
ss=satellite number
tttt=start time of swath (hour and minute of local standard time)
rr=frequency set (lo or hi)
For example, the file "TD04302002150312.lo.txt" was acquired on April 30, 2002 from the F15 satellite at 3:12 AM, and the frequency is low. Low-frequency files contain brightness temperatures for 19.3, 22.22, and 37.0 GHz, while high-frequency files contain brightness temperatures for the 85.5 GHz channel.
File sizes range from 33 bytes to 244 KB.
Total volume is 175 MB.
Southernmost Latitude: 34.5°N
Northernmost Latitude: 44.5°N
Westernmost Longitude: 100°W
Easternmost Longitude: 90.0°W
Data were acquired from 29 April and 13 July 2002.
Temporal Resolution
For a given satellite, coverage is possible twice a day, approximately 12 hours apart, on the ascending and descending passes.
Parameter Description
The following table describes the data columns for the low frequency (.lo.txt) files:
Column | Parameter |
---|---|
1 | Latitude in degrees North |
2 | Longitude in degrees West |
3 | 19 GHz V TB |
4 | 19 GHz H TB |
5 | 22 GHz V TB |
6 | 37 GHz V TB |
7 | 37 GHz H TB |
The following table describes the data columns for the high frequency (.hi.txt) files:
Column | Parameter |
---|---|
1 | Latitude in degrees North |
2 | Longitude in degrees West |
3 | 85 GHz V TB |
4 | 85 GHz H TB |
Unit of Measurement
Unit of measurement is brightness temperature (TBs).
Sample Data Record
The following is a sample from the file "TD04302002141607.lo.txt."
44.46 -99.63 268.11 261.98 268.53 266.66 263.45 44.36 -99.92 263.14 254.22 264.36 262.16 255.76 44.45 -99.17 271.20 264.89 269.96 268.66 264.65 44.35 -99.46 268.16 261.98 268.36 266.83 263.48 44.24 -99.75 264.23 254.94 263.38 260.59 254.14
The next sample is from the file "TD04302002141607.hi.txt."
44.46 -99.87 265.55 262.71 44.46 -99.63 265.66 263.68 44.41 -99.78 262.97 260.78 44.36 -99.92 261.02 257.87 44.45 -99.40 267.14 263.88 44.40 -99.55 264.68 262.11
Software and Tools
Data Acquisition and Processing
Data were available to the investigators as antenna temperatures. Latitude and longitude coordinates for each pixel were included with these records. Each orbit consisted of about 5 mb of data in compressed mode. When a study area was specified in the data search procedure, all orbits that cross that area were extracted. For an individual satellite, two orbits might cover parts of the study area. On a given day, it was possible to have coverage by each of the three satellites twice a day. It was also possible to have no coverage. During the SMEX02 period from April 29 to July 13th, SSM/I overpasses were available.
Processing Steps
The raw SSM/I data sets were acquired and further processed by reducing the data set size by eliminating scans without coverage in the SMEX02 region, converting the antenna temperatures to brightness temperatures, and reformatting the data into ASCII files. The processed data files include a latitude and longitude assigned to each data point. Data are provided as separate files for low- (19.3, 22.2, and 37.0) and high-frequency channels (85 GHz) because the frequency of measurement is higher for 85 GHz.
The SSM/I instrument package has been available on at least one Defense Meteorological Satellite Program (DMSP) satellite since 1987. It is a conical scanning microwave radiometer system operating at a look angle of 53°. The following table summarizes the key features of the instruments. The nominal swath width is 1400 km. Data are collected at 128 locations across track on every scan at 85 GHz. Only 64 observations are made across track on every other scan at the other frequencies.
Frequency (GHz) | Polarization | Spatial Resolution (km) |
---|---|---|
19.3 | H and V | 69 x 43 |
22.2 | V | 60 x 40 |
37.0 | H and V | 37 x 28 |
85.5 | H and V | 15 x 13 |
The next table lists the characteristics of the various platforms that were in operation during SMEX02. For a given satellite, coverage is possible twice a day, approximately 12 hours apart, on the ascending and descending passes.
Spacecraft | Launch Date | Supported Through | Ascending Equatorial Crossing Time (LTZ) |
---|---|---|---|
F13 | March 1995 | present | 18:15 |
F14 | May 1997 | present | 20:21 |
F15 | December 1999 | present | 21:31 |
For more information, see the Summary of SMMR, SSM/I, SSMIS Sensors Document.
References and Related Publications
Contacts and Acknowledgments
Thomas J. Jackson
Jun Wen
US Department of Agriculture (USDS) Agricultural Research Service (ARS) Hydrology Lab.
Document Information
DOCUMENT CREATION DATE
December 2003