The Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperature product provides near-real-time polar stereographic gridded daily brightness temperatures for both the Northern and Southern Hemispheres.
Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures, Version 1
|Temporal Resolution:||1 day|
|Platform(s)||DMSP 5D-3/F17, DMSP 5D-3/F18|
|Data Contributor(s):||Jim Maslanik|
|Metadata XML:||View Metadata Record|
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.Cavalieri, D. J., P. Gloersen, and H. J. Zwally. Edited by J. Maslanik and J. Stroeve. 1999. Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures, Version 1. [Indicate subset used]. Boulder, Colorado USA. NASA National Snow and Ice Data Center Distributed Active Archive Center. doi: http://dx.doi.org/10.5067/AKQDND71ZDLF. [Date Accessed].
Detailed Data Description
Near-real-time passive microwave gridded daily brightness temperatures data are received daily from the Special Sensor Microwave Imager/Sounder (SSMIS) on board the Defense Meteorological Satellite Program (DMSP) F18 satellite, and are gridded onto the polar stereographic grid. SSMIS data used for this data set are received from the Comprehensive Large Array-data Stewardship System (CLASS) at the National Oceanic and Atmospheric Administration (NOAA). Two-byte scaled integer data are available at a resolution of 25 km for the 19, 22, and 37 GHz channels, and at 12.5 km resolution for the 85 GHz and 91GHz channels. NSIDC plans daily updates to the data.
The near-real-time data do not supplant the standard DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures data set product, but instead fill the gap in time between present-day and the delivery of the DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures data set. Therefore, users are cautioned that data differences may exist and should use the standard product when available. Also, these data may contain errors and are not suitable for time series, anomalies, or trends analyses. Near-real-time products do not undergo quality assessment and are therefore not intended for operational use.
The near-real-time brightness temperature files are stored as 2-byte scaled integer binary data
The data reside on FTP in the
ftp://sidads.colorado.edu/pub/DATASETS/nsidc0080_nrt_polar_stereo_tbs/ directory. Within this directory, the data for the F17 satellite goes through 3/31/2016, and the data for the F18 satellite starts on 4/1/2016..
This section explains the file naming convention used for this product with an example.
Example File Name: tb_f18_20160724_nrt_s19v.bin
Refer to Table 1 for the valid values for the file name variables listed above.
||Indicates this file contains brightness temperature data|
||Indicates which DMSP satellite the data came from (
||Indicates that data are near-real-time|
||Identifies this as a binary data file
Distribution size: 200 - 1064 KB
North and south polar regions
The spatial resolution is 25 km for the 19, 22, and 37 GHz channels, and at 12.5 km resolution for the 85 GHz and 91GHz channels.
Projection and Grid Description
The gridded brightness temperature data are displayed in polar stereographic projection. For more information, see Polar Stereographic Projections and Grids. The grid size varies depending on the region and frequency as shown in Table 2.
|North||85.5 GHz or 91.7 GHz||608||896|
|South||85.5 GHz or 91.7 GHz||632||664|
Brightness temperature is the effective temperature of a blackbody radiating the same amount of energy per unit area at the same wavelength as the observed body. This is also called effective temperature.
Brightness temperatures are calculated at the following channels: 19.3V, 19.3H, 22.2V, 37.0V, 37.0H, 85.5V, 85.5H, 91.7V, and 91.7H. The SSM/I uses the 85.5V and 85.5H channels and the SSMIS uses the 91.7V channel. Nine channels result from vertical and horizontal polarization for each frequency, except 22.2 GHz, which is vertical only. Brightness temperature values are precise to 0.01 K.
Unit of Measurement
Brightness temperatures are measured in kelvins (K).
Data are stored as scaled 2-byte integers representing brightness temperature values (in tenths of a kelvin), ranging from 50 K to 350 K. The brightness temperatures are multiplied by a factor of ten so that the precision of the data and the units in the data file are tenths of a kelvin. For example, a stored integer value of 2358 represents a brightness temperature value of 235.8 K. A value of 0 represents missing data.
Software and Tools
Tools for reading and displaying the brightness temperature files are available via FTP. Included are tools to extract the files; determine geolocation (geocoordinates) of data; display, extract and export the data; and masking tools that limit the influence of non-sea ice brightness temperatures.
The tools are divided into directories on the FTP site as shown in Figure 1.
Table 3 lists the tools that can be used with this data set. For a comprehensive list of all polar stereographic tools and for more information, see the Polar Stereographic Data Tools Web page.
|Tool Type||Tool File Name(s)|
Data Acquisition and Processing
The SSMIS instrument is a microwave radiometer that senses emitted microwave radiation from the Earth's surface. This radiation is affected by surface and atmospheric conditions, and thus provides a range of geophysical information.
These near-real-time SSMIS gridded brightness temperature data are computed daily from swath brightness temperatures obtained from CLASS at NOAA.
SSMIS data from the DMSP-F18 satellite are used in the current near-real-time product starting with 4/1/2016 to present.
Due to the compromised data integrity with the DMSP F17 vertically polarized 37 GHz channel (37V) of the Special Sensor Microwave Imager and Sounder (SSMIS) in April, 2016, NSIDC started distributing data from the F18 satellite on 1 April 2016.
SSM/I Data from the DMSP-F13 Satellite Switched to SSMIS Data from the DMSP-F17 Satellite
On 02 June 2009, NSIDC switched its SSM/I data processing stream from the DMSP-F13 satellite to the SSMIS data processing stream from the DMSP-F17 satellite because the DMSP-F13 satellite came to the end of its mission and no longer produced reliable data. For data continuity, F17 data were processed back to 01 April 2008.
Note: The SSMIS sensor on the F17 satellite is similar to the SSM/I sensor on the F13 satellite and has the same low frequency channels: dual-polarized 19 GHz and 37 GHz channels, and a vertically polarized 22 GHz channel. However, the high-frequency 85.5 GHz channel on SSM/I was replaced by a 91 GHz channel on SSMIS. Users should note that the different frequency will affect any products that employ a high frequency channel. Any such products should be evaluated for the impact of the different frequency and adjustments may be necessary for consistent products. For more information regarding the SSMIS instrument, refer to the Special Sensor Microwave Imager/Sounder (SSMIS) Web page.
SSM/I Data from the DMSP-F13 Satellite Switched to the DMSP-F15 Satellite
On 02 June 2008, NSIDC switched its SSM/I processing stream from the DMSP-F13 satellite to the DMSP-F15 satellite due to a failing recorder on F13. For continuity, F15 data were acquired and processed from 01 January 2008 until 25 February 2009. On 16 February 2009, however, NSIDC switched its SSM/I processing stream back to the DMSP-F13 satellite due to an issue with the DMSP-F15 SSM/I 22 GHz frequency brightness temperature fields. NSIDC continued to produce the F13 products until further degradation of the SSM/I instrument on 11 May 2009. Processed F13 data are available for the 01 July 2008 through 11 May 2009 time period.
The SSMIS sensor is a conically-scanning passive microwave radiometer that harnesses the imaging and sounding capabilities of three previous DMSP microwave sensors, including the SSMI, the SSM/T-1 temperature sounder, and the SSMI/T-2 moisture sounder. The SSMIS sensor measures microwave energy at 24 frequencies from 19 to 183 GHz with a swath width of 1700 km. For more information regarding the SSMIS instrument, refer to the Special Sensor Microwave Imager/Sounder (SSMIS) Web page.
Contacts and Acknowledgments
James Maslanik -Retired
Research Professor Emeritus
Aerospace Engineering Sciences
University of Colorado at Boulder
Boulder, CO 80309-0431
Document Revision Dates:
29 July 2016
20 June 2009
02 June 2009
13 January 2009
27 May 1999
Document ID: nsidc-0080
NSIDC User Services
Phone: 1 303 492-6199
Fax: 1 303 492-2468
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