On Monday, 11 July from 3:00 p.m. through Wednesday, 13 July until 5:00 p.m., NSIDC data distribution, services, and Web site will be unavailable to accommodate a major upgrade to our data center. We apologize for any inconvenience this may cause you. Need to talk to us? You can always contact our friendly User Services Office at email@example.com or + 1 303.492.6199.
The Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperature product provides near-real-time brightness temperatures for both the Northern and Southern Hemispheres.
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. Zwally. 1999. Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures. [indicate subset used]. Edited by J. Maslanik and J. Stroeve. Boulder, Colorado USA: NASA DAAC at the National Snow and Ice Data Center.
DMSP 5D-2/F13, DMSP 5D-3/F17, DMSP 5D-2/F15
North and south polar regions
25 km, 12.5 km
1 July 1999 - present
2-byte scaled integer data
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Warning: 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), NSIDC will be distributing data from both the F17 and F18 satellites, starting with 1 April 2016 data. Using data from the 37V channel from the F17 satellite is not recommended. Instead, you should use data from the F18 satellite's 37V channel.
These brightness temperatures are used to generate Near-Real-Time DMSP SSM/I-SSMIS Daily Polar Gridded Sea Ice Concentrations. Near-real-time passive microwave brightness temperatures are received daily from the Special Sensor Microwave Imager/Sounder (SSMIS) on board the Defense Meteorological Satellite Program (DMSP) F17 satellite, and are gridded onto the SSM/I polar stereographic grid. The SSMIS instrument is the next generation Special Sensor Microwave/Imager (SSM/I) instrument. 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 via FTP 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. These data will be retained on the FTP site until NSIDC's standard brightness temperature product, DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures, is available.
Typically, NSIDC receives the standard SSM/I brightness temperatures from Remote Sensing Systems, Inc. (RSS), who derive them from SSM/I antenna temperatures, between three and six months after the initial satellite overpass. NSIDC chose to provide near-real-time brightness temperatures to facilitate time-sensitive research dependent upon precise detection of seasonal polar sea ice formation and break up. Daily brightness temperatures consist of seven files, one for each channel and polarization, for each hemisphere.
Possible differences between the standard and near-real-time products remain to be determined. The near-real-time data do not supplant the standard products, but instead fill the gap in time between present-day and the delivery of the RSS data. Users are therefore cautioned to be aware of potential data differences and should continue to use the standard products derived from the RSS data for time series analyses.
Note: 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.
Near-real-time data will remain on-line and available to users for three months after receipt of NSIDC's standard products from RSS. The file naming convention allows users to easily distinguish the near-real-time data from the standard SSM/I brightness temperatures.
For general information about these data, please see the DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures. Users interested in understanding how the near-real-time data were acquired and processed should review the Near-Real-Time SSM/I-SSMIS EASE-Grid Daily Global Ice Concentration and Snow Extent documentation.
The near-real-time brightness temperature files are stored as 2-byte scaled integer data.
The data reside on FTP in the ftp://sidads.colorado.edu/pub/DATASETS/nsidc0080_nrt_polar_stereo_tbs/ directory. Within this directory there is one folder: F18 and a listing of data files. The F18 folder contains the date from the F18 satellite and the listing of data files are data from the F17 satellite.
The data files are named according to the following convention and as described in Table 1:
|tb||Indicates this file contains brightness temperature data|
|fxx||Indicates which DMSP satellite the data came from (f13:
DMSP-F13; f15: DMSP-F15; f17:
Note: DMSP-F13 and -F15 data currently retained in the FTP directory should be used for intercomparison purposes only.
|nrt||Indicates that data are near-real-time|
|R||Region (n: north; s: south)|
|CC||Channel (19: 19 GHz, 22: 22 GHz, 37: 37 GHz, 85: 85 GHz, or 91:91 GHz)|
|P||Polarization (h: horizontal, v: vertical)|
|.bin||Identifies this as a binary data file|
Distribution size: 200 - 1100 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.
The data are available from 1 July 1999 to present.
The temporal resolution is daily
Data are available via FTP.
Table 2 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)|
|mapll.for and mapxy.for|
|psn12lats_v3.dat and pss12lats_v3.dat|
|psn12lons_v3.dat and pss12lons_v3.dat|
|psn25lats_v3.dat and pss25lats_v3.dat|
|psn25lons_v3.dat and pss25lons_v3.dat|
|Pixel-Area||psn12area_v3.dat and pss12area_v3.dat|
|psn25area_v3.dat and pss25area_v3.dat|
|Land Masks||gsfc_12n.msk and gsfc_12s.msk|
|gsfc_25n.msk and gsfc_25s.msk|
|Land Overlays||coast_12n.msk and coast_12s.msk|
|coast_25n.msk and coast_25s.msk|
|ltln_12n.msk and ltln_12s.msk|
|ltln_25n.msk and ltln_25s.msk|
The DMSP-F13 satellite that has been central to our brightness temperature products for the past several years is nearing the end of its mission and is no longer a reliable resource for our brightness temperature products. As is standard data practice, we have transitioned to a newer sensor. As of 02 June 2009, NSIDC has switched its SSM/I processing stream from the DMSP-F13 satellite to SSMIS data from the DMSP-F17 satellite. For data continuity, F17 data have been acquired and processed back to 01 April 2008.
One year earlier, 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.
However, although you may choose to use data from either the F13 or F15 satellites, NSIDC recommends using these data for intercomparison purposes only. SSMIS data from the DMSP-F17 satellite are used for the current near-real-time product. Regarding the F13 and F15 data, you should be aware of the following differences:
Regarding the F17 data, users should note a difference in the high frequency channel. The SSMIS sensor is similar to the SSM/I sensor 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 has been 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 SSMIS Instrument Description Web page.
01 December 1999
Document Revisions Dates