Sea Ice Concentrations from Nimbus-7 SMMR and DMSP SSM/I Passive Microwave Data

Summary

This data set is generated from brightness temperature data derived from Nimbus-7 Scanning Multichannel Microwave Radiometer (SMMR) and Defense Meteorological Satellite Program (DMSP) -F8, -F11 and -F13 Special Sensor Microwave/Imager (SSM/I) radiances at a grid cell size of 25 x 25 km. The data are provided in the polar stereographic projection.

This product is designed to provide a consistent time series of sea ice concentrations (the fraction, or percentage, of ocean area covered by sea ice) spanning the coverage of several passive microwave instruments. To aid in this goal, sea ice algorithm coefficients are changed to reduce differences in sea ice extent and area as estimated using the SMMR and SSM/I sensors. The data are generated using the NASA Team algorithm developed by the Oceans and Ice Branch, Laboratory for Hydrospheric Processes at NASA Goddard Space Flight Center (GSFC).

These data include gridded daily (every other day for SMMR data) and monthly averaged sea ice concentrations for both the north and south polar regions. Two types of data are provided: final data and preliminary data. Final data are produced at GSFC about once per year, with roughly a one-year latency, and include data since 26 October 1978. Final data are produced from SMMR brightness temperature data processed at NASA GSFC and SSM/I brightness temperature data processed at the National Snow and Ice Data Center (NSIDC). Preliminary data are produced at NSIDC approximately every three months (quarterly), using SSM/I data acquired from Remote Sensing Systems, Inc. (RSS), and include roughly the most recent three to twelve months of processed data.

Data are scaled and stored as one-byte integers in flat binary arrays. For each data file, a corresponding PNG browse image file is provided. Data are available via FTP.

Citing These Data

While the final and preliminary data are reasonably consistent, the particular type of data used for any publication, presentation, or other application should be clearly stated. The following examples show how to cite the use of this data set in a publication. The citation to use depends on whether final or preliminary data were used; if both were used, please cite each type. List the principal investigators, year of data set release, data set title, dates of data used (for example, 01 January to 15 March 2004), publisher (NSIDC), and media format.

To broaden awareness of our services, NSIDC requests that you acknowledge the use of data sets distributed by NSIDC. Please refer to the citation below for the suggested form, or contact NSIDC User Services for further information. We also request that you send us one reprint of any publication that cites the use of data received from our Center. This helps us to determine the level of use of the data we distribute. Thank you.

Final Data
Cavalieri, D., C. Parkinson, P. Gloersen, and H. J. Zwally. 1996, updated 2006. Sea ice concentrations from Nimbus-7 SMMR and DMSP SSM/I passive microwave data, [list dates of temporal coverage used]. Boulder, Colorado USA: National Snow and Ice Data Center. Digital media.

Preliminary Data
Meier, W., F. Fetterer, K. Knowles, M. Savoie, M. J. Brodzik. 2006, updated quarterly. Sea ice concentrations from Nimbus-7 SMMR and DMSP SSM/I passive microwave data, [list dates of temporal coverage used]. Boulder, Colorado USA: National Snow and Ice Data Center. Digital media.

Overview Table

Category Description
Data format One-byte (scaled integer) flat binary arrays preceded by a 300-byte header; PNG browse images
Spatial coverage and resolution North and south polar regions at 25 km resolution
Temporal coverage and resolution Final data: 26 October 1978 through the most current processing
Preliminary data: The most recent three to twelve months of processed data

SMMR data collected every other day; SSM/I data collected daily
Tools for accessing data Software and tools for reading and displaying data are available via FTP.
Data range 0 to 250 (fractional coverage scaled by 250; percentage scaled by 2.5)
Grid type and size See Polar Stereographic Projections and Grids. Grid size varies by region:
North: 304 columns x 448 rows
South: 316 columns x 332 rows
File naming convention
Final daily: nt_YYYYMMDD_SSS_vVV_R.bin
Final monthly: nt_YYYYMM_SSS_vVV_R.bin
Preliminary daily: nt_YYYYMMDD_f13_pre_R.bin
Preliminary monthly: nt_YYYYMM_f13_pre_R.bin
File size North: 136492 bytes
South: 105212 bytes
Parameter Sea ice concentration
Procedures for obtaining data Data are available via FTP.

Table of Contents

1. Contacts and Acknowledgments
2. Detailed Data Description
3. Data Access and Tools
4. Data Acquisition and Processing
5. References and Related Publications
6. Document Information

1. Contacts and Acknowledgments

Investigators

Final data investigators:

Donald J. Cavalieri, Claire L. Parkinson, Per Gloersen, and H. Jay Zwally
NASA Goddard Space Flight Center (GSFC)
Greenbelt, Maryland USA

Preliminary data investigators:

Walt Meier, Florence Fetterer, Ken Knowles, Matt Savoie, Mary Jo Brodzik
National Snow and Ice Data Center (NSIDC)
Boulder, Colorado USA

Technical Contact

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

2. Detailed Data Description

This data set is a sea ice concentration time series generated from brightness temperature data derived from SMMR and SSM/I radiances. The data set includes gridded daily (every other day for SMMR data) and monthly averaged sea ice concentrations for both the north and south polar regions from 26 October 1978 through the most current processing. No data coverage is available for regions poleward of 84.5° N latitude for SMMR and poleward of 87° N latitude for SSM/I, due to the inclination of the platform orbits. SMMR data were acquired every other day, while SSM/I data are acquired daily.

The goal of this data set is to provide a long term, consistent sea ice concentration product in which sea ice extent and area differences between the sensors are reduced and could serve as a baseline for future measurements. To achieve this, it is necessary to address differences between the SMMR and the DMSP-F8, -F11, and -F13 SSM/I sensors. This document describes the basic characteristics of the SMMR and SSM/I platforms and summarizes the problems encountered when deriving sea ice concentrations from brightness temperatures measured by sensors with different frequencies, different footprint sizes, different visit times, and different calibrations. A major obstacle to resolving these differences is the lack of sufficient overlapping data from sequential sensors. The techniques employed to solve these problems, or at least reduce their impacts, include:

Basic limitations also arise from the sensor resolution, temporal coverage, and algorithm assumptions and characteristics. The NASA Team algorithm is not designed to provide ice concentration for fresh-water ice (for example, lake and river ice). The filtering used to remove land-to-ocean spillover may affect the area of some open water features within the ice pack near coasts (coastal polynyas).

Using These Data

Potential applications for these sea ice concentration data include:

Users should be aware that the ice concentration maps were derived from algorithms that were "tuned" to minimize the differences in ice extent and ice covered area during the overlap periods when transitioning from one instrument to the next (overlap from SMMR to DMSP-F8 SSM/I, from DMSP-F8 to -F11 SSM/I, and from DMSP-F11 to -F13 SSM/I). This does not mean that the ice concentrations themselves are well matched. See the Data Verification by Data Center section of this document for a summary of ice extent and ice covered area differences during the overlap periods.

It is also important to know that SMMR and SSM/I have different data gaps at the North Pole due to orbital differences. Therefore, any time series of parameters, such as ice extent and ice covered area, need to take these differences into account. A pole mask is provided for this purpose (see the Masks and Overlays section).

Particular care is needed to interpret the sea ice concentrations during summer when melt is present, and in regions where new sea ice makes up a substantial part of the sea ice cover. Some residual errors remain due to weather effects and mixing of ocean and land area within the sensor field of view, and due to sensor differences.

It is recommended that sea ice extent and area be computed from daily maps of ice concentrations that are then used to compute monthly averages of those parameters. Computations of sea ice extents and sea ice areas should not be made from the monthly-averaged ice concentration maps because that may result in a biased time series.

Final and Preliminary Data

Two types of data are provided: final data and preliminary data. Final data are produced at GSFC about once per year, with roughly a one-year latency, and include data since since 26 October 1978. Preliminary data are produced at NSIDC approximately every three months (quarterly), using data acquired from Remote Sensing Systems, Inc. (RSS), and include roughly the most recent three to twelve months of processed data. When final data are available, they replace any preliminary data for the same time period. Therefore, this product contains only one sea ice concentration file (final or preliminary) for any given time period.

Preliminary and final data are processed almost identically. The differences are:

For more information about the data acquired from RSS, see the DMSP SSM/I Daily Polar Gridded Brightness Temperatures data set.

Format

Data are scaled flat binary with one byte per pixel. Data are stored as one-byte integers representing scaled sea ice concentration values. See the Parameter Range section for more information. For each data file, a corresponding browse image file in PNG format is also provided.

The file format consists of a 300-byte descriptive header followed by a two-dimensional array of one-byte values containing the data. The file header is composed of:

For compatibility with ANSI C, IDL, and other languages, character strings are terminated with a NULL byte.

The file header can be accessed in a variety of ways. For example, it can be treated as a simple sequence of bytes containing ASCII character strings or as a complex data structure of arrays. The following table describes the file header.

File Header
Bytes Description
1-6 Missing data integer value
7-12 Number of columns in polar stereographic grid
13-18 Number of rows in polar stereographic grid
19-24 Unused/internal
25-30 Latitude enclosed by polar stereographic grid
31-36 Greenwich orientation of polar stereographic grid
37-42 Unused/internal
43-48 J-coordinate of the grid intersection at the pole
49-54 I-coordinate of the grid intersection at the pole
55-60 Five-character instrument descriptor (SMMR, SSM/I)
61-66 Two descriptors of two characters each that describe the data;
for example, 07 cn = Nimbus-7 SMMR ice concentration
67-72 Starting Julian day of grid data
73-78 Starting hour of grid data (if available)
79-84 Starting minute of grid data (if available)
85-90 Ending Julian day of grid data
91-96 Ending hour of grid data (if available)
97-102 Ending minute of grid data (if available)
103-108 Year of grid data
109-114 Julian day of grid data
115-120 Three-digit channel descriptor (000 for ice concentrations)
121-126 Integer scaling factor
127-150 24-character file name
151-230 80-character image title
231-300 70-character data information (creation date, data source, etc.)

The data can be read with image processing software by specifying a 300-byte header, with an image size of 304 columns x 448 rows for Arctic data and 316 columns x 332 rows for Antarctic data. In a high-level programming language or image processing software, declare a 300-byte array for the header and an array (for example, 304 x 448 for Arctic) for the image. Read the 300-byte array first, then read the image array.

File and Directory Structure

Data are on the FTP site in the /pub/DATASETS/seaice/polar-stereo/nasateam/ directory. Final and preliminary data are in separate directories within /nasateam/, named final-gsfc and preliminary, as shown below.

Within the final-gsfc and preliminary directories are north and south directories that contain data files, and a browse directory that contains browse image PNG files. Daily and monthly data are further separated into directories named daily and monthly. For final daily data, there is also one directory for each year of available data. For example, all of the final north daily data for 1990 are in a directory named /seaice/polar-stereo/nasateam/final-gsfc/north/daily/1990/.

The directory structure is illustrated below; not all directories are shown fully expanded. The structure for each south directory matches that of the corresponding north directory. Each browse directory is divided into a structure that reflects that of the data. In this illustration, the year directories underneath final-gsfc are representative placeholders; on the FTP site, there are actually many such directories, each named for the year of data it contains, such as 1987, 2000, etc.

File Naming Convention

Final Data

The file naming convention for the final daily data is nt_YYYYMMDD_SSS_vVV_R.bin, where the nt prefix indicates this was created with the NASA Team algorithm, the .bin extension indicates a binary file, and

SSS = sensor (n07 for Nimbus-7 SMMR; f08, f11, or f13 for DMSP-F8, -F11 or -F13 SSM/I)
YYYY = four-digit year
MM = two-digit month
DD = two-digit day
VV = data version number (for example, 01)
R = region (n = north; s = south)

For example, nt_20030115_f13_v01_n.bin is the final daily file from sensor DMSP-F13 for the date 15 January 2003; it is Version 01 data for the north region.

The file naming convention for the final monthly data is nt_YYYYMM_SSS_vVV_R.bin, where the nt prefix indicates this was created with the NASA Team algorithm, the .bin extension indicates a binary file, and

SSS = sensor (n07 for Nimbus-7 SMMR; f08, f11, or f13 for DMSP-F8, -F11 or -F13 SSM/I)
YYYY = four-digit year
MM = two-digit month
VV = data version number (for example, 01)
R = region (n = north; s = south)

For example, nt_200301_f13_v01_n.bin is the final monthly file from sensor DMSP-F13 for January 2003; it is Version 01 data for the north region.

Preliminary Data

The file naming convention for the preliminary daily data is nt_YYYYMMDD_f13_pre_R.bin, where the nt prefix indicates this was created with the NASA Team algorithm, f13 indicates data are from the DMSP-F13 sensor, pre indicates these are preliminary data, the .bin extension indicates a binary file, and

YYYY = four-digit year
MM = two-digit month
DD = two-digit day
R = region (n = north; s = south)

For example, nt_20060715_f13_pre_n.bin is the preliminary daily file for the north polar region for 15 July 2006.

The file naming convention for the preliminary monthly data is nt_YYYYMM_f13_pre_R.bin, where the nt prefix indicates this was created with the NASA Team algorithm, f13 indicates data are from the DMSP-F13 sensor, pre indicates these are preliminary data, the .bin extension indicates a binary file, and

YYYY = four-digit year
MM = two-digit month
R = region (n = north; s = south)

For example, nt_200607_f13_pre_n.bin is the preliminary monthly file for the north polar region for July 2006.

Browse Images

Browse image files are named using the same convention as the data files, except the file extension is .png extension instead of .bin.

File Size

Data file size varies by region:

North:  136492 bytes
South:  105212 bytes

Spatial Coverage

Data set coverage includes the polar regions defined by the Polar Stereographic Projections and Grids spatial coverage map.

SSM/I instrument coverage is global, except for circular sectors centered over the pole, 280 km in radius, located poleward of 87°. These sectors are never measured due to orbit inclination. The measurement footprint size (effective field of view) varies by frequency, as shown in the following table.

SSM/I
Frequency Footprint Size
19.3 GHz 70 x 45 km
22.2 GHz 60 x 40 km
37.0 GHz 38 x 30 km

SMMR instrument coverage is global, except for circular sectors centered over the North pole, approximately 611 km in radius, located poleward of 84.5°. These sectors are never measured due to orbit inclination. The 50° scan pattern provided a swath width of 780 km at the Earth's surface. The spatial resolutions at the various frequencies ranged from approximately 27 km at 37 GHz to 148 km at 6.6 GHz. The measurement footprint size varies by frequency, as shown in the following table.

SMMR
Frequency Footprint Size
6.6 GHz 148 x 95 km
10.7 GHz 91 x 59 km
18.0 GHz 55 x 41 km
21.0 GHz 46 x 30 km
37.0 GHz 27 x 18 km

Projection and Grid Description

The sea ice concentration data are displayed in polar stereographic projection. For more information, see Polar Stereographic Projections and Grids. The grid size varies depending on the region, as shown in the following table.

Region Columns Rows
North 304 448
South 316 332

Temporal Coverage

Final data are from 26 October 1978 through the most current processing. See the Data Acquisition Methods section for dates by instrument and platform.

Preliminary data are for about the most recent three to twelve months of processing.

Temporal Resolution

The SMMR instrument scanner operated only on alternate days, due to spacecraft power limitations. Therefore, SMMR data were only collected every other day. Typically, there are at least 14 days of coverage per month, although there are major data gaps in August of 1982 (4, 8, and 16 August 1982) and August of 1984 (13 through 23 August 1984) for both polar regions.

SSM/I data were and continue to be collected daily. A major data gap in the SSM/I data exists from 3 December 1987 to 13 January 1988.

Sea ice concentrations are provided for each day of data and also as monthly means. The monthly means are generated by averaging all the available daily files for each individual month, excluding pixels of missing data (see the Monthly Data Generation section of this document for more information).

Parameter or Variable

Parameter Description

Sea ice concentration represents an areal coverage of sea ice. For a given grid cell, the parameter provides an estimate of the fractional amount of sea ice covering that cell, with the remainder of the area consisting of open ocean. Land areas are coded with a land mask value.

Parameter Source

Data sources are Nimbus-7 SMMR and DMSP-F8, -F11 and -F13 SSM/I instruments.

Parameter Range

Data are stored as one-byte integers representing sea ice concentration values. The sea ice concentration data are packed into byte format by multiplying the derived fractional sea ice concentration floating-point values (ranging from 0.0 to 1.0) by a scaling factor of 250. For example, a sea ice concentration value of 0.0 (0%) maps to a stored one-byte integer value of 0, and a sea ice concentration value of 1.0 (100%) maps to a stored one-byte integer value of 250. To convert to the fractional parameter range of 0.0 to 1.0, divide the scaled data in the file by 250. To convert to percentage values (0% to 100%), divide the scaled data in the file by 2.5.

Data files may contain integers from 0 to 255, as described in the following table.

Data Value Meaning
0 - 250 Sea ice concentration (fractional coverage scaled by 250)
251 Circular mask used in the Arctic to cover the irregularly-shaped data gap around the pole (caused by the orbit inclination and instrument swath)
252 Unused
253 Coastlines
254 Superimposed land mask
255 Missing data

Data Validation by Source

The performance of the NASA Team algorithm was assessed in numerous studies (for example, Cavalieri et al. 1992). These results apply to this data set. However, improvements in this data set that differ from previous studies include the minimization of coastal and open-ocean influences that tend to yield inaccurate sea ice concentrations. Visual data checking was used to assess the performance of these modifications.

Confidence Level/Accuracy Judgment

Estimates of the accuracy of the NASA Team algorithm vary depending on sea ice conditions, methods, and locations used in individual studies. Cavalieri et al. (1992) summarizes several of these studies. In general, accuracy of total sea ice concentration is within +/- 5% of the actual sea ice concentration in winter, and +/- 15% in the Arctic during summer when melt ponds are present on the sea ice. Accuracy tends to be best within the consolidated ice pack when the sea ice is relatively thick (greater than 20 cm) and ice concentration is high. Accuracy decreases as the proportion of thin ice increases. See Cavalieri et al. (1992), Steffen et al. (1992), and other listed references for an overview of the algorithm performance.

Data Verification by Data Center

NSIDC staff visually checks the data files and selected graphics files. This includes verification of proper file structure, comparisons to existing SMMR- and SSM/I-derived sea ice concentration grids, masks, and information files, and examination of data quality.

Some weather-related effects and land contamination are still present. The amount and spatial distribution of remaining weather effects vary with season. Also, occasional bad scan lines still appear in the data. Based on NSIDC analyses, some sensor-to-sensor differences are likely to remain in these data, particularly for marginal ice zones. See NSIDC Special Report 5: An Intercomparison of DMSP F11- and F13-derived Sea Ice Products for summaries of differences among the SSM/I sensors.

Residual weather effects and processing errors in May 1986 data result in large bands of very low ice concentrations over the open ocean in the Weddell, Bellingshausen, and Amundsen seas in the Southern Hemisphere. Although the magnitude of these false ice concentrations is less than one percent, users should be aware that such errors do occur in data for many days within that month.

Overlap periods exist when transitioning from one instrument to the next. These overlaps are from SMMR to DMSP-F8 SSM/I, from DMSP-F8 to -F11 SSM/I, and from DMSP-F11 to -F13 SSM/I. During overlap periods, data were available from two instruments, although good data may not be available from both instruments during the entire operating overlap. Differences in ice covered area and ice extent during the overlap periods were minimized by tuning the sea ice algorithms. Wavelet analysis of the time series of ice extent and ice covered area show no significant offsets between the different satellites.

The following tables summarize the comparison between the ice covered areas and ice extent during the overlap periods, including mean differences and linear regression results of ice covered areas and ice extent. Mean differences are computed for SMMR minus DMSP-F8 SSM/I, DMSP-F8 SSM/I minus DMSP-F11 SSM/I, and DMSP-F11 SSM/I minus DMSP-F13 SSM/I. Regression coefficients are computed using y = a0 + a1*x, for each (x, y) pair (x=SMMR, y=DMSP-F8 SSM/I); (x=DMSP-F8 SSM/I, y=DMSP-F11 SSM/I); and (x=DMSP-F11 SSM/I, y=DMSP-F13 SSM/I). While this analysis shows no significant differences between the overall summaries of ice covered area and ice extent, significant regional differences in ice concentration may still be present.

North
  Mean Difference
(x 106km2)
Standard Deviation
(x 106km2)
a0
(x 106km2)
a1
(x 106km2)
Correlation
Coefficient
% Difference
SMMR to DMSP-F8 SSM/I            
ice area 0.073 0.054 0.214 0.947 0.999 1.34%
ice extent 0.055 0.096 0.412 0.941 0.998 0.70%
DMSP-F8 to DMSP-F11 SSM/I            
ice area -0.019 0.036 0.955 0.914 0.996 0.18%
ice extent 0.002 0.058 0.351 0.972 0.983 0.01%
DMSP-F11 to DMSP-F13 SSM/I            
ice area -0.0112 0.0296 0.0079 0.997 0.999 0.18%
ice extent -0.0004 0.0457 0.0199 0.997 0.999 -0.01%

South
  Mean Difference
(x 106km2)
Standard Deviation
(x 106km2)
a0
(x 106km2)
a1
(x 106km2)
Correlation
Coefficient
% Difference
SMMR to DMSP-F8 SSM/I            
ice area 0.018 0.072 0.225 0.982 0.992 0.15%
ice extent 0.005 0.058 -0.198 1.011 0.998 0.0%
DMSP-F8 to DMSP-F11 SSM/I            
ice area -0.038 0.092 0.630 0.924 0.996 0.49%
ice extent 0.012 0.067 0.289 0.974 0.998 0.08%
DMSP-F11 to DMSP-F13 SSM/I            
ice area 0.0311 0.0344 -0.0474 1.007 0.999 0.26%
ice extent 0.0126 0.0402 -0.0186 1.002 0.999 0.08%

3. Data Access and Tools

Data Access

Data are available via FTP.

Software and Tools

Software for reading and displaying the files is available in the tools directory on the FTP site. Software includes IDL and Matlab routines to ingest and read sea ice concentration data. Masks and overlays are also provided.

Tools

Tools include files described in the following table.

File Description
showice.m A Matlab program that displays an image of the sea ice concentration grids in either of two color scales.
showice.pro An IDL program that displays images of the sea ice concentration grids or of the GIF files themselves (automatically). This program does not support the latitude and longitude files listed below. Also note that IDL Version 5.4 and higher does not support reading or writing GIF images. Users using IDL Version 5.4 and higher will therefore not be able to view the GIF images using this program. An alternative format for IDL 5.4 and higher is Portable Network Graphics (PNG).
psn25lats_v2.dat
pss25lats_v2.dat
Grids that determine the latitude of a given pixel for the 25 km grids for either hemisphere. These latitude grids are in binary format and are stored as 4-byte integers (little endian) scaled by 100,000 (divide the stored value by 100,000 to get decimal degrees). Each array location (i, j) contains the latitude value at the center of the corresponding data grid cells.

psn25lats_v2.dat: North, 304 columns x 448 rows
pss25lats_v2.dat: South, 316 columns x 332 rows
psn25lons_v2.dat
pss25lons_v2.dat
Grids that determine the longitude of a given pixel for the 25 km grids for either hemisphere. These longitude grids are in binary format and are stored as 4-byte integers (little endian) scaled by 100,000 (divide the stored value by 100,000 to get decimal degrees). Each array location (i, j) contains the longitude value at the center of the corresponding data grid cells.

psn25lons_v2.dat: North, 304 columns x 448 rows
pss25lons_v2.dat: South, 316 columns x 332 rows
psn25_area_v2.dat
pss25_area_v2.dat
Grids that determine the area of a given pixel for the 25 km grids for either hemisphere. The arrays are in binary format and are stored as 4-byte integers scaled by 1000. Each array location (i, j) contains the real value of the corresponding grid cell. Both arrays are 304 columns x 448 rows.

Note the data ranges given above are latitude and longitude values for the center of each grid cell. The range covered by the full grid extends to the pole (90° N or 90° S) and all longitudes (-180° to +180°).

Masks and Overlays

Masks and overlays provided include files described in the following table.

File Name Description
gsfc_25n.msk Northern 25 km land and coast mask
gsfc_25s.msk Southern 25 km land and coast mask
coast_25n.msk Northern 25 km coastline grid overlay
coast_25s.msk Southern 25 km coastline grid overlay
ltln_25n.msk Northern 25 km lat/lon grid overlay
ltln_25s.msk Southern 25 km lat/lon grid overlay
pole_n.msk Circular mask that symmetrically covers the observed maximum extent of the missing data (resulting from the orbit inclination and instrument swath) near the North Pole. This is a one-byte array of 304 columns and 448 rows with no header. The area of the SSM/I hole has a value of 1. The additional area of the SMMR hole (a ring around the SSM/I hole) has a value of 2. Everything else has a value of 0.
region_n.msk
region_s.msk
Region masks for the polar stereographic grid. For more information, see Region Masks below.
Region Masks

Two region masks for the polar stereographic grid are also provided. The files are region_n.msk (Arctic) and region_s.msk (Antarctic). These region masks are described further in "Arctic and Antarctic Sea Ice, 1978-1987 Satellite Passive Microwave Observations and Analysis," NASA SP-511. The region mask file contains a 300-byte header, followed by a two-dimensional byte array (304 columns by 448 rows for north polar region; 316 x 332 for south polar region), stored by rows in column order. Regions are assigned different pixel values as shown in the following table.

Pixel Value Arctic Region Antarctic Region
1
Non-regional ocean  
2
Sea of Okhotsk and Japan Weddell Sea
3
Bering Sea Indian Ocean
4
Hudson Bay Pacific Ocean
5
Baffin Bay/Davis Strait/Labrador Sea Ross Sea
6
Greenland Sea Bellingshausen Amundsen Sea
7
Kara and Barents Seas  
8
Arctic Ocean  
9
Canadian Archipelago  
10
Gulf of St. Lawrence  
11
Land Land
12
Coast Coast
0
Lakes, extended coast  

Ocean Masks and Images of Maximum Ice Extent

Please see the Sea Ice Trends and Climatologies from SMMR and SSM/I data set for information.

Related Data Collections

4. Data Acquisition and Processing

Theory of Measurements

The SMMR and SSM/I instruments are microwave radiometers that sense emitted microwave radiation. This radiation is affected by surface and atmospheric conditions, and thus provides a range of geophysical information.

Source/Platform

The Nimbus-7 and DMSP F-series spacecraft fly in near polar sun-synchronous orbits. The orbits are compared in the following table.

Comparison of Orbital Parameters
Parameter Nimbus-7 DMSP-F8 DMSP-F11 DMSP-F13
Nominal Altitude* 955 km 860 km 830 km 850 km
Inclination Angle 99.1 degrees 98.8 degrees 98.8 degrees 98.8 degrees
Orbital Period 104 minutes 102 minutes 101 minutes 102 minutes
Ascending Node Equatorial Crossing
(local time)
approximately 12:00 P.M. approximately 6:00 A.M. approximately 5:00 P.M. approximately 5:43 P.M.
Algorithm Frequencies* 18.0, 37.0 GHz 19.4, 37.0 GHz 19.4, 37.0 GHz 19.4, 37.0 GHz
Earth Incidence Angle* 50.2 53.1 52.8 53.4
3 dB Beam Width (degrees)* 1.6, 0.8 1.9, 1.1 1.9, 1.1 1.9, 1.1

*Indicates sensor and spacecraft orbital characteristics of the three sensors used in generating the sea ice concentrations.

Sensor or Instrument Description

The SMMR is a 10-channel instrument delivering orthogonally polarized antenna temperature data at five dual-polarized (horizontal, vertical) frequencies: 6.6 GHz, 10.7 GHz, 18.0 GHz, 21.0 GHz, and 37.0 GHz. Please see the SMMR Instrument Description for more details.

The SSM/I is a seven-channel, orthogonally polarized, passive-microwave radiometric system. The instrument measures combined atmosphere and surface radiances at 19.3 GHz, 22.2 GHz, 37.0 GHz and 85.5 GHz frequencies. Please see the SSM/I Instrument Description for more details.

Data Acquisition Methods

The combined SMMR and SSM/I sea ice concentration time series is produced from brightness temperatures obtained from GSFC and NSIDC. The four sets of satellite data currently used to create this data stream, and the time periods for which the data are usable, are shown in the following table.

Platform and Instrument Time Period
Nimbus-7 SMMR 26 October 1978 through 20 August 1987
DMSP-F8 SSM/I 9 July 1987 through 31 December 1991
DMSP-F11 SSM/I 3 December 1991 through 30 September 1995
DMSP-F13 SSM/I 3 May 1995 through the most recent data (data acquisition is ongoing)

SMMR
Sea ice concentrations were processed by GSFC using SMMR brightness temperatures. The SMMR brightness temperatures were processed and quality checked at GSFC (Gloersen et al. 1992).

SSM/I
DMSP-F8, -F11, and -F13 SSM/I brightness temperature data used to create this sea ice concentration time series (final data) are distributed by NSIDC. Processing of DMSP-F13 SSM/I brightness temperatures is ongoing. Data acquisition, filtering bad data, handling geolocation errors, implementation of an antenna pattern correction, and the swath-to-grid conversion are all described in the documentation for the DMSP SSM/I Daily and Monthly Polar Gridded Sea Ice Concentrations data set.

Derivation Techniques and Algorithms

This section is extracted from NASA Technical Memorandum 104647.

Sea ice concentrations for this data set were produced using a revised NASA Team algorithm that uses a different set of tie points and weather filters than the original NASA Team algorithm (see NASA Team Sea Ice Algorithm for a description of the original algorithm). NASA Technical Memorandum 104647 includes information about differences (e.g., tie points) between the original algorithm and the revised NASA Team algorithm. The NASA Team algorithm uses different channels of the SMMR and the SSM/I brightness temperature data:

Instrument Channels
SMMR  - vertically and horizontally polarized 18.0 GHz
 - vertically polarized 37.0 GHz
SSM/I  - vertically and horizontally polarized 19.4 GHz
 - vertically polarized at 37.0 GHz

The weather filter used for the SMMR (Gloersen and Cavalieri 1986) was found to be inadequate for the SSM/I because of the SSM/I's use of the 19.4 GHz channels (which are further up on the shoulder of the water vapor line at 22.2 GHz) rather than the 18.0 GHz channels. A different weather filter is used to reduce spurious sea ice concentrations from SSM/I that result from the presence of atmospheric water vapor, non-precipitating cloud liquid water, rain, and sea surface roughening by surface winds. This filter is a combination of the SSM/I 37.0 and 19.4 GHz channels, which effectively eliminates most of the spurious sea ice concentration measurements resulting from wind-roughening of the ocean surface, cloud liquid water, and rainfall. Another filter that is based on the 19.4 and 22.2 GHz channels is also used. The rationale behind combining the 19.4 and 22.2 GHz channels is based on the sensitivity of the 22.2 GHz to water vapor and on the need to minimize the effect of ice temperature variations at the ice edge.

Processing Steps

Platform and Sensor Differences

Comparisons of sea ice concentrations calculated for each sensor during overlap periods using published algorithm tie points reveal significant differences. These may result from differences in sensor and orbital characteristics, differences in observation times (and therefore tidal effects), or differences in algorithm coefficients. Sensor and orbital characteristic differences for the Nimbus-7 SMMR and DMSP-F8 SSM/I include antenna beam width, channel frequency, spacecraft altitude, ascending node time, and angle of incidence. In addition, the sea ice algorithm tie points are significantly different. The DMSP-F8, -F11, and -F13 sensors also differ in ascending node time, altitude, and angle of incidence. Because the visit times of the three DMSP satellites occur during different phases of the diurnal cycle, tidal effects may result in differences in the sea ice distribution. GSFC presumes that any such effects are mitigated by the correction scheme described below. The Comparison of Orbital Parameters table in the Source/Platform section summarizes sensor and orbital characteristic differences. The GSFC processing attempts to accommodate for these differences in each pair of sensors by employing a set of algorithm tie points determined through linear relationships between the observed brightness temperatures during the overlap periods.

Nimbus-7 SMMR and DMSP-F8 SSM/I Transition
Daily brightness temperature maps from the Nimbus-7 SMMR and from the DMSP-F8 SSM/I during their period of overlap, 9 July to 20 August 1987, were compared for both the Arctic and Antarctic. Unfortunately, there were only 22 days of common coverage. A linear, least squares best fit of the cumulative data was obtained for each of the corresponding channels. For the purpose of eliminating spurious brightness temperatures resulting from residual land spillover effects, an Arctic land mask that expanded three to four pixels out from the original land mask was used in the determination of the best fit between the two data streams.

The eliminated pixels represent only a very small fraction of the total number of sea ice concentration pixels, but eliminating them helps considerably in reducing the outliers on the scatter plots. These linear relations were used to generate a set of SSM/I tie points that are consistent with the original SMMR sea ice algorithm tie points (Gloersen et al. 1992). The published DMSP-F8 SSM/I tie points (Cavalieri et al. 1992) were not used. In addition to using these transformations, the DMSP-F8 SSM/I open water tie points were subjectively tuned to help minimize the differences between the SMMR and DMSP-F8 SSM/I sea ice extent and area during the overlap period. In all cases, except for the Antarctic DMSP-F8 SSM/I values, the tuned amount is within one standard error of estimate. GSFC suspects the reason for the larger tuned values results from greater weather effects during the overlap period.

For more information on the regression coefficients and revised tie points, see the NASA Technical Memorandum 104647.

DMSP-F8 and DMSP-F11 SSM/I Transition
The transition period from DMSP-F8 to -F11 includes only 16 days of good data overlap, from 3 to 18 December 1991. The DMSP-F11 SSM/I open water tie points were also tuned to help reduce differences in sea ice extent and area as was done with the DMSP-F8 SSM/I values. A further adjustment to the Antarctic 37V sea ice type-B F11 tie point was also made to reduce the sea ice area difference. In this case, the amount of tuning needed to reduce the sea ice extent and area differences between the DMSP-F8 and -F11 values is well within one standard error of estimate.

DMSP-F11 and DMSP-F13 SSM/I Transition
The effects of changing from the DMSP-F11 to the -F13 satellite were examined for a 5-month overlap period, from 5 May 1995 through 30 September 1995. Generally, in terms of hemispheric averages of mean ice concentration, the biases introduced by the transition are slight and not statistically significant; however, in some regions relatively large and significant differences are seen. In addition, differences in sea ice extent and total ice covered area between the two platforms were found to be statistically significant. For more information please see NSIDC Special Report 5: An Intercomparison of DMSP F11- and F13-derived Sea Ice Products.

Land Spillover and Residual Weather-Related Effects

The next step in preparing the data is the correction for land-to-ocean spillover (often referred to as "land contamination") and residual weather-related effects. While these steps eliminate much of the land-to-ocean spillover and weather effects over open ocean, these problems are not entirely removed. See the section Data Verification by Data Center for additional comments.

Arctic SMMR Total Ice Concentration NIMBUS-7 Day 213 08/01/83

Figure 1a. Sea ice concentration map of the Arctic for Day 213, 1983 before the application of the land spillover and residual weather corrections.
Figure 1b. After corrections.

Land-to-Ocean Spillover
Land-to-ocean spillover refers to the problem of blurring sharp contrasts in brightness temperature, such as exist between land and ocean, by the relatively coarse width of the sensor antenna pattern. This problem is of concern because it results in false sea ice signals along coastlines. (Both land and sea ice have much higher brightness temperatures than ocean.) The method used to reduce the spillover is an extension of the method employed for the single-channel Nimbus-5 Electrically Scanning Microwave Radiometer (ESMR) data in Parkinson et al. (1987). The rationale behind the approach is that a minimum observed (generally in late summer) sea ice concentration in the vicinity of coastlines where no sea ice remains offshore is probably the result of land spillover and is thus subtracted from the image. To reduce the error of subtracting sea ice in areas of actual sea ice cover, the technique searches for and requires the presence of open water in the vicinity of the image pixel to be corrected.

Land-to-ocean spillover was reduced by the following three-step procedure:

  1. A matrix M was created covering the entire grid and identifying each pixel as land, shore, near-shore, offshore, or non-coastal ocean. The identification of land pixels was straightforward, obtained from the land/sea mask. The identification of shore, near-shore, and offshore pixels was based on the scheme plotted in Figure 2b, where the pixel to be identified is labeled I,J. This pixel is considered a "shore" pixel if any pixel adjacent to it is land, a "near-shore" pixel if none of the A pixels is land but at least one of the B pixels is land, and an "offshore" pixel if none of the A or B pixels is land but at least one of the C pixels is land. All other ocean pixels are considered "non-coastal ocean". This matrix M is created once and then used throughout the data set.


  2. A matrix CMIN, to represent minimum sea ice concentrations on a pixel-by-pixel basis throughout the entire grid, was created for each instrument type. CMIN was created by first constructing a matrix P containing the minimum monthly average sea ice concentrations throughout a given year, then adjusting that matrix at offshore, near-shore, and shore pixels. In the case of SMMR, 1984 monthly data were used, whereas in the case of SSM/I, 1992 monthly data were used. In both cases, the adjustments were as follows: (a) at offshore pixels, any P values exceeding 20% were reduced to 20%; (b) at near-shore pixels, any P values exceeding 40% were reduced to 40%; and (c) at shore pixels, any P values exceeding 60% were reduced to 60%. The CMIN matrix was created once for SMMR and once for SSM/I, then used throughout the data set.


  3. The daily sea ice concentration matrices were adjusted at any offshore, near-shore, and shore pixels in the vicinity of open water. Specifically, the "neighborhood" of an offshore pixel was defined as containing the 8 other pixels in the 3 x 3 box centered on the offshore pixel; the "neighborhood" of a near-shore pixel was defined as containing the 24 other pixels in the 5 x 5 box centered on the near-shore pixel; and the "neighborhood" of a shore pixel was defined as containing the 48 other pixels in the 7 x 7 box centered on the shore pixel. At any time when the neighborhood of an offshore, near-shore, or shore pixel contains three or more open-water pixels (sea ice concentration less than 15%), then the calculated sea ice concentration at the offshore, near-shore, or shore pixel is reduced by the value for that pixel in the matrix CMIN. Wherever the subtraction leads to negative sea ice concentrations, the concentrations are set to 0%. This land-spillover correction algorithm is clearly a rough approximation, as the contaminated amount does not stay constant over time; but the scheme has been found to reduce substantially the spurious sea ice concentrations on the grids.

An alternative method for reducing the effects of land contamination on summaries of the data is to use an expanded land mask to limit the area under analysis (Maslanik et al. 1996).

Figure a.

Figure 2a. Schematic illustrating the effect of the coarse resolution of the microwave antenna on a coastline. This effect, referred to as land-to-ocean spillover, results in false sea ice signals in the vicinity of the coast.
Figure 2b. Seven-by-seven array used in the procedure to reduce the land-to-ocean spillover effect.

Residual Weather-Related Effects
A correction is made for residual weather effects that were missed by the automatic weather filters. For final data, this correction is made based on monthly climatological sea surface temperatures (SSTs) from the NOAA Ocean Atlas (Levitus and Boyer 1994). These data, originally on a two-degree by two-degree grid, were remapped onto the SSM/I grid. Because the SST data did not extend to the SSM/I coastline, the data were extrapolated to the coastline once they were mapped onto the SSM/I grid. The SST maps are used as follows:

For preliminary data, a conservative mask is applied based on the maximum monthly ice extent from 1978 through 2001.

Filling Data Gaps

There are instances of missing data. In some cases whole days (or weeks or months) are missing. In other cases, large swaths or wedges of missing data exist within an image, along with scattered pixels of missing data throughout the grid. The scattered pixels of missing data, resulting generally from mapping the orbital data to the SSM/I grid, were filled by applying a spatial linear interpolation scheme on the brightness temperature maps. The larger areas of missing data, resulting from gaps between orbital swaths (generally at low latitudes on daily maps) or from partial coverage or missing days, were filled by temporal interpolation on the sea ice concentration maps. No data at all were available for the period from 2 December 1987 through 12 January 1988. This gap was not filled by temporal linear interpolation; instead it was left as missing data.

These interpolations are applied only to final data, not preliminary data. The preliminary daily files will have scattered missing pixels and may occasionally have larger areas of missing data.

Monthly Data Generation

Once daily data have been processed as previously described, monthly data are generated. Monthly averaged sea ice concentration grids are produced from an average of the daily sea ice concentration grids available for each month. Monthly files for both hemispheres are provided for every month beginning October 1978. However, for October 1978, December 1987 and January 1988, the time series was incomplete: only three days of data were available during October 1978 to generate the monthly mean, only two days were available for December 1987, and only 19 days were available for January 1988. Therefore, the monthly means for these months do not represent the "true" monthly means.

In most cases, GSFC used all daily data to compute monthly averaged sea ice concentrations from a particular instrument until the data were no longer available. For example, SMMR data were used to compute monthly sea ice concentrations until the instrument stopped collecting data on 20 August 1987. Beginning 21 August 1987, SSM/I data were used. In 1991, DMSP-F8 SSM/I data were used through December 18; beginning December 19, DMSP-F11 SSM/I data were used

Note
It is recommended that sea ice extent and area be computed from daily maps of ice concentrations that are then used to compute monthly averages of those parameters. Computations of sea ice extents and sea ice areas should not be made from the monthly-averaged ice concentration maps because that may result in a biased time series.

5. References and Related Publications

See the following for background information pertaining to the instruments and sensor-level products used to generate this data set. Other references, particularly for sea ice characteristics and algorithm performance, are available in journals from the NSIDC library. Also, see the Selected Bibliography: SSM/I Brightness Temperatures for the Polar Regions.

Background on the Sea Ice Concentrations from Nimbus-7 SMMR and DMSP SSM/I Passive Microwave Data Set
Cavalieri et al. (1997)

Background on the SMMR and SSM/I Sensors
NSIDC Brightness Temperature User's Guide (1992), Gloersen and Barath (1977), Gloersen et al. (1992), Hollinger (1989), Hollinger and Lo (1983), Hollinger et al. (1990), Poe and Conway (1990), Svendsen et al. (1983), and Wentz (1991, 1992, 1993).

Raw Sensor Data and Brightness Temperatures
See references above, Abdalati et al. (1995), and Goodberlet (1990).

Sea Ice Physics and Characteristics
Ackley (1979), Ackley et al. (1980), Wadhams et al. (1987), Carsey (1982), Gloersen et al. (1992). Also see the algorithm references below.

Passive Microwave Algorithms for Sea Ice
Gloersen and Cavalieri (1986), Cavalieri et al. (1992), Cavalieri et al. (1984), Cavalieri (1994), Comiso (1983), Comiso (1990), Comiso et al. (1992), Comiso et al. (1984), Emery et al. (1994), Gloersen and Cavalieri (1986), Gloersen et al. (1992), Grenfell and Comiso (1986), Hollinger et al. (1984), Maslanik (1992), Massom (1991), Steffen and Schweiger (1991), Steffen et al. (1992), Svendsen et al. (1983), Swift and Cavalieri (1985), and Swift et al. (1985).

Applications of Passive Microwave-Derived Sea Ice Data
Campbell et al. (1974, 1975a, 1975b, 1976a, 1976b, 1978, 1980a, 1980b, 1981, 1984, 1987), Carsey (1982, 1985), Cavalieri et al. (1983, 1986, 1990, 1991), Cavalieri and Parkinson (1981, 1987), Cavalieri and Martin (1985), Cavalieri and Zwally (1985), Comiso (1986, 1991), Comiso et al. (1992), Comiso and Sullivan (1986), Comiso et al. (1991), Gloersen et al. (1973, 1974a, 1974b, 1975a, 1975b, 1978, 1984, 1989, 1992), Gloersen and Campbell (1988a, 1988b, 1991a, 1991b), Maslanik et al. (1996), Massom (1991), Zwally (1984), Zwally et al. (1976, 1983a, 1983b, 1985), Zwally and Gloersen (1977), and Zwally and Walsh (1987).

Other Algorithm, Format, and Processing Issues
Martino et al. (1995), NCSA (1993), Poe and Conway (1990), and Snyder (1982).

Abdalati, W., K. Steffen, C. Otto, and K. C. Jezek. 1995. Comparison of Brightness Temperatures from SSM/I instruments on the DMSP-F8 and -F11 satellites for Antarctica and the Greenland Ice Sheet. International Journal of Remote Sensing. 16(7):1223-1229.

Ackley, S. F. 1979. Mass balance aspects of Weddell Sea pack ice. Journal of Glaciology 24(90):391-406.

Ackley, S. F., A. J. Gow, K. R. Buck, and K. M. Golden. 1980. Sea ice studies in the Weddell Sea aboard USCGC Polar Sea. Antarctic Journal of U. S. 15(5):84-86.

Bonbright, D. I. 1984. PODS SSM/I Functional Requirements (Version 1.0). Jet Propulsion Laboratory Document 715-63.

Bonbright, D. I., J. W. Brown, J. E. Hilland, I. T. Hsu, J. A. Johnson, T. L. Kotlarek, R. A. Lassanyi, C. L. Miller, C. S. Morris, and F. J. Salamone. 1987. NASA ocean data system version 3.0. User handbook. Jet Propulsion Laboratory. Document 715-66, 50 pp.

Campbell, W. J. 1973. NASA remote sensing of sea ice in AIDJEX. Proceedings of the World Meteorological Organization Technical Conference, Tokyo, Japan, WMO No. 350:55-66.

Campbell, W. J., P. Gloersen, and H. J. Zwally. 1994. Short- and long-term temporal behavior of polar sea-ice covers from satellite passive-microwave observations. Geophysical Monograph 85. Editors O. M. Johannessen, R. D. Muench, and J. E. Overland. American Geophysical Union, Washington, D. C.

Campbell, W. J., P. Gloersen, and H. J. Zwally. 1984. Aspects of Arctic sea ice observable by sequential passive-microwave observations from the Nimbus-5 satellite, in Arctic Technology and Policy, I. Dyer and C. Chryslers, eds., Hemisphere Publishing, New York, 197-222.

Campbell, W. J., P. Gloersen, and R. O. Ramseier. 1975. Synoptic ice dynamics and atmospheric circulation during the Bering Sea Experiment. Proceedings of the Final Symposium on the Results of the Joint Soviet-American Expedition, K. Ya. Kondratyev, Yu. I. Rabinovich, and W. Nordberg, eds., Gidrometeoizdat, Leningrad, 196-218. (Republished as USSR/USA Bering Sea Experiment by A. A. Balkema, Rotterdam, 307 pp., 1982.)

Campbell, W. J., P. Gloersen, E. G. Josberger, O. M. Johannessen, P. S. Guest, N. Mognard, R. Shuchman, B. A. Burns, N. Lannelongue, and K. L. Davidson. 1987. Variations of mesoscale and large-scale sea ice morphology in the 1984 Marginal Ice Zone Experiment as observed by microwave remote sensing. Journal of Geophysical Research 92:6805-6824.

Campbell, W. J., P. Gloersen, W. Nordberg, and T. T. Wilheit. 1974. Dynamics and morphology of beaufort sea ice determined from satellite, aircraft, and drifting stations, in Proc. of the Symp. on Approaches to Earth Survey Problems Through Use of Space Techniques, Akademie-Verlag, Berlin, 311-327.

Campbell, W. J., P. Gloersen, R. O. Ramseier, and H. J. Zwally. 1980. Arctic sea ice variations from time-lapse microwave imagery. Boundary-Layer Meteorology 18:99-106.

Campbell, W. J., P. Gloersen, W. J. Webster, T. T. Wilheit, and R. O. Ramseier. 1976. Beaufort Sea ice zones as delineated by microwave imagery. Journal of Geophysical Research 81:1103-1110.

Campbell, W. J., R. O. Ramseier, H. J. Zwally, and P. Gloersen. 1981. Structure and variability of Bering and Okhotsk sea ice cover by satellite microwave imagery, in Energy Resources of the Pacific, M. T. Halbouty, ed., American Association of Petroleum Geologists, Tulsa, Oklahoma, 343-354.

Campbell, W. J., P. Gloersen, H. J. Zwally, R. O. Ramseier, and C. Elachi. 1980. Simultaneous passive and active microwave observations of near-shore Beaufort Sea ice. Journal of Petroleum Technology 21:1105-1112.

Campbell, W. J., R. O. Ramseier, W. F. Weeks, and P. Gloersen. 1976. An integrated approach to the remote sensing of floating ice. Proceedings of the XXVI International Astronautical Congress, Lisbon, Portugal, L. G. Napolitano, ed. 445-487.

Campbell, W. J., J. Wayenberg, J. B. Ramseyer, R. O. Ramseier, M. R. Vant, R. Weaver, A. Redmond, L. Arsenault, P. Gloersen, H. J. Zwally, T. T. Wilheit, T. C. Chang, D. Hall, L. Gray, D. C. Meeks, M. L. Bryan, F. T. Barath, C. Elachi, F. Leberl, and T. Farr. 1978. Microwave remote sensing of sea ice in the AIDJEX main experiment. Boundary-Layer Meteorology 13:309-337.

Campbell, W. J., W. F. Weeks, R. O. Ramseier, and P. Gloersen. 1975. Geophysical studies of floating ice by remote sensing. Journal of Glaciology 15:305-328.

Carsey, F. D. 1985. Summer Arctic sea ice character from satellite microwave data. Journal of Geophysical Research 90(C3):5015-5034.

Carsey, F. D. 1982. Arctic sea ice distribution at end of summer 1973-1976 from satellite microwave data. Journal of Geophysical Research 87:5809-5835.

Cavalieri, D. J. 1994. A microwave technique for mapping thin sea ice. Journal of Geophysical Research 99(C6):12,561-12,572.

Cavalieri, D. J., P. Gloersen, C. l. Parkinson, J. C. Comiso, and H. J. Zwally. 1997. Observed hemispheric asymmetry in global sea ice changes. Science 278(5340): 1104-1106.

Cavalieri, D. J. and S. Martin. 1994. The contribution of Alaskan, Siberian, and Canadian coastal polynyas to the cold halocline layer of the Arctic Ocean. Journal of Geophysical Research 99:18,343-18,362.

Cavalieri, D. J., and S. Martin. 1985. A passive-microwave study of polynyas along the Antarctic Wilkes Land coast, in Oceanology of the Antarctic Continental Shelf, S. S. Jacobs, ed., Antarctic Research Series, American Geophysical Union, Washington, D. C. vol. 43:227-252.

Cavalieri, D. J., C. l. Parkinson, P. Gloersen, J. C. Comiso, and H. J. Zwally. 1999. Deriving long-term time series of sea ice cover from satellite passive-microwave multisensor data sets. Journal of Geophysical Research 104(7): 15,803-15,814.

Cavalieri, D. J., and C. L. Parkinson. 1987. On the relationship between atmospheric circulation and the fluctuations in the sea ice extents of the Bering and Okhotsk Seas. Journal of Geophysical Research 92: 7141-7162.

Cavalieri, D. J., and C. l. Parkinson. 1981. Large-scale variations in observed Antarctic sea ice extent and associated atmospheric circulation. Monthly Weather Review 109(11):2323-2336.

Cavalieri, D. J., and H. J. Zwally. 1985. Satellite observations of sea ice. Advanced Space Research 5:247-255.

Cavalieri, D. J., B. a. Burns, and R. G. Onstott. 1990. Investigation of the effects of summer melt on the calculation of sea ice concentration using active and passive-microwave data. Journal of Geophysical Research 95:5359-5369.

Cavalieri, D. J., P. Gloersen, and W. J. Campbell. 1984. Determination of sea ice parameters with the NIMBUS-7 SMMR. Journal of Geophysical Research 89(D4):5355-5369.

Cavalieri, D. J., P. Gloersen, and T. T. Wilheit. 1986. Aircraft and satellite passive-microwave observations of the Bering Sea ice cover during MIZEX West. IEEE Transactions on Geosciences and Remote Sensing GE-24: 368-377.

Cavalieri, D. J., S. Martin, and P. Gloersen. 1983. Nimbus-7 SMMR observations of the Bering Sea ice cover during March 1979. Journal of Geophysical Research 88:2743-2754.

Cavalieri, D. J., K. M. St. Germain, and C. T. Swift. 1995. Reduction of weather effects in the calculation of sea ice concentration with the DMSP SSM/I. Journal of Glaciology. 41(139):455-464.

Cavalieri, D. J., J. Crawford, M. Drinkwater, W. J. Emery, D. T. Eppler, L. D. Farmer, M. Goodberlet, R. Jentz, A. Milman, C. Morris, R. Onstott, A. Schweiger, R. Shuchman, K. Steffen, C. T. Swift, C. Wackerman, and R. L. Weaver. 1992. NASA sea ice validation program for the DMSP SSM/I: final report. NASA Technical Memorandum 104559. National Aeronautics and Space Administration, Washington, D. C. 126 pages.

Cavalieri, D. J., J. Crawford, M. R. Drinkwater, D. Eppler, L. D. Farmer, R. R. Jentz and C. C. Wackerman. 1991. Aircraft active and passive microwave validation of sea ice concentration from the DMSP SSM/I. Journal of Geophysical Research 96(C12):21,989-22,009.

Cavalieri, D. J., C. l. Parkinson, P. Gloersen, and H. J. Zwally. 1997. Arctic and Antarctic sea ice concentrations from multichannel passive-microwave satellite data sets: October 1978 to December 1996, User's Guide. NASA Technical Memorandum 104647. 17 pages.

Comiso, J. C. 1991. Satellite remote sensing of the polar oceans. Journal of Marine Systems 2:295-434.

Comiso, J. C. 1990. Arctic multiyear ice classification and summer ice cover using passive microwave satellite data. Journal of Geophysical Research 95(C8):13411-13422.

Comiso, J. C. 1986. Characteristics of Arctic winter sea ice from satellite multispectral microwave observations. Journal of Geophysical Research 91(C1): 975-994.

Comiso, J. C. 1983. Sea ice effective microwave emissivities from satellite passive microwave and infrared observations. Journal of Geophysical Research 88(C12):7686-7704.

Comiso, J. C., and A. L. Gordon. 1987. Recurring polynyas over the Cosmonaut Sea and the Maud Rise. Journal of Geophysical Research 92:2819-2833.

Comiso, J. C., and C. W. Sullivan. 1986. Satellite microwave and in-situ observations of the Weddell Sea ice cover and its marginal ice zone. Journal of Geophysical Research 91(C8):9663-9681.

Comiso, J. C., and H. J. Zwally. 1989. Polar microwave brightness temperatures from Nimbus-7 SMMR, NASA RP-1223, 82 pages.

Comiso, J. C., and H. J. Zwally. 1984. Concentration gradients and growth/decay characteristics of the seasonal sea ice cover. Journal of Geophysical Research 89:8081-8103.

Comiso, J. C., and H. J. Zwally. 1982. Antarctic sea ice concentrations inferred from Nimbus-5 ESMR and Landsat imagery. Journal of Geophysical Research 87:5836-5844.

Comiso, J. C., S. F. Ackley, and A. l. Gordon. 1984. Antarctic sea ice microwave signatures and their correlation with in-situ ice observations. Journal of Geophysical Research 89(C1):662-672.

Comiso, J. C., T. C. Grenfell, D. Bell, M. Lange, and S. Ackley. 1989. Passive microwave in-situ observations of Weddell Sea ice. Journal of Geophysical Research 88(C12):7686-7704.

Comiso, J. C., T. C. Grenfell, M. Lange, A. Lohanick, R. Moore, and P. Wadhams. 1992. Microwave remote sensing of the Southern Ocean Ice Cover. Chapt. 12 In: Microwave remote sensing of sea ice. Frank Carsey, editor. American Geophysical Union. Washington, D. C. 243-259.

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Comiso, J. C., P. Wadhams, W. Krabill, R. Swift, J. Crawford, and W. Tucker. 1991. Top/bottom multisensor remote sensing of Arctic sea ice. Journal of Geophysical Research 96(C2):2693-2711.

Emery, W. J., C. Fowler, J. A. Maslanik. 1994. Arctic sea ice concentrations from SSM/I and AVHRR satellite data. Journal of Geophysical Research 99(C9):18,329-18,342.

Eppler, D. T., L. D. Farmer, A. W. Lohanick, M. A. Anderson, D. J. Cavalieri, J. C. Comiso, P. Gloersen, C. Garrity, T. C. Grenfell, M. Hallikainen, J. A. Maslanik, C. Matzler, R. A. Melloh, I. Rubenstein, C. T. Swift. 1992. Passive microwave signatures of sea ice. In Microwave Remote Sensing of Sea Ice, ed. F. Carsey, Geophysical Monograph 68 (AGU).

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6. Document Information

Acronyms

The following acronyms and abbreviations are used in this document:

Acronyms Used in this Document
ANSI American National Standards Institute
ASCII American Standard Code for Information Interchange
CIRES Cooperative Institute for Research in Environmental Sciences
DMSP Defense Meteorological Satellite Program
DOS Disk Operating System
ESMR Electrically Scanning Microwave Radiometer
FNMOC Fleet Numerical Meteorology and Oceanography Center
FTP File Transfer Protocol
GIF Graphical Interchange Format
GSFC Godddard Space Flight Center
IDL Interactive Data Language
NASA National Aeronautics and Space Administration
NEMS Nimbus-E Microwave Spectrometer
NOAA National Oceanic and Atmospheric Administration
NSIDC National Snow and Ice Data Center
PNG Portable Network Graphics
RSS Remote Sensing Systems, Inc.
SCAMS Scanning Microwave Spectrometer
SMMR Scanning Multichannel Microwave Radiometer
SSM/I Special Sensor Microwave/Imager
SST Sea surface temperature
URL Uniform Resource Locator

Document Creation Date

1996

Document Revision Date

April 2008
October 2006

Document URL

http://nsidc.org/data/docs/daac/nsidc0051_gsfc_seaice.gd.html