Microwave brightness over the poles (DMSP, daily)
What it measures. Provides daily maps over the polar regions of natural microwave energy from the surface, expressed as brightness temperature (how warm the surface looks to the sensor) across several frequencies and polarizations.
How it's made. Built from the SSM/I and SSMIS passive microwave sensors on a series of DMSP satellites, gridded daily into a polar map (12.5-25 km) using a simple averaging method, with a record stretching back to 1987.
How & where you'd use it. A building-block input used to track sea ice, snow cover, and surface conditions over the poles, and to study long-term polar climate change.
What's measured
Coverage & cadence
- Time span1987-07-09 → ongoing
- Measured byDMSP 5D-2/F11 (SSM/I) · DMSP 5D-2/F13 (SSM/I) · DMSP 5D-2/F8 (SSM/I) · DMSP 5D-3/F17 (SSMIS) · DMSP 5D-3/F18 (SSMIS)
- Processing levelLevel 3
- Spatial extent-180, 30, 180, 90
- FormatsnetCDF-4
- StatusACTIVE
What you can do with it
- Track deforestation, fire scars and land-cover change
- Monitor crop and vegetation health (NDVI/EVI)
- Map how built-up vs. green an area is over time
Official description
This data set provides daily gridded brightness temperatures derived from passive microwave sensors and distributed in a polar stereographic projection. NSIDC produces daily gridded brightness temperatures from orbital swath data generated by the Special Sensor Microwave/Imager (SSM/I) aboard the Defense Meteorological Satellite Program (DMSP) F8, F11, and F13 platforms and the Special Sensor Microwave Imager/Sounder (SSMIS) aboard DMSP F17 and F18. The SSM/I and SSMIS channels used to calculate brightness temperatures include 19.3 GHz vertical and horizontal, 22.2 GHz vertical, 37.0 GHz vertical and horizontal, 85.5 GHz vertical and horizontal (on SSM/I), and 91.7 GHz vertical and horizontal (on SSMIS). Data at 85.5 GHz and 91.7 GHz are gridded at a resolution of 12.5 km, with all other frequencies at a resolution of 25 km. Orbital data for each 24-hour period are mapped to respective grid cells using a simple sum-and-average method, also known as the drop-in-the-bucket method. Data coverage began on 09 July 1987 and is ongoing through the most current processing, with updated data processed several times annually.
Get the data
import earthaccess
earthaccess.login(strategy="netrc") # free Earthdata Login
results = earthaccess.search_data(
short_name="NSIDC-0001",
version="6",
bounding_box=(-122.5, 37.2, -121.8, 37.9), # your area (W,S,E,N)
temporal=("2024-01-01", "2024-12-31"), # your dates
)
files = earthaccess.open(results) # stream straight from NSIDC_CPRD Browsing CMR needs no login. Downloading or streaming bytes needs a free Earthdata Login + the earthaccess package. Official links
- Search and order NASA Earth Science data using spatial and temporal filters. Reformatting, reprojecting, and subsetting options are available for some data sets. GET DATA
- Quickly download a few files using a web browser, or access data through a command-line utility such as WGET. GET DATA
- Search data by spatial and/or temporal ranges or file name. Choose from various download options, including a Python script. GET DATA
- A Python library to search and access NASA Earth science data with just a few lines of code GET DATA
- Find more data access options and help resources. VIEW RELATED INFORMATION
- DMSP SSM/I-SSMIS Daily Polar Gridded Brightness Temperatures, Version 6 User Guide VIEW RELATED INFORMATION
- Special Report 07: Impact of Various Processing Options on SSM/I-derived Brightness Temperatures VIEW RELATED INFORMATION
- Special Report 05: An Intercomparison of DMSP F11- and F13-derived Sea Ice Products VIEW RELATED INFORMATION