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Ocean surface temperature (SST) can range from 28F near the North and South poles to more than 86F in the tropics. SST measurements provide details on ocean processes and dynamics, and can indicate the location of ocean features including fronts and eddies as well as highlight coastal upwelling and exchanges between the coastal shelf and open ocean. 

SST can directly affect weather systems. For example, warm ocean waters can spawn and intensify tropical storms, hurricanes, and typhoons. Similarly, SST influences climate patterns, such as through the development of warmer water El Niño and cool-water La Niña seasonal weather events that strongly correlate with temperatures and precipitation amounts during North American winters.

SST also is a factor in how healthy ocean environments are for animal and plant life. If temperatures are too warm, they can spawn toxic algal blooms or lead to fish kills and coral bleaching events.

How is Ocean Temperature Measured?

SST can be measured by satellite instrument observations, buoys, ocean gliders, drifters, mooring, ships or from the shoreline. Depending on the method, temperature measurements range in depth from 10 microns up to approximately 15 feet.

NASA’s data archives house current and historical measurements from virtually all of these methods, many in analysis-ready formats and available in the cloud.

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Access a range of datasets and data tools to further your sea surface temperature research.

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GHRSST Sea Surface Temperature showing the Gulf Stream of the Atlantic Ocean on 29 May 2024
This image shows the Gulf Stream as a ribbon of dark red hugging the East coast of the United States before heading toward the North Atlantic Current and Europe. The base true-color corrected reflectance image was acquired by the Visible Infrared Imaging Radiometer Suite (VIIRS) aboard the joint NASA/NOAA NOAA-20 satellite. Overlaid on the base image is Sea Surface Temperature from the Group for High Resolution Sea Surface Temperature (GHRSST). The Multiscale Ultrahigh Resolution (MUR) L4 analysis is based upon nighttime GHRSST L2P skin and subskin SST observations from several instruments, including the NASA Advanced Microwave Scanning Radiometer-EOS (AMSR-E), the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA's Aqua and Terra platforms, the U.S. Navy microwave WindSat radiometer, and in-situ SST observations from the NOAA iQuam project.

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