Notice:
This site has successfully transitioned the image data source from GOES-16 to
GOES-19. There are some remaining anomalies in the production of mesoscale
geocolor images which are being investigated. Everything else should be operating
as expected. Please contact:
NESDIS.STAR.webmaster@noaa.gov if you have any questions.
20 May 2025 - 18:02 EDT
20 May 2025 - 22:02 UTC
GOES-West Full Disk - Derived Motion Winds
12 hour loop - 12 images - 60 minute update
To enlarge, pause animation & click the image. Hover over popups to zoom. Use slider to navigate.
While GOES animation code will not run on older Internet Explorer browsers,
they work in the newest versions of Microsoft Edge. If you are using
Internet Explorer, please try a different browser: Chrome, Firefox, Safari, or
MS Edge are all supported.
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1000 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1100 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1200 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1300 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1400 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1500 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1600 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1700 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1800 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 1900 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 2000 UTC
Derived Motion Winds - Derived Motion Winds - 20 May 2025 - 2100 UTC
Derived Motion Winds key:
Red barbs: High level winds: 100 - 400mb, altitude approximately 23,000 - 46,000 ft. (7-14 km)
Cyan barbs: Mid-level winds: 400 - 700mb, altitude: approximately 10,000 - 23,000 ft. (3 - 7 km)
Yellow barbs: Low-level winds: > 700mb, altitude: approximately < 10,000 ft. (< 3 km)
Derived Motion Wind Vectors (DMW) are produced using sequential ABI images and as such they can provide important information about winds at different levels during asynoptic times. Areas of wind shear or jet maxima can be identified. Wind Vectors are computed using both visible and infrared (including water vapor) imagery. DMWs are used to identify regions of strong winds or wind shear to confirm model forecasts and/or to anticipate the result of strong winds or shear.