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12 Nov 2025 - 15:34 EST
12 Nov 2025 - 20:34 UTC
GOES-19 CONUS - Derived Motion Winds
3 hour loop - 12 images - 15 minute update
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Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1701 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1716 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1731 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1746 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1801 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1816 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1831 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1846 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1901 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1916 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1931 UTC
Derived Motion Winds - Derived Motion Winds - 12 Nov 2025 - 1946 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.