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13 Dec 2024 - 22:00 UTC
GOES-East Full Disk - Derived Motion Winds
2 hour loop - 12 images - 10 minute update
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Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1000 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1100 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1200 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1300 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1400 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1500 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1600 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1700 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1800 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 1900 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 2000 UTC
Derived Motion Winds - Derived Motion Winds - 13 Dec 2024 - 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.