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6 Jun 2025 - 05:06 EDT
6 Jun 2025 - 09:06 UTC
GOES-19 Full Disk - Derived Motion Winds
12 hour loop - 12 images - 60 minute update
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Derived Motion Winds - Derived Motion Winds - 05 Jun 2025 - 2100 UTC
Derived Motion Winds - Derived Motion Winds - 05 Jun 2025 - 2200 UTC
Derived Motion Winds - Derived Motion Winds - 05 Jun 2025 - 2300 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0000 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0100 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0200 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0300 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0400 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0500 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0600 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0700 UTC
Derived Motion Winds - Derived Motion Winds - 06 Jun 2025 - 0800 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.