| CCAR - Colorado Center for Astrodynamics Research Satellite Oceanography : Applications : |
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Navigating the Bermuda Races
Sailboat races to Bermuda Navigational charts prepared The tactical strategies
Sailors use Jenifer Clark's product (Figure 2) to locate the warm and cold eddies, as well as the Gulf Stream. Arrows indicate the direction of flow; Sea surface temperatures are in degrees F and show warm-core and cold-core eddies that correspond to topographic highs and lows in the altimetry maps. The altimeter data are invaluable for depicting the locations of cold-core eddies, which are heavier than the surrounding water and have a tendency to sink below the surface. The thermal infrared imagery only sees the surface or skin temperature of the ocean. Because the cold-core eddies often are right below the surface, they are not detectable by their sea surface temperature signature. Also, cloud cover blocks the satellite from reading the sea surface temperature, so that the eddies are no longer visible. However, the microwave radar altimeter measurements can "see" through the clouds. Jenifer Clark uses the topography maps to identify the eddies, and their direction of rotation. In the 1986 Newport to Bermuda race, cold eddies were recorded rotating at speeds as high as 7 knots! During this race, one competitor was on the eastern side of the cold eddy. He was headed south but the intense current was pushing him backwards!
The straight line from Marion to Bermuda is the rhumb line for the race in 1999 (Figure 3). Note how well the warm and cold eddies correlate between the thermal infrared image (Figure 4) and the TOPEX topographic map (Figure 5). A warm eddy rotating clockwise near 39N 69W in the thermal infrared image shows up in the TOPEX map as a surface being 20 cm higher that the surrounding water (concentric red circles). South of the Stream in the thermal infrared image is a very large cold eddy (rotating counterclockwise) centered near 35N 67W, directly on the rhumb line. The TOPEX image depicts the cold eddy location with sea heights 30 cm below the surrounding water (concentric blue circles). Figure 4 shows Jenifer
Clark's Gulfstream analysis, derived in part from the false colored thermal
infrared imagery from NOAA polar orbiting satellites, and Figure 5 shows the TOPEX analysis of sea surface
height anomalies . The warm eddy signatures can be seen as concentric red
circles, in both images, indicating sea heights above the mean level of 10-15
cm near 39N 70W. The cold eddy located at 32N 74W shows sea heights are 20 cm
below the surrounding water while the cold eddy near 35N 70W has sea heights
depressed 10 cm below the surrounding water. The cold eddy near 36N 66W shows
that the sea heights are 30 cm below the surrounding water. Since these sea
heights are so distinct, the implication is that the current speed associated
with this eddy is more intense than the others noted.
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Copyright © 1999 Colorado Center for Astrodynamics Research, Department of Aerospace Engineering Sciences, University of Colorado at Boulder, USA. All rights reserved. | ||||||||||