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currents II

-water interaction and drag , circular and geostrophic flow  General ocean flow pattern Wind-Water surface interaction Water motion at the surface of the ocean () is driven by wind effects. Friction causes drag effects on the water, transferring from the atmospheric to the ocean surface water. The drag Wind generates vertical and horizontal motion in the water, triggering convective motion, causing turbulent mixing down to about 100m depth, which defines the isothermal mixed layer. The drag force FD on the water depends on wind velocity v: 2 FD  CD  Aa v CD  drag coefficient dimensionless factor

for wind water interaction CD  0.002, A  cross sectional area depending on surface roughness, and particularly the emergence of waves! Katsushika Hokusai: The Great Wave off Kanagawa The Beaufort Scale is an empirical measure describing wind speed based on the observed conditions (1 knot = 0.514 m/s = 1.85 km/h)! For land and city people

Bft 6 Bft 7 Bft 8

Bft 9 Bft 10 Bft 11 Bft 12 m Conversion from scale to wind velocity: v  0.836 B3/ 2 s A strong breeze of B=6 corresponds to wind speed of v=39 to 49 km/h at which long waves begin to form and white foam crests become frequent. The drag force can be calculated to:

kg km m F  C  A v2  1200 v  45 12.5  C  0.001 D D a a m3 h s D 2 kg 2  m  2 FD  0.0011200  Am 12.5  187.5 A N or FD A   187.5 N m m3  s 

For a strong gale (B=12), v=35 m/s, the drag on the water will be:

2 kg  m  2 FD / A    0.00251200 35   3675 N m m3  s  kg m  1200 v  35  C  0.0025 a m3 s D Ekman transport

The frictional drag force of wind with velocity v or x generating a water velocity u, is balanced by the force, but drag decreases with depth z. m   F A  C  v2   F A  2m Au sin   f u  D D D a c c A m 2sin   f s1  Coriolis parameter  z A

F / A z  z z  1    f u   D m / A z z  z 1 τ force N in vector terms f zˆ u   D   z kg zˆ u defines vector direction of transport τ  f zˆ u  D z 0 D   f zˆ u dz  f zˆ MEk  0  kg  MEk  u dz   Ekman mass transport vector  m s  the force vector the Since M assumption M   f D D

Ek Ek magnitude    water

z z  the 2

    D z   

,  is 

 the horizontal 0

 f f 

perpendicular u   sin   is 1 

is direction z 

u  is M perpendicular 

u  a : Ekman

dz 

Ek moreless z

wind  sin   

of m

kg 90

to

direction  the s

0

both linear   

to frictional

f transport

vectors  the

M

u, increase

Ek

moving depth

drag and

of water depth vector

density wi th

depth Example for Ekman transport

What drag force (pressure) does it take at a latitude of 35oN to move water over a depth of 10 m within 1 minute by 100 m to the right?

0 5 1 D z  f  M Ek f  2sin 35   7.29210 s f  27.292105 s1 sin 350  4.183105 s1 kg 100m kg M  u  z 1200  10m  20,000 Ek m3 60s m s kg kg N  z  f  M  4.183105 s1 20,000  0.837 1 D Ek m s m s2 m2

kg 1  2 m km Weak force, done by v  D  m s  0.913  3.3 C kg s h winds of B≈2 with : D 1200 0.001 m3

Typical surface wind stress conditions

Annual mean wind stress  on the ocean in units (N/m2). The green shade represents the magnitude of the stress. Typical wind stress values in the Westerlies reach  ≈ 0.1 to 0.2 N/m2. The strongest stress component can be observed for the Roaring Forties, the weakest component is in the Doldrums.  z C   v2  z  f  M M  D  D a D Ek Ek f 2sin

2 Calculate the mass transport MEk for a typical wind stress of D = 0.25 N/m o at the southern latitude of 40 S. f  2sin 400    7.292105 s1 f  27.292105 s1 sin 400  9.37105 s1 N 0.25  2 kg M  D  m  2.67103 Ek f  9.37105 s1 m s

About 2 tons of water are shifted within 1 sec by 1 meter to the left!

Determine the wind velocity for a typical drag coefficient CD=0.002? kg 9.37105 s1 2.13103 f  M f  M m km v2  Ek v  Ek  m s  0.29 1 C  C  kg s h D a D a 0.0021200 m3 About B=1-2 on the Beauford Scale Impact on ocean currents The direction of Ekman transport depends on the hemisphere. In the this transport is at a 90o angle to the right of the wind direction, and in the it occurs at a 90o angle to the left of the wind direction. This generates gyres, circular motions in ocean basins limited by continental coasts. Reality Realityis more iscomplex more complex because becauseof additional of additional forces due forces to friction due toand the drag temperatureforces effects, provided which by the add atmospheric to the windformation circulation phenomenon! and by the friction forces exerted by deeper water layers! The cold Peruvian current (an eastern ) flows towards the along the coast of Ecuador and Peru. It flows with a speed of 0.1 to 0.15[m/s]. In the absence of an El Niño, prevailing surface winds cause Ekman transport to the left or away from the coast, with subsequent of cold water.

Kon Tiki, Heyerdahl’s thesis of populating Polynesia from the East rather than from the North-West by taking advantage of Humboldt current for sea travel.

Pressure conditions towards ocean depth can be expressed in terms of the salinity and temperature dependence of ocean water density dP  g   dz P  g     S,T, P z ref neglecting  S,T, P P z  P  g    z    surface ref   Approximately a linear increase of surface z  pressure with depth – in contrast the P  1atm  105 Pa displays an exponential surface decrease of pressure with altitude . m kg z  100m P100m  105 Pa  9.81 1000 100m  106 Pa s2 m3 z  1km P1km  107 Pa Flow at larger depth is directed z  4km P4km  4107 Pa by the pressure gradient and the , “geostrophic flow”. Geostrophic flow

A is an oceanic flow in which the pressure gradient force is balanced by the Coriolis effect. The direction of geostrophic flow is parallel to the isobars, with the high pressure to the right of the flow in the Northern Hemisphere, and the high pressure to the left in the Southern Hemisphere.

Fluid or gaseous media move from high pressure to low pressure regions. The force pushing the water is called the pressure gradient force Fp. In a geostrophic flow, water moves along the lines of equal pressure (isobars), instead of moving from a high pressure to low pressure region. This occurs due to ’s rotation that cause the Coriolis force Fc. The Coriolis force acts at right angles to the flow. When it balances the pressure gradient force (Fp=Fc), the resulting flow becomes the geostrophic flow. Flow velocity Variations of pressure conditions or isobars with depth are associated with temperature and salinity conditions and can cause horizontal flow. The pressure gradient is balanced by the Coriolis force. This allows an estimate of the flow speed.

1 F  F  f  zˆ  u  P  0 c p  yielding a flow velocity 1 u  zˆ  P f   g z   The pressure gradient is also affected along usurface   coastlines with upwards sloping ground level. f  ref L

With f being the Coriolis parameter and g the earth acceleration. L represents the distance over which the salinity and temperature dependent density anomaly  changes. Between 20oN and 40oN, L≈2000km. Geostrophic ocean flow

Consider the as a sample. The is a pressure or density with depth that in combination with the previously discussed Coriolis force affects the direction and determines the surface flow velocity g z   usurface   f  ref L

With f being the Coriolis parameter and g the earth acceleration. L represents the distance over which the salinity and temperature dependent density anomaly  changes. Between 20oN and 40oN, L≈2000km. Estimate the gulf stream surface velocity usurface assuming a distance between 20oN and 40oN of L=2000 km for a depth of z=1000 m! g z   kg kg kg usurface     26 3  22 3  4 3 f  ref L m m m f  2  sin300    7.292 105 s1 f  7.292 105 s1 m kg 9.81 1000 4.0 2 3 m u  s  m  3101 surface kg 7.292 105 s1 1000 2,000,000m s m3 Overall agreement within the range of local speed variations. The maximum speed is observed at the western boundaries of the Gulf stream with v ≈ 1m/s, while in the interior of the gyre, the speed is much lower, v≈10cm/s. Gulf stream flow velocity simulation for different temperature zones

NASA/Goddard Space Flight Center Scientific Visualization Studio Single water drop flow

The flow pattern is complex and the flow velocity varies greatly. Both observables are defined by coastal boundaries, drag forces at the surface, density gradients at deep depths, and the Coriolis force. Geostrophic flow induced variations in ocean surface height The curvature of the flow and the horizontal velocity gradient across the flow causes a pressure gradient perpendicular to the flow direction, which translate into variations of the ocean surface height . m 104 s1 1106 m 0.1 f  L u    ;   s 1m 106 g m L 9.81 2 s m for : u  0.1 f 104 s1;L  1000km Ocean Surface Height s Example Gulf of Mexico Flow pattern Water height

Altitude anomalies http://www.aoml.noaa.gov/phod/dhos/altimetry.php Maps of obtained from satellite altimetry measurements are used to derive surface ocean currents. Higher values of sea level (oranges and reds) are associated with gyres and warm eddies, while lower values are associated to colder features. Drifter trajectories illustrate circulation features. Sea height anomaly maps show the difference of sea level from average conditions, while sea height maps show absolute values of the sea level. Changing average sea altitude levels

Sea level trend between 1992 and 2009 with respect to a reference level , based on satellite altitude measurements. Yellow and red regions show rising sea level, Basedwhile on green observational and blue data regions such showas falling level measurements sea level. and satellite based altimetry