ESPL lecture 1

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  • Created on: 28-05-22 19:18
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  • ESPL
    • aeolian multiple choice
      • lecture 1
        • winds - and trade winds
          • winds are thermally driven by the heat budget
            • the differences of heat latitudinally create differences in heat distribution nd budget globally
              • this difference creased moving air - rising or sinking based on pressure
                • air moves from high to lower pressure through the differential creating WIND
                  • PGF – pressure gradient force – the force of moving from high to low pressure 
          • the differences of heat latitudinally create differences in heat distribution nd budget globally
            • this difference creased moving air - rising or sinking based on pressure
              • air moves from high to lower pressure through the differential creating WIND
                • PGF – pressure gradient force – the force of moving from high to low pressure 
          • cells
            • the Hadley cell drives wind through circulation - moves air in pockets globally through ascending and descending air
              • the crioulos effect determines the direction of winds
        • Large-scale airflow patterns - coriolous
          • the spinning of the earth causes wind to move in different directions in each hemisphere
            • deflect to the right in the N hemisphere and the right in the southern hemisphere
              • The spinning gives the winds a secondary direction of force and the overall direction acts as a function of the total forces acting upon it (see green arrows) 
                • Coriolis and PFG can cancel each other out leading to a deviation and horizontal movement
          • Wind has momentum the mass if the wind X the velocity Part of the momentum is based on the spinning of the earth à this is greatest near the equator – see circular motion – furthest from the axis of rotation
            • At its widest part it is rotating fastest – higher rotational force Momentum in conserved 
              • Rotational speed becomes less of a contribution their relational speed is higher compared to the speed of rotation Higher speeds of wind at higher latitudes
              • WIND and MOMENTUM
                • Wind has momentum the mass if the wind X the velocity Part of the momentum is based on the spinning of the earth à this is greatest near the equator – see circular motion – furthest from the axis of rotation
                  • At its widest part it is rotating fastest – higher rotational force Momentum in conserved 
                    • Rotational speed becomes less of a contribution their relational speed is higher compared to the speed of rotation Higher speeds of wind at higher latitudes
                    • WIND and MOMENTUM
                      • wind has momentum =mass X velocity
                        • mass based on qualities of the atmosphere
                • wind has momentum =mass X velocity
                  • mass based on qualities of the atmosphere
        • large scale airflow patterns-continentality
          • the global circulation is affected by the distribution of land and ocean
            • this also impacts wind speed
              • local topography like mountains can impact wind speeds
            • smoothness and roughness also impacts wind speeds - smoother surfaces = faster wind
              • Westerlies in N hemisphere a weather systems from other latitudes impact winds in their surroundings 
                • eddies and turbulent flows disrupt air - low pressure system (30-60 degrees N/S)
        • global distribution of windspeeds
          • higher over the seas = lmore smooth
            • slower over land - westerlies are quicker than trade winds - 60 degrees N/S
        • BOUNDARY LAYER INTERFERENCE
          • biggest interference with the surface
            • air region above the surface where airflow is influenced by ground’s friction Dependent on the roughness of the surface
              • full atmospheric boundary layer - 1-2km
                • near ground boundary layer - 10cm
              • velocity profile - change in speed with height
                • velocity profile determined by air flow type
                  • laminar flow - air moves in layers and do not mix - not common in natural flow
                    • turbulent flow - more common eddies in flow mix and deforms the air
                      • irregular gusts with fastest air moving at bottom due ot the compression of air
                    • requires negligible friction constant velocity at a height
          • Profile measurements with height – velocity profile Profile shape (plot) will allow the winds behaviour to be quantified and the movement caused by the wind to be assessed and predicted. 
            • Relationship between surface profile and air flow.
            • Velocity profile Closest to ground = more friction = slower winds Turbulent mixing is effective at moving velocity away from the surface Most exchange happens near the surface 
              • Turbulent mixing, creates a rapid increase of u near bed
              • If height (z) plotted on log scale … over flat, un-vegetated ground, without strong heating… the velocity profile will plot as a straight line (semi-log plot)
                • the law of the wall
                  • Height in LOG Intercepts on y axis  the law of the wall – 1.Uses a log fit, velocity profile bever reaches surface (y axis intercept) by assuming a log fit 
                    • 2.Assumes that above the surface what exists in reality is a )ms-1 dead air zone with no wind speed because of friction
                  • Z0 – aerodynamic roughness length – property of air flow Measure  - take height/30 Rougher surfaces = increased Z0 Protection form erosion by rougher surfaces 
                    • Surfaces should always have the same Z0 at any different wind speed
                  • profile where LoW holds
                    • u/u_? =1/k Ln z/z_0
                      • u = velocity (at height z) z0 = aerodynamic roughness length k = von Karman’s constant (~0.4) u* = shear velocity
                        • LofW allows key parameters (z0 & u*) to be derived from u & z
      • lecture 1
        • Shear velocity is proportional to gradient of velocity profile 
        • •Drag of airflow over ground exerts shear stress at surface (?0)  
          • •This stress represents ability of wind to move sediment   …BUT we cannot directly measure ?0
            • •Instead, we can calculate shear velocity (u*), which is proportional to the slope (y/x) of the velocity profile
              • Law of the wall
                • Faster wind speed = greater shear stress Ability to entrain particles - erosivity power and potential to move matter = erosivity
                  • •So, u* is proportional to the slope (y/x) of the profile •i.e. faster wind at z results in a steeper profile gradient, therefore greater drag and greater u*
                • Remember… •Assumes windspeed is zero just above surface •Applies only when velocity profile is log straight •Law of the Wall does not hold:
                  • -Airflow is topographically-altered (e.g. accelerated) X -In non-neutral atmospheric conditions X -Vegetated surfaces X (Needs adjustment…)
                • Vegetated surfaces  - on average may give a Z0 at a greater height 
      • sediment types
        • percentages of rocks           20% carbonates       15% sandstone        60% clay minerals and quatrz
          • quarts dominates aeolian deposits because it is heavy and chemically stable
            • Abundant (60%), highly resistant When in transport it isn’t broken down physically or chemically – accumulates 
              • Chemically stable – requires highly alkaline solutions to dissolve  - pHs not found naturally
        • sediment sizes
          • •Sand = 63 to 2000 mm diameter particles
            • •Silt + clay  < 63 mm diameter (often referred to as ‘dust’ in aeolian processes)
      • particle entrainment
        • lift and drag promote entrainment
        • gravity (particle size, mass) prevent 
        • Cohesion – attraction – electrostatic forces, interparticle forces, friction, Small pressure systems within the grain 
          • system Pressure tries to move the particle up into the velocity gradient  - pressure difference
            • If enough shear velocity is applied, it will be entrained This is the CSV U*c Threshold to entrainment 
              • For winds to help the landscape the CSV needs to be understood Function of… particle size, Gravity, Atmospheric density, Moisture, 
                • Not a factor of the wind but sediment and environment If the shear velocity is enough to cause entrainment 
                  • Wind represent erosivity – ability to erode Surface represents erodibility – ability to be eroded
                    • u*c  is the u*  at which aeolian transport occurs   = threshold of entrainment
                      • u*c = f(particle size, gravity, atmospheric density) u*c is related to the sediment & environment
        • bagnolds equation
          • Relates to sediment and the environment Denser sediment = more shear velocity to move Air density – usually a constant g – gravity D – greater diameter = bigger grains are harder to move
            • A - coefficient of flow (value depends on if fluid or impact threshold is relevant) Usually has 1 of 2 values – Fluid  - just air flow increasing in velocity  - energy transfer à the impact of other sand grains = impact threshold  - lower than fluid
        • creep
          • •Rolling of large (>500 mm) grains along surface/bed
            • •Bagnold (1941) 20-25% sand moves by creep (up to 40%)
              • saltation
                • Most dynamic process Moves a wide range of particle sizes Biggest size fraction of sand (70-500mm)
                  • Incoming particles hit the surface with a shallow rebound (6-16°) and then a steeper rebound (50-90°) from the bed Asymmetric movement 
                  • Ration H x12-15 = hop distance 
                  • Some energy lost to the bed 50-60% retained 10% lost into the dislodged particles 
                    • reptation - splash
                      • Most relocating grain occur down wind Some do go back into the flow This breaks cohesion  - breaking bonds freeing them for other forms of transportsed

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