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CEPD03 Coastal Sediment Transport 3

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Coastal Sediment Transport CEPD03 Lecture 3 Prof. Dano Roelvink Dr. Jan van de Graaff
Transcript

7/26/2019 CEPD03 Coastal Sediment Transport 3

http://slidepdf.com/reader/full/cepd03-coastal-sediment-transport-3 1/42

Coastal Sediment Transport

CEPD03

Lecture 3

Prof. Dano Roelvink

Dr. Jan van de Graaff

7/26/2019 CEPD03 Coastal Sediment Transport 3

http://slidepdf.com/reader/full/cepd03-coastal-sediment-transport-3 2/42

Contents

• Overview of problems

• Bed shear stress by waves and current

• Sediment transport by waves and current

• Longshore sediment transport• Cross-shore sediment transport

• Coastline changes

• Dune erosion• Sedimentation in channels and trenches

• Stability of channels and inlets

7/26/2019 CEPD03 Coastal Sediment Transport 3

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Exercise about lectures 1 and 2

• V=0.7 m/s

• H=1 m

• h=2 m• T=7 s

• D50=0.2 mm; D90=0.3 mm

• r=0.05 m• Compute

0, , , , , ,c w w cw b su f S S    

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Longshore transport

• Simple method to estimate longshore

velocity

• Use estimated wave height in surf zone

• Derive radiation stress gradient from this

• Balance radiation stress gradient with

bottom shear stress

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Radiation stress

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Longshore wave forces

 

cos sin

sincos

sin

cos

sincos

 xy g 

 y

 g 

 g 

 g 

S C  F E  x x C 

 EC  x C 

 EC   x   C 

 EC 

C x

 

  

 

 

  

   

     

 

         

7/26/2019 CEPD03 Coastal Sediment Transport 3

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Longshore wave forces

 

 

sincos

sincos

sin( )

 y g 

 g 

w y

 F EC  x C 

 EC C x

 D F 

  

  

 

   

 

=0

(Snel’s

Law)

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 Assignment

• Hs0=3m, T=8s,

•  Angle of incidence:

• 75,60,50,45,40,30,20,10 deg.• Compute conditions at breaker line

• Compute longshore sediment transport

using coefficient B=0.04

0.7  

7/26/2019 CEPD03 Coastal Sediment Transport 3

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Contents

• Wave energy balance

• Dispersion relation

• Wave celerity and group velocity

• Snel’s Law • Shoaling and refraction

• Wave breaking

• Dissipation

• Solving 1D energy balance

• Radiation stresses and wave forces

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Wave energy balance

   

2 2 2

cos   sin

1   1

2 8

 g    g 

rms

 E  EC    EC D

t    x y

 E g ga gH 

     

   

       

Wave energy Group

velocity

Wave angle Wave

dissipation

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Dispersion relation

• Relation between wave period T and wave

length L for given water depth

2

tanh( )2

2

1

2 sinh(2 ) g 

 gk kh

 Lk    C  L   T k 

d khC nC C  

dk kh

  

 

     

 

 

   

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Deep water

22

tanh( ) 1 sinh( )

2

2

2

1

2 g 

kh kh

 gk k  g 

 L g    gT 

k    C  L   T k 

d C nC C  

dk 

  

  

     

 

 

   

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Shallow water

2

tanh( ) sinh( )

( ) /

2

2

1

2 sinh(2 ) g 

kh kh kh kh

 gk kh k gh

 Lk    C g h

 L   T k d kh

C nC C ghdk kh

 

  

     

 

 

   

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Wave refraction

05102030

Depth

contours

Wave rays

Wave crests

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Snel’s Law 

• Valid for straight contour lines

• Relates local wave angle to deep water

wave angle

0

0

sin   sin

c c

 

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Wave breaking

• Complex process

• Various approximations, e.g.

 – Battjes and Janssen, 1978

 – Thornton and Guza, 1983

 – Roelvink, 1993

 – Baldock, 1998

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Baldock model

2

max

2 2

max

1

4ms

 H 

 H 

w p rms D g f e H H  

max

0.88tanh( )

0.88

kh H 

 

Coefficient

~1

Coefficient

~0.6-0.8

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1D Wave energy balance

    cos   sin g    g    w

 E  EC 

t    y EC    D

 x  

   

Wave energy Group

velocity

Wave angle Wave

dissipation

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Solving 1D wave energy balance

• Outside surf zone:

 – Wave energy flux is constant

 – Group velocity follows from dispersion relation

 – Wave angle follows from Snel’s Law 

 

0 0 0

cos 0

cos cos

 g 

 g g 

 E C 

 x EC E C 

 

 

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Shoaling and refraction

• Shoaling is change in wave height due to

change in group velocity

• Mostly increasing towards shore

• Refraction is bending of wave rays

towards shore, leads to decrease of wave

height because energy is spread over

wider area

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Wave refraction

05102030

Depth

contours

Wave rays

Wave crests

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Solving 1D wave energy balance

• Inside surf zone:

 – Group velocity follows from dispersion relation

 – Wave angle follows from Snel’s Law 

 – Dissipation follows from e.g. Baldock, relating wavedissipation to wave energy and water depth

 – Solve E  numerically, starting from known value

outside breaker zone

cos ( , ) g w EC D E h x

 

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Solving 1D wave energy balance

• Very simple numerical scheme:

 

1   , 1 1 ,

,

1

, 1 1

cos cos( , )

cos   ( , )

cos

i g   i i i g i   i

w i i

i g i i w   i i

i

 g i i

 E C E C 

 D E h x

 E C D   E h x

 E  C 

 

 

 

 

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Radiation stresses

 xxS 

 xxS 

 yxS   yxS 

 yyS 

 yyS 

 xyS 

 xyS 

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Wave forces

 xy xx x

 xy yy

 y

S S  F  x y

S S  F  x y

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Radiation stresses

2

2

1cos

2

cos sin

1sin

2

 xx

 xy yx

 yy

 g 

S n n E  

S S n E  

S    n n E 

C n

 

 

 

       

   

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Wave forces

• Follow from radiation stress gradients

• Radiation stresses are function of wave

energy, wave direction and ratio wave

celerity to group velocity

• In 1D case we can compute all these

easily


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