heat flow-2

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Ali Oncel [email protected] .sa Department of Earth Sciences KFUPM Heat Flow Solid Earth Geophysics Parks and Plates ©2005 Robert J . L illie N A TIO NAL PARK LANDS N A TIO NAL PARK LANDS Over H otspot - Highly E levated Off of Hotspot - L ower F arther from Hotspot and E roded - E ven L ower

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Page 1: Heat Flow-2

Ali [email protected]

Department of Earth SciencesKFUPM

Heat Flow

Solid Earth Geophysics Parks and Plates

©2005 Robert J. LillieNATIONAL PARKLANDSNATIONAL PARKLANDS

Over Hotspot -Highly

Elevated

Off of Hotspot -

Lower

Farther from Hotspot and Eroded

- Even Lower

Page 2: Heat Flow-2

What could you say about the qualitative behavior of the Heat

Conduction equation after so many things?

1D Heat Conduction Equation

pp c

AT

c

k

t

T

2

3D Heat Conduction Equation

p

c

pp c

A

z

T

c

k

t

T

2

2

Specific heat

Specific heat is defined as the amount of heat required to raise 1 kg of material by 1C. Thus, Wkg-1 oC-1 is the unit for specific heat.

Page 3: Heat Flow-2

Calculation of Simple Geotherms –Equilibrium Geotherms

pp. 279 of Fowler, 2005

Page 4: Heat Flow-2

Equilibrium Geotherms

• The temperature vs. depth profile in the Earth is called the geotherm.

• An equilibrium geotherm is a steady state geotherm.• Therefore:

2

20,

T T Aand

t z k

pp. 275 of Fowler, 2005

time

rate A per unit volume per unit time

Thermal Conductivity

Page 5: Heat Flow-2

Boundary conditions

• Since equation above is a second order differential equation, we should expect to need 2 boundary conditions (bc) to obtain a solution.

• A possible pair of bc’s is:– Temparature T=0 on z=0

– Surface heat flow Q= =-Q0 on z=0

– Then

pp. 277 of Fowler, 2005

2

20,

T T Aand

t z k

zT

kzQ

)(

kQzT

/0

Page 6: Heat Flow-2

Solution

• Integrate the differential equation once:

• Use the second bc to constrain c1

• Substitute for c1:

1

T Azc

z k

01

Qc

k

0QT Az

z k k

pp. 277 of Fowler, 2005

Page 7: Heat Flow-2

Solution

• Integrate the differential equation again:

• Use the first bc to constrain c2 which is the constant of integration.

• Substitute for c2:

• Note: Q0 will usually be a negative number in z-positive-downward frame.

20

22

Q zAzT c

k k

2 0c

20

2

Q zAzT

k k

pp. 278 of Fowler, 2005

Page 8: Heat Flow-2

Oceanic Heat FlowHeat flow is higher over and more scattered over young oceanic crust, which is formed by intrusion of basaltic magma from below.

The heat drives water convection due to very permeable of the fresh basalt despite the fact that ocean crust is gradually covered by impermeable sediment and water convection ceases.

Ocean crust ages as it moves away from the spreading center. It cools and it contracts.

pp. 289 Fowler, 2005

Page 9: Heat Flow-2

d = 5.65 – 2.47e-t/36

d (km) = bathymetric depth

t (Ma) = Lithosphere age

Q=Heat Flow

pp. 289-290 Fowler, 2005

These data have been empirically modeled in two ways:

d = 2.6 + 0.365t1/2For ages <20 my:

For ages >20 my:

For ages >55 my:For ages <55my: Q = 510 t-

1/2

Q = 48+ 96e-t/36

Page 10: Heat Flow-2

Oceanic Heat Flow, Mean Depth,t1/2, t-1/2 Age Law

For ages <70 my:

For ages <120 my:

See for detail on Table 7.5, pp. 296, Fowler, 2005

Page 11: Heat Flow-2

Half Space Model: Specified temperature at top boundary. No bottom boundary condition. Cooling and subsidence are predicted to follow square root of time as discussed by:

Plate Model: Specified temperature at top and bottom boundaries. Cooling and subsidence are predicted to follow an exponential function of time. Roughly matches Half Space Model for first 70 my.

pp. 294 Fowler, 2005

Lith

osph

ere

Page 12: Heat Flow-2

pp. 298 Fowler, 2005

Plate Motion

The base of the mechanical boundary layer is the isotherm chosen to represent the transition between rigid and viscous behavior. The base of the thermal boundary layer is another isotherm, chosen to represent correctly the temperature gradient immediately beneath the base of the rigid plate. In the upper mantle beneath these boundary layers, the temperature gradient is approximately adiabatic. At about 60-70 Ma, the thermal boundary layer becomes unstable, and small-scale convection starts to occur. With a mantle heat flow of about 38x10-3 Wm-2 the equilibrium thickness of the mechanical boundary layer is approximately 90 km.

Thermal Structure of oceanic lithospheri

c plate.

Page 13: Heat Flow-2

Radioactive Heat Generation

Radioactive elements:

Uranium (238U, 235U), Thorium (232Th)

and Potassium (40K)

Page 14: Heat Flow-2

Continental Heat Flow

Heat flow versus crustal age for the continents. The heights of the boxes indicate the standard deviation about the mean heat flow, and the widths indicate the age ranges (After Sclater et al., 1980)

pp. 299 Fowler, 2005

Page 15: Heat Flow-2

Heat Flow Provinces from Eastern USA

pp. 299 Fowler, 2005

Internal heat generation

Measured Heat Flow

Page 16: Heat Flow-2
Page 17: Heat Flow-2

The model of plate cooling with age generally works for continental lithosphere, but is not very useful.

Variations in heat flow in continents is controlled largely by changes in the distribution of heat generating elements and recent tectonic activity.

Continental

Heat Flow

pp. 302 Fowler, 2005

Page 18: Heat Flow-2

Range of Continental and Oceanic Geotherms in the crust and upper

mantle

pp. 303 Fowler, 2005

Page 19: Heat Flow-2

Oceanic Lithosphere

Thermal models of the lithospheric plates beneath oceans and continents. The dashed line is the plate thickness predicted by the PSM plate model; k (values of 2.5 and 3.3) is the conductivity in Wm-1 C-1.