G.S. Golitsyn A.M. Obukhov Institute of Atmospheric Physics, RAS Moscow, RF

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STATISTICS and ENERGETICS of the SOLID EARTH PROCESSES: RELIEF, PLATES, EARTH PROCESSES, VOLCANOES G.S. Golitsyn A.M. Obukhov Institute of Atmospheric Physics, RAS Moscow, RF

description

STATISTICS and ENERGETICS of the SOLID EARTH PROCESSES: RELIEF, PLATES, EARTH PROCESSES, VOLCANOES. G.S. Golitsyn A.M. Obukhov Institute of Atmospheric Physics, RAS Moscow, RF. a). b). Relief. Decomposition on spherical harmonics up to number Earth Venus Mars(200 km) - PowerPoint PPT Presentation

Transcript of G.S. Golitsyn A.M. Obukhov Institute of Atmospheric Physics, RAS Moscow, RF

Page 1: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

STATISTICS and ENERGETICS of the SOLID EARTH PROCESSES:

RELIEF, PLATES, EARTH PROCESSES, VOLCANOES

G.S. GolitsynA.M. Obukhov Institute

of Atmospheric Physics, RASMoscow, RF

Page 2: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

a)

b)

Page 3: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

ReliefDecomposition on spherical harmonics up to number

Earth

Venus

Mars (200 km)

Legendre polinomials

planetary radius

2S n n4 180n

4 50n

75n

01 0

, 1 cos sin sinl

clm slm lml m

r a c m c m P

sinlmP

0a

n

Page 4: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Spectral dispersion

Earth km, km

Venus km , km km

Relief spectrum for regional transsects

, , km

Turcotte for 60 trajectories

Synthetic spectrum

1

2 2 2 20l clm slm hm v

V k a c c

2 6.1h 2

2.5h

2 0.9h 2 0.95h 1

nkS k k 2

kl

0.3 30l

2.03 0.04n

2.01n

Page 5: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Dependence of the spectral power density S on wave number k for the synthetic depositional topography. The data points are the average of

50 simulations.

Page 6: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Slope Spectrum

white noise in the space

m for large scale harmonics of Earth

erosion:

water flows on slopes

and wind decelerates over slopes

0.3k

2kk S k

Page 7: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Structure function

If , then

m, km, then m

2

hh x r h x D r

2 1 cosD r kr S k dk

2kS k k kD r r

0.3k 1000r 1/ 2 550D r

Page 8: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

In vertical motions the whole crust with km is involved

The relative dispersion of the potential energy

- mean geothermal flux density

Myr

30H

hU Hg

2 29 10F Wm

3 3 4 2 3

min 2 2 7

3 10 3 10 10 2.5 101

9 10 3 10 /

U kgm m ms m

U Wm s yr

Page 9: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Convection

In the viscous fluid

the rate of energy dissipation/generation of kinetic

energy at convection

thermal expansion of mantle

ms , kgm , m /s K

km, m s m s

cm yr , stress at core?

1/ 20.1 /u v d/ pgF c

5 12 10 K

10g 2 33 10 3 700pc 2 2

3000d 172 10 2 1 1110 2 3

6u 1

Page 10: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Check of the convection velocities in viscous and turbulent regimes

Page 11: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Earthquakes

Gutenberg-Richter, 1942, Ishima, 1939 (see Kasahara, 1981)

Correlation function of random forces

where is the stress minimum correlation time

(the free energy of deformation)

0f f fB f t f t

0

f

d

dt

Page 12: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Frequency spectrum

white noise

motion equation, momentum

red noise

0

cosf f fE B d const

dpf

dt

22p fD p t p t

2p fE

p

Page 13: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Flow of events

, cumulative frequency

mean waiting time (Feller)

energy

maxE

E

N E N E dE

1

EN E

2 2p fE p D

/ ffE N E N E

E

Page 14: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Examples

Tsunami:

land slides upon the soil mass

Number of lakes

,

Turcotte, Ryanzhin

nN h h 1.01n

nN M M 0.95 1.1n

nN S S 0.93 0.95n

M

Page 15: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Earthquakes again

magnitude m = 1 ar

Gutenberg-Richter

for , for

S.S. Grigorian 1988, Rundle 1989

Young modulus, mean slip

Seismic moment

0lg /m S S 0 100S 2

N m a bm

1b 8m 1.5b 8m

M Su

2lg 63

m M

u

Page 16: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Energy of seismic waves (Kanamory 1994)

total energy of an event

stress drop Bar = 4 MPa Aki, 1967

length scale

Similarity criterium

at , the process 2 D

1 D

Chile , Sumatra

56 10 ,sE M 00.07sE E

40

1/ 3/L M

/L H

1 7.5,m 7.5m 7.5m

9.5m 9.2m

Page 17: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF
Page 18: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF
Page 19: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Scatter plot of observed rupture areas against the

theoretical values

Page 20: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

The scatterplot of the observed rupture length against the theoretical value

Page 21: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

Dimensional analysis: energy dimension, E, time, T

seek , by geothermal flux

seismic moment

similarity criterium

at …

from global catalogs

1N M 1,F ET

M E

,FN M f

M

1/ 3/MH

L H

1: 1f a

1/ 3

2 / 31/ 3

/ 0.4M FN M M

H H

Page 22: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

at

for large

2lg 63

m M

lg ,N m a bm 1/ 3lg 12 / ;a F H 1b

1 0.4f

0.4F

N MM

m 1.5,b lg 0.4a F

Page 23: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

time in years.

globally: one quake per year with

global geothermal flux

effective action coefficientaveraged over millenia

7.6m

2lg 63

m M 202.5 10M N m E310E M

3 3 2010

7

10 10 2.5 1010

1 3 10 /

MW

yr s yr

134.5 10F W 10

413

102 10 0.02%

4.5 10F

!!fEN E

lg 7.6 ,N m m

Page 24: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF
Page 25: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF

volume energy

/ 31 ,n nN V aV a r 2.14;n / 3 0.71n

V E

2lg lg ,

3N V a V 1lg ;a a 510

Page 26: G.S. Golitsyn A.M. Obukhov Institute  of Atmospheric Physics, RAS Moscow, RF
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