References
and
notes
There
are
three
kinds
of
references
in
this
monograph:
(1
) Key
words
a
nd
phases
,
and
search
strings,
which
can
be
ins
e
rted
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sear
c h
engine
such
as
Goo
g le.
These
are
set
in
special
type
,
and
are
called
Googlets
;
(2
)
web
addresses
;
and
(3)
normal
author-date
refer-
enc
e
s.
Supplementary
m a
terial
can
be
found
on:
www.gps
.
caltech
.
edu
l~
dla
l
www.caltechbook
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l
141
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mantleplumes.org
This
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also
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found
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anderson,
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ry
of
the Earth,
abbreviated
TOE
,
c
an
be
found
on
www.
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techbook
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cal
tech
.
edu
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14
I,
and
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mantleplumes
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ures
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s
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maps
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compl
e
ment
some
of
the
material
published
here
.
The
following
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strings
are
also
useful
for
find-
ing
material
that
supplements
the
text
:
treatise
on
geochemistry
physics
of
the
earth
' s
interior
convection
in
the
earth
and
planets
N
otes
on
Goog
le
ts
The
Web
has
completely
c
hanged
the
wa
y
re
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and
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rese
a r c
h,
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arch
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movi
es
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the
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of
inter
est.
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example
,
if
one
wants
to
investigate
the
relationship
between
the
D
ec
can
trap
s
and
Reunion
one
can
insert
[Reu
n
ion
Deccan
mantlep
l
umes]
into
Google
.
If
one
wants
to
know
more
about
shear-wave
splittin
g
or
the
Love
Raylei
g h
discrepancy
one
just
types
into
Coo
gle
[shear-wave
splitting]
or
[Love
Rayleigh
discrepancy]
.
Often
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and
a
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list
of
references
e.g .
[Anderson
tomo-
graphy]
.
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e d
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a l
and
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c
an
be
used
without
interro
g
atin
g
the
web
.
But
if
this
resource
is
available
and.
if
used
,
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n
cut
down
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r e
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plementary
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cs
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boldface
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usual
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of
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g
and
footnotin
g.
They
can
be
treat
ed
as
keywords
,
useful
but
not
essential.
The
key
phrases
have
been
desi
g
ned
so
that,
when
used
in
a
search,
th
e
top
hits
will
contain
relevant
information.
There
may
be,
of
course,
some
un-useful
and
redundant
hits
in
the
top
five
.
Supplementary
and
c
urrent
material
can
be
found
with
keywords
Don
L
Anderson
and
mantleplumes
.
The
Gen
eral
Ref eren
ces
, Suppl
eme
ntary
Re
adin
g
and
R
ec-
ommend
ed Reading
sections
that
ar
e
common
in
many
monographs
of
this
type
have
been
largely
replaced
by
Googlets
that
come
before
the
main
referenc
e
se
c-
tion
of
each
chapter
.
Ref
e
ren
ces
General
references
Ther
e
are
many
fads
, false
starts
and
dead
ends
in
all
sc
ientific
endeavors,
but
there
are
also
some
rock
-
solid
foundation
and
milestone
papers
.
The
followin
g
is
a
hi
g
hly
selective
compilation
of
significant
publi
c
ation
s
in
g
eodynamics
,
Earth
structur
e
and
mantle
geochem
-
istry
,
most
of
which
has
stood
the
test
of
time
and
have
set
the
stage
for
either
our
present
understandin
g
or
d e
monstrate
that
we
have
wandered
from
a
fruitful
be
g
inning.
If
the
net
and
Googl
e
disappeared
a g
ood
start
on
the
subject
matter
of
this
book
could
be
made
from
a
subset
of
the
publications
in
the
followin
g
list
.
In
many
respects
, we
have
lost
g
round!
Classical
references
Birch,
F.
(1952)
Elasticity
and
constitution
of
the
Earth's
interior.].
Geophys
. Re
s.
,
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,
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N.
L.
(1928)
Th
e E
volution
of I
gn eou
s
Ro
ck
s.
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NJ
,
Princeton
University
Press.
Bowie
. W.
(1927)
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stas
y .
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York
,
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.
Bullen,
K.
E. (1975)
Th
e E
arth
's D
ensity.
London
,
Chapman
and
Hall.
Bull
e n,
K.
(1947)
An
Introduction
to
the Theory
of
Se
ismology.
Cambridge,
Cambridge
University
Pr
ess.
Chandrasekhar
,
S.
(1961)
Hydrod
y
nami
c
and
Hydroma
gnetic S
tability.
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Clar
e
ndon
Press.
Daly
, R. A. (1933)
Ign
eous
Rocks
and
the
Depths
of
the
Earth
.
New
York,
McGraw
Hill.
Daly,
R.
A.
(1940)
Strength
and
Structure
of
the
Earth
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Englewood
Cliffs,
NJ,
Prentice-Hall.
Darwin,
G.
H.
(1879)
On
the
bodily
tides
of
viscous
and
semi-elastic
spheroids
and
on
the
ocean
tides
upon
a
yielding
nucleus.
Phil.
Trans.
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Soc.
London
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1970.
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S.
(1961)
Continent
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ocean
basin
evolution
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floor.
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854-7
.
Du
Toit
,
A.
L.
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Our
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ering
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Th
e Bow
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ls
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, W.
M.
(1969)
Convection
and
stress
propagation
in
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upper
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Application
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e
rn
Physics
to
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,
S.
K.
New
York,
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Wiley
&
Sons,
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.
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.
Gast
,
P.
W.
(1969)
The
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of
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from
St.
Helena
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Ascension
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tt
.,
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, McGraw-Hill.
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Edition
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York,
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A.
(1937)
The
viscosity
of
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History
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In
Petrologic
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e
s:
A
Volume
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of
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F.
Buddin
gton,
eds.
Engel
,
A.
E.
J.,
James,
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L.
and
Leonard,
B.
F.
Boulder,
CO,
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of
America,
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.
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age
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e,
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,
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transport
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.,
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H.
(1926)
The
stability
of
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layer
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, H.
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, H. (1939)
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with
new
editions
in
1948
and
in
1961
(also
in
the
Oxford
Classic
Texts
in
the
Physical
Sciences
series).
REFERENCES
AND
NOTES
357
Jeffreys,
H.
and
Swirles,
B. (eds
.) (1971-77)
Collect
ed
Papers
of
Sir
Harold
Jeffreys
on
Geophysic
s and
other
Sciences
(in
six
vo
l
umes).
London
,
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&
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la,
W.
M.
(1968)
An
Introduction
to
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etary
Physics,
the
Terrestrial
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L.
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On
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horizontal
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higher
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-
65
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Thompson,
D'Arcy
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Growth
and
Form.
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University
Press
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A.
(1924)
The
Origin
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Continents
and
Oc
eans
.
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York,
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.
CHAPTER
REFERENCES
PART
I.
PLANETARY
PERSPECTIVE
Chapter
I .
Origin
and
early
history
Solar
system
abundances
Or
igin
of
Moon
References
Anders,
E.
(1968)
Chemical
processes
in
the
early
solar
system,
as
inferred
from
meteorites.
Acct.
Ch
em . R
es
.,
1,
289-98
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Fuchs
,
L.
H
.,
Olsen,
E.
and
jensen
,
K.
(1973)
Mineralogy
,
mineral-chemistry
,
and
composition
of
the
Murchison
(C2)
meteorite.
Smithsonian
Contrib.
Earth
Sci.,
10,
39
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Grossman,
L.
(1972)
Condensation
in
the
primitive
solar
nebula.
Geochim.
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Acta,
36,
597-619
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Grossman
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L.
and
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(1974)
Early
chemical
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solar
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ce
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12,
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].
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and
Anders,
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Safronov,
V.
S.
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AND
NOTES
Centre
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Scientifique
,
pp
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3 .
Selected
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Murthy,
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Chapter
2.
Comparative
planetology
o r i g
in
of
the
M
oo
n
a
nd
the
si
n g l e
im
pa
ct
hypot
h
esis
origin
o f
th
e
Ear
t h
a
nd
Moon
timing
of
meta
l -
si
li
cate
fractio
n
atio
n
Ele
m
entary
an
d
nu
clidic
a b
undances
i n
the
solar
syste
m
t i
ming
of
meta
l
-s
il
icate
fractionat
i o n
w
Hf
References
Ha
rtman,
W.,
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and
Taylor,
G.
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Origin
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Houston,
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Chapt
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The
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s
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eart
h
e n
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ea
r
th
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L.
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W.
and
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Chemical
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and
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Pro
c.
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77
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E. (1977)
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1299.
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School
of
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A.
(1962)
Chondrules
and
the
origin
of
the
terrestrial
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Nature,
194,
127-30.
Further
reading
Anders
,
E.
and
Owen,
T.
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shallow
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far-from-equilibrium
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tomographic
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Harper
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Oliver
Hager
O '
Connell
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often
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mantl
e
convection
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the
plates
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comp
l
ex
computer
simulations
of
man-
t le
convection
have
not
yie
l
ded
anything
resemblin
g
plate
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By
about
1980
the
drivin
g m
ec
hanisms
of
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ate
tectonics
were
fairly
well
und
e
rstood;
the
p l
ates
and
slabs
drove
themselves
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were
respon-
si
bl
e
for
density
variations
in
the
underlying
man-
t le.
TI1es
e
plate
models
of
mantle
convection
assumed
shallow
return
flow
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nd
upper
mantl
e convec-
tion.
TI1e
advent
of
supercomputers
an
d
hi
g h
Rayleigh
numb
er
convective
simu
l
ations
of
whole
mantle
con-
vection
h ave
not
g i
ven
us
much
mor
e
add
iti
onal
insight
. Th e
upper
mantle
counterflow
and
top-down
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tecto
ni
cs
are
mostly
over
l
ooked
in
mod-
ern
treat
ises
on
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geody-
namics,
which
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mantle
convec-
tion
.
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milestone
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geo-
dynami
cs
and
plate
tectonic
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listed
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