The
map
above
shows
how
much
the
North
Magnetic
pole
has
shifted
between
1590
and
today.
From
the
map’s
author:
Positions
of
North
Magnetic
Pole
of
the
Earth.Poles
shown
are
dip
poles,
defined
as
positions
where
the
direction
of
the
magnetic
field
is
vertical.Red
circles
mark
magnetic
north
pole
positions
as
determined
by
direct
observation,
blue
circles
mark
positions
modelled
using
the
GUFM
model
(1590–1890)
and
the
IGRF-12
model
(1900–2020)
in
1
year
increments.For
the
years
1890–1900,
a
smooth
interpolation
between
the
two
models
was
performed.
The
modelled
locations
after
2015
are
projections.
Why
and
How
the
Earth’s
North
Magnetic
Pole
Shift
The
Geodynamo
in
the
Outer
Core
-
Molten
outer
core:
Earth’s
magnetic
field
originates
primarily
in
its
liquid
iron–nickel
outer
core.
Convection
currents
in
the
molten
metal,
combined
with
Earth’s
rotation,
create
electric
currents.
These
currents
generate
a
magnetic
field
through
what
is
called
the
geodynamo. -
Constant
flux:
Because
the
flow
patterns
in
the
outer
core
are
dynamic
(like
weather
patterns
on
Earth’s
surface,
but
on
geologic
timescales),
the
magnetic
field
is
never
entirely
static.
This
leads
to
gradual
“secular
variation”,
or
drift,
in
the
field
configuration. -
Pole
wandering:
The
magnetic
poles
are
where
field
lines
are
most
strongly
vertical.
As
the
magnetic
field
changes,
these
“verticality”
points
move.
The
North
Magnetic
Pole
has
therefore
been
wandering
across
the
Arctic.
Rate
of
Drift
-
Over
the
last
century
and
a
half,
the
speed
of
the
North
Magnetic
Pole’s
motion
has
varied
significantly. -
In
the
early
20th
century,
it
moved
roughly
10
km
per
year. -
Around
the
late
20th
century
and
early
21st
century,
measurements
indicated
the
drift
speed
increased
to
over
50
km
per
year. -
Recently,
there
have
been
indications
that
the
speed
may
have
slowed
somewhat
again,
but
the
pole
still
continues
to
move
in
the
general
direction
of
Siberia.
A
Brief
History
of
North
Magnetic
Pole
Observations
-
James
Clark
Ross
(1831):
The
British
explorer
who
made
one
of
the
first
well-documented
discoveries
of
the
approximate
location
of
the
North
Magnetic
Pole
on
the
Boothia
Peninsula
in
Canada. -
Later
Arctic
Explorers
(late
19th–early
20th
centuries):
Explorers
like
Roald
Amundsen
confirmed
that
the
pole
was
no
longer
exactly
where
Ross
first
found
it,
noting
a
shift
of
tens
of
kilometers
over
the
decades. -
Modern
Measurements
(Mid-20th
century
to
Present):
Satellite
technology
(like
the
European
Space
Agency’s
Swarm
mission)
and
global
observation
networks
give
us
real-time
tracking
of
the
magnetic
field.
They
have
documented
the
significant
acceleration
in
the
pole’s
drift
rate
in
recent
decades.
The
Carrington
Event
(1859)
and
Geomagnetic
Storms
The
Solar
Superstorm
-
What
Happened:
On
September
1–2,
1859,
astronomer
Richard
Carrington
observed
an
intense
white-light
solar
flare
on
the
Sun.
The
associated
coronal
mass
ejection
(CME)
hit
Earth
roughly
17
hours
later,
causing
the
Carrington
Event,
the
largest
recorded
geomagnetic
storm
in
history. -
Effects
on
Earth:
Telegraph
systems
across
North
America
and
Europe
failed
or
caught
fire;
auroras
were
seen
as
far
south
as
the
Caribbean. -
Relevance
to
Pole
Shift:
Solar
storms
and
CMEs
can
temporarily
disturb
Earth’s
magnetic
field,
creating
geomagnetic
storms.
However,
long-term
pole
shifts
are
tied
more
to
core
fluid
dynamics
(the
geodynamo)
than
to
external
solar
activity.
Events
like
the
Carrington
superstorm
can
produce
short-lived
perturbations
but
do
not
directly
cause
the
slow
secular
drift
of
the
poles.
Geomagnetic
Reversal:
History
and
Mechanism
What
Is
a
Geomagnetic
Reversal?
A
geomagnetic
reversal
occurs
when
the
North
and
South
Magnetic
Poles
effectively
swap
positions.
In
the
rock
record,
this
can
be
seen
as
a
flip
in
the
orientation
of
magnetic
minerals,
which
align
with
Earth’s
ambient
magnetic
field
at
the
time
of
their
formation.
Historical
Record
-
Brunhes–Matuyama
Reversal
(~780,000
years
ago):
The
most
recent
major,
well-confirmed
reversal
in
Earth’s
geological
record. -
Frequency:
Over
the
past
20
million
years,
reversals
have
occurred
on
average
every
200,000
to
300,000
years,
but
the
timing
is
irregular
and
can
vary
greatly. -
Multiple
Reversals:
Analysis
of
ocean
floor
basalts
(especially
along
mid-ocean
ridges)
has
revealed
a
“barcode”
pattern
of
magnetic
stripes.
These
stripes
reflect
past
reversals
as
new
crust
is
created
at
the
ridges
and
locked
in
the
prevailing
magnetic
polarity.
Timescale
and
Process
-
Gradual
Flip:
Contrary
to
the
idea
of
an
“overnight
flip,”
reversals
often
unfold
over
thousands
of
years.
During
these
transitions,
the
magnetic
field
can
become
weaker
and
more
complex,
with
multiple
“north”
and
“south”
poles
possibly
appearing
in
different
locations. -
Field
Strength
Decline:
Some
measurements
suggest
Earth’s
overall
magnetic
field
strength
has
decreased
by
around
10-15%
in
the
last
150–200
years,
prompting
speculation
about
whether
a
reversal
might
be
“due.”
However,
the
field
has
weakened
and
recovered
many
times
in
the
past
without
a
complete
reversal.
Enjoy
this
map?
Please
help
us
by
sharing
it:
Go to Source
Author: Brilliant Maps