The boundary between the northern and southern Sqcurrent loops over the African continent
The regular produced
quiet day geomagnetic
by electric current
togcthcr
with
their
induced
SKISSER
currents fioxing
hemisphere
e.xternal d:ril)
The
Sy current
studied
ha\c
been
northern
since the early found
to
summer
developed
than
and
A complicating low latitudes
from
the
west to east known
of CH~IM~X
occur. the
For
example,
northern
the southern
and tends
south ofthepeo@raphicalequator
durmg
loop
is more
to penetrate
IP~~c~zand WILKISS.
IY)hj) The
f~~rm of the daily
decltn:ltron
(1)~ .lt
m;l~nstlcallv
a
relatl\e
SIOLI.
lY631 Thus
\tatll)n
the \ou~h\rard
the mornlnp$ declln.ttlon.
~~11
loops
at a moderate
latitude
component
produce
III
theafternoon
follo\red cxpcctcd
to hho\r
daily
and no regular pattern. the morning
compared
seasonal solar controlled the current station
Ilo\\
by a minimum
in the
hemisphere stations
loops
in theshape
be underdilTerent
to the afternoon.
loops the daily
be of
loopsin
Because ofthe
boundary
declination
near the geographical
near
would
of small amplitude
Due todistortion
shift ofthe
flou 01
in east declination
the current variations
III
In the eastward
peak. Magnetic
between
thc:\ol-tlcc:\?~t~chstationscan
sinplc
a peak
mlnimum
hx an afternoon
the boundary
northern
of current
In the southern
there I\ ould he a morning
:i of
(PKICF and
due to thenortherly
currents.
o\d~c~~d
on
of the position
to the current
This \rill be follo\ved
decltnatlon
of the mapnctlc obseriatorj
qutet da> IS Indicative
the station
the
variation
magnetic
bet\teen
variations
equator
houndciry
at a
can show
all threet~p~\ofbehaviouratdifferenttimesofthe)’ear.
297
currents.
1.7 S) b>
Nairobi
under
the southern
in Aupust..lanuar~
feature \\ hen stud>lng
is the intense band ofcurrent as the equatorial
in erect. a local intensllicatlirn
and
latitude
and
respecti\,el!
the
changes in these parameter>
(J)
nearthe
of
at the world
(geographic
Curves -4. R And Cshoiv
of the northern
April:October
and these have been
work
(1973).
currentsand
in
in F-I~. I \\ hlch shows such carlatmns
at Nairobi
the influence
in the southern intensity
observed
observatories
B~H~I I \ (IY-IO). Seasonal
side of
clockwise
can be deduced
variations
nrtti w-l\ ofmagnetIc much
shape
systems
the outer
take the form of two counter
and clockwise
size.
geomagnetic
within
On the daylight
the Earth the ionospheric
hemisphere
This is illustrated
currents
large I~~ps with currents the northern
(SC/) arc
observed
laycrb of the Earth.
conducting
variations
systems in the ionosphere
Sqcurrenth Ilouinp
electrqlet.
of the Sr/ current
at
from This is. uh~ch
S
298
occurs
v.irhin
magnetic
a rcti degrees
dip equator.
enhanced
electrical
conductivity
B4KER
obsrr\ed
in the geomagnetic
enhancement the dall)
of. and centred
A theoretical
given by
daily
variations
is a local
2 in the amplitude
of the horironral
component
of
(H) of
field.
R (-under S loop) variations
at
I I .Afrlcan observa~ories(lisred
in Table I)on aseries of
fi\e
In each of the months
magnetically
to-da) to
April,
quiet
days
July and October
and morning-to-afternoon
olthe
boundary
occur.
In
equators equator
Africa
the
America
(studied
bq Ht,rros.
magnetic
equator
is at about
studies
special interest brtuecn
ij
and
Figure \;tmtion~
northern
2 \ho\\
5 sketcho
111saqt
declination
current
loop.
and ICI the h[,und;lr! near equ:llorlitl
constant hh,iped parameter
latitude d.111\
R. \ho\\n
idealixd
rlw
tn
daily
under (a) the current
to he under
and ‘tfternoon
‘T‘h~s pi\es
between
loop
the laoph. Frequently.
I\ not al\\.i!\
\arl;tllon\
the
(b) the southern
lo~>p\ In the mrlrning
iT any.
SC/ system.
rot- xtationb
het\\een
I).
I
S loop
I
latitude.
arc thus of
the relationship.
or
Dm
in
of South
1967a and b) where the
5tatlOn appears
the hi)und;!l-!
side
I? S geographic
external
I
am N IOOD
geographic
aXis and the houndar!
d llie
loops
I
and the magnetic
on the western
in determining
I
R zero o+jboundary
, c
loops were found
In these two regions
the electrojer
lhe current
that
shifts in the position
liesclose to IO h geographiclatltude.Thisis to the situation
currenl
E u
magnetic
contrast
5
‘0
1969. Seasonal, day-
between the current
have a large separation.
Comparatl\e
R (+ under N loop)
this region w’as
This paper studies rhe daily declination
January.
I
[or
(1953). The main efl’ect
h) a factor ofabout
the eeomagetic
SH.XH
;tnd L
on. the
explanation
wlthin
and MARTYS
lariation
J SLI\XIK
parallel
a
different indicating
IU ;i hne of
to td! “91” or (el “W”
The
diurnal
range
in t.ig. 1. \$a\ ~~22 lo locale
Ihe
boundar! taking
in a quantitatll
positive
values south.
with
(Fig.
3) enable
determined
with
show “M” separate Figure
baundar!,
pm.
latitude
011
boundar!
3a-d
conclusions
were plotted
particular
da!>. ma!
be
for the five international Table
between the northern
and southern
the boundar!
geographic
latitude,
Hecauseofthe
solar contrill
ol”lono~phrric
electron that
current month>.
was stable at about degree\
south
&the
dcnslly
III
rhe
orthe boundar\
except for the morning
it ~+as several
he expected
April. Jul! and
2 summarises
\vith regard to the positron
each day. F-or the two cqumoctial
u,hen
bc
but with lo\\ time re\olution.
1969 respecti\el!.
October.
queer to
When station>
position,
quiet days for the four months Januar!,. October
itsell
for gi\cn
accurac\.
type variation\
a.m. and
determined.
the
Iarnude
reasonable
or “W”
nrgati\e
zero range at the boundar!
Plots ofR against geopraphlcal da)5
It ma! be regarded ‘1,
e \\ a).
values north of the boundar!.
systems on April
and
II N i 2 of 23 April
of the equator
latitudsdlstrlburl,,n the E replon it mlghr
nenr rhe equlno\c<
the hounder!
shouldlieclose~~~the~eo~raphicalequatorandthat
the
0
. A
D ;
3rd
-
IO th
6th
*
19th
IO th l3Th 29th
‘3
r
23rd
l
26
a
; + A
0
th
omtopn
am top1 ll
. 0 +
0
Jan 1969
Apr
1969
~240
__-_ 3c
2.
, !i
4th
3
1:
19th
/v
20th
!. Lm
.’
*.
eo-
v
29th topm
__ ,-,
7 :.-7-
/ d
I20 -
5 th
I?
‘c
8Ih
,*
14th
‘C ‘0
15 th 26th
I.
30th
40-
B ;‘
1 5 C \ z
I d .
+
O--
-4c-
Qz
.
8”
E’ .
-8O-
-120-
1
-160-
-2oo-
I
30 ‘k
20
IO
0 Lotltude
IO
I 20
I 30
act
1969
-j 4c :S
Y
iotlfude
Ik~g -7 (.II_(~I Show plot> elf R against lalltude for the I I observarorles llstsd in Table I. for qulrr &I!, 11, 4prll. July and October 1969 respecrively. The boundary positIon< for each da! h;t\c h?
300
J. SKIS\EK and E SHAH
N
Table 2 The latitude of the boundary betueen the current loops on the selected qmel days In 1969
Date
Boundary posltlon a m. pm
I969
Summary
for the monlh
Januar!
X 5 50.5 N 6 +2s 2 &I s
6
IO Ii 29 April IO 19 21 23 26 July 4 5 19 20 29 Ocrober 8 I4 15 26 30
norrhern
and
similar Africa
current
latitude
of the magetic
equator
ris r3 s +‘S 22s +2S
I2 II IO II II
i_ I.5 X kl5K A2 N .1.5X xI.iN
was south of the equator
dependence ion
responsible
electron
would
for
the
the
Sy currents
that Huctuations
from
of geopraphic
of the resulting
Sq currents.
as expected.
boundary
was clearly
equatorial position.
produce
latitude
5;
analysis
for
workers,
of the Sq field from
Polar
between was iii The
example
is the
Year geomagnetic
WILKISSI
1963lTheyplot
eqlrlpotentialsR(ratherthancurrents)forJmonths(l.e. summer).
and along the Greenwich
the R = 0 equipotential Sat
12OOLT.
In January, would
the converse
be expected
strengthening northern
with
and
hemisphere. position
to the sttuation
the southern
pushing
the
for quiet
occurred
There boundary latitude equator.
boundary is thus
shift of about during
of the magnetic
3 towards
equator
the dip
a much
larger
of the five days the
was at about clear
from
between 2-S and
the day with
a fairly
the
days in 1969 when the
was found to be quite variable
between thecurrent especially
loop
into
this does not accord
shaft on one day (6th). On three afternoon
for July
current
boundary
However
with results obtained boundary
meridian
shows a shift from 44 Sat 0800
equator
on
south shown
and BARTELS( 1930)
A good
system
of the geographical
11 N in the afternoon
by GAPMAX
later
day to day with limits in the mornings
the
system on
so that it dips further
arm and this trend is also clearly
on charts of Sq drawn and by many
the magnetic
current
control
and in the mornings
the day so that the boundary
range
on INSwestern
8.5 N. A northvvard
fourofthefivedaystherewasanorthvvardshift the
the
There 15
current
was thus towards
such days must bedistorted
to II In
field dependence
and geomapnctic
of movement
The shape of the northern
northern IS
vAB forces. It is likei!
well south
on
ll’k2’N
data for 1932-J by PRIcEand
field
on four days being close to 17 S. lHowe\er.
8 and 22 during
II
(throuph
the
which
the northern
and strengthened
the
which
of the Sr/ current\.
thus a mixture In July,
when
in the latter are largely responsible
the day to day variabilit!
equator.
of
will ,rls~~ha\e a magnetic
since they. arise hasic‘ili!
the
of the electrojrt.
the boundary
Eh4F.s
equator.
the magnetic
formation
dynamo
direction
over
with
conductivitics
boundaryat
be of
show that rhc
gyrofrequencies)
may also inllucnce
addition.
expanded
that
of the ionospheric and
electrojet
therefore
h!
as a m. same as a.m Zdme iis a.m as a.m.
in the morning
11 N after the development
to
seems possible
day
boundary al I I .5 N f I except a.m on 23rd when at 6.S
>ams as a.m.
the results
group
boundary shms N during - 3 (but by 17 on 6th)
boundary al 12-S+ I’ m the mornings on 4 days northward shift of between 8-X 4 days during the day
13 13 I2 II 5
in this
posibon variable day b!
II *l-N same as am.
and the axis of the
boundary shifted
the one day
boundary day
same as a.m same as a.m. same as a.m
1I N, coincident
was at about On
the
N 5 S h
+I +I +2 21
loops
electrojet.
It
I\:
I2 12 6 II5
for quiet days in April and October
boundary
N
115 xl
and sizes. However.
+05-N II N I &2X I +2h’ II iI N
s
7 51
8 ‘I_
southern
shapes
I05
1I
N.
general
trend.
The
loops is much nearer the than the geographical
at the equinoxes.
.4t other
times.
when the boundary IS south of the magnetic equator in
latitude between the tuo contments is more than 20
the mornings.
This
it tends t0 stabilize
along the magnetic
suggests that the dipequator posttinn. whtch also
equator later in the day. No cases of movement of the
differs in the same sense by about the same amount
boundary
between the tu’o continents. IS important in intiuencmg
away from
the magnetic equator
were
the boundary
observed. HL.TTOL
t 1967a and b) analysed declination data for
the IGY from a number ofclosely observatories
with latitudes
31.7 S in South
spaced geomagnetic
in the range 5S”N
America. As mentioned earlier.
gives the opp~~rtunity to compare the African reported
here with
those from
current,
this
contrjbutions
the complementary
situation m South America where the magneticequator
as it
period. This boundary during
mdivtdual days in the threecon\~entional seasons from inspection
of stacked 5 variations
for the range of
stations. There was considerableday-to-day
variability
during the post midd;i!
from the magnettc
during
of the northern
Europe/Africa.
the 1.G.Y.. noted
and southern
10. further
equator to about 1-Z Sin the morning but the boundary
daily revoiutton.
shifted
side of the
December solstice about S,N
the southern
In the
loops penetrated to
in the morning, shifting to about 5% in the
afternoon. and in the northern summer the boundary well south
of the magnetic equator in the morning
moving
to about
equator.
in the afternoon.
tit The boundary further
is
south
in
I:! S. the latitude
between South
of the magnetic
It is clear that the current Amertca
: in
Africa,
cspcc‘iall! in the .I and E seasons when its difference
in
the Sy current
Earth
shoax
of the magnetic
the two
mam current
displacement
equator. loops
hers.
system on the da&tit latitudes.
system as a whole appears to “run” “rail”
than in
one complete
a complicated
at IOR and moderate
and espectall!
loops is much
than
ffexures
SC/foci were on
Their results. and those reported
suggest that as the Earth rotates through
d:l\
that the
south in the Americas
average, the northern vortex penetrated south ofthedip to about 7 S in the afternoon.
equator
hours.
vartations
position
north
southern
the houndar!
PRICE and STC)TE( 1964). in their analysts ofquiet magnetic latitudes
on
and
tends to stabilize
is far removed
morning
averageabout
a gtv’en day. At the equinoxes,
This
the da?. to dra\t
northern
happens frequently, even on days when the
in the position of the boundary in all seasons and in the within
during
both
close to theastsoftheelectrojet
Hutton
on a number of
intensifies from
current systems.
at that time was at about 13-S geographic latitude. noted the boundary position
and southern
(ii) The trend tn both continents is for the electrojet
and
results
between the northern
current systems.
pattern Although
in some M a! on the
the boundur! may she\\
from the dip equator in the local morning
nt the
bet\ve,-11
consrderahk
;tt ccrtatn pertod.
W~MW