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S3-2 REV 4460/N
15 October, 1976
60
2330
2336
2340
2346
E
x
30
700
500
300
B
y
0
100
2
100
2300
230
2500
2
700
260
10
9
10
8
10
7
180°
90°
0°
UT
MLT
ALT
2330.0
60
18.0
249
2332.7
70
17.5
238
2335.5
80
15.4
245
2340.5
80
9.0
296
2342.9
70
7.9
354
2346.0
60
7.5
430
Figure 8.3b
S3-2 observations from a north polar pass on October 15, 1976. The dashed
line is the baseline for
B
y
. [After Smiddy et al. (1980). Reproduced with permission of
the American Geophysical Union.]
Now consider the ionospheric load. In this resistive medium the horizontal
current from dawn to dusk is
J
E
x
h
. In a steady state the current entering
the ionosphere in current sheet 1,
J
z
dx
, must be equal to the total horizontal
current in the vertical extent
h
of the ionosphere. Thus, making use of
=
σ
p
δ
δ
B
y
=
μ
0
J
z
dx
and the fact that
p
=
σ
p
h
, we have
δ
B
y
=
μ
0
δ
E
x
(8.17a)
p
This equation may be rewritten in the equivalent forms
δ
E
x
=
δ
B
y
/μ
0
p
(8.17b)
δ
B
y
/δ
E
x
=
μ
0
p
(8.17c)
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