Geoscience Reference
In-Depth Information
we have
=
ω
2
σ
σ
k
2
k
2
⊥
c
2
A
−
.
For low frequencies, when the first term on the right-hand side can be ignored,
the above reduces to
i
σ
P
σ
k
=
±
k
⊥
.
It follows from Fig. 2.4 and the last equation that the ratio of a longitudinal
scale
L
to the transversal scale
L
⊥
in the
F
-layer is of the order of
L
/L
⊥
∼
300. This means that the wave magnetospheric perturbations with
L
⊥
a
few kilometers, reach the
E
-layer almost without decay. But perturbations
with
L
⊥
<
1 km decay so much that they cannot reach the
E
-layer.
References
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Solar-Terrestrial Physics
, Clarendon Press, Ox-
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,
18
,
1939.
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