Geoscience Reference
In-Depth Information
The spectrum of lightning discharge is given by m.!/ D MF .!/, where M is the
“magnitude” of the current moment and the function F .!/ describes a shape of the
spectrum. Here we have made the following abbreviations
Z
i 0 Ǜ H LF .!/
2
cosh .kh/
sinh .kd/
kJ 1 .kr/
3
g r D
dk;
(5.56)
0
Z
0 F .!/
2
cosh f k.d h/ g
sinh .kd/
g ' D
kJ 1 .kr/dk
(5.57)
0
Z
LJ 1 Ǜ H v ' Ǜ 2 H C Ǜ P C LJ 1 Ǜ P v r kJ 1 .kr/
3
w r D
dk
(5.58)
0
where the functions , LJ 3 , and q are given in Eqs. ( 5.30 ), ( 5.31 ), and ( 5.34 ),
respectively, J 1 .kr/ is the Bessel function of the first kind and the first order.
As is seen from Eqs. ( 5.54 )-( 5.58 ), only the radial component ıB r includes the
resonance factor q, while the perpendicular component ıB ' does not exhibit the
resonance properties. The resonance factor q in turn depends on the “wave numbers”
2
2 x 0 for the ground,
ionosphere, and magnetosphere, respectively. The factor LJ 3 in denominators of the
functions g r and w r describes the field damping with distance due to the presence
of exponential functions. The latter factor is a function of d and ; that is, a function
of the atmospheric and ground parameters.
The radial component given by Eq. ( 5.54 ) consists of two terms. The first
one describes the IAR excitation due to the CG lightning discharge whereas the
second term is caused by the neutral gas flow inside the E-layer. Alternatively, the
perpendicular component ( 5.55 ) can be excited by only the lightning discharges.
However, the last statement holds true only in the case of axial-symmetrical
distribution of the neutral wind velocities in the ionosphere.
D k 2
i 0 ! g , I D k 2 L 2
x 0 , and 2 M D k 2 L 2
5.3.4
A Model Calculation of the IAR Spectra
To study the contribution of a solitary lightning discharge to the SRS of the IAR, we
now shall ignore the neutral gas flow in the E layer, so that the neutral wind velocity
is assumed to be zero. Figure 5.12 shows a model calculation of the lightning-
generated spectra of the resonance component ıB r for the typical nighttime
parameters of the mid-latitude ionosphere. The lightning flash contains three CG
return strokes. The discharge shape and the spectrum, F .!/, are approximated
by Eqs. ( 3.7 ) and ( 3.8 ). The numerical parameters of the lightning discharge used
in making this plot are given in Chap. 3 . The numerical values for the various
magnetospheric, ionospheric, and other parameters are: V AI D 500 km/s, V AM D
5 10 3 km/s, L D 500 km, d D 100 km, z D d, h D 0, g D 2 10 3 S/m,
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