Geoscience Reference
In-Depth Information
1E+2
1E+3
1E+4
1E+5
1E+6
1E+3
1E+4
1E+5
1E+6
1000
1000
e
e
O +
O +
He +
F2-layer
H +
He +
H +
12LT
Summer
R=150
NO +
12LT
Winter
R=15
F1-layer
NO +
O2 +
O2 +
e
e
O +
O +
E-layer
100
100
1000
1000
O +
e
e
O +
He +
H +
He +
H +
NO +
NO +
O2 +
O2 +
O +
O +
00LT
Winter
R=15
00LT
Summer
R=150
e
100
NO +
100
O2 +
1E+2
1E+3
1E+4
1E+5
1E+2
1E+3
1E+4
1E+5
1E+6
number density [cm −3 ]
number density (cm-3)
Fig. 2.2. The height distribution of electron and ion number densities, at the 50
geomagnetic latitude for winter (left frame) and summer (right frame) at noon
(upper frame) and midnight (lower frame). After IRI-2000 [9]
10 11 N N 2 T e 1+0 . 93
10 2 T 1 / e 1 ,
ν e N 2 =2 . 5
×
×
10 10 N O 2 T 1 / 2
10 2 T 1 / 2
e
ν e O 2 =1 . 5
×
(1 + 4 . 2
×
) ,
e
10 10 N O T 1 / 2
ν e O =2 . 8
×
,
e
10 10 N H T 1 / 2
ν e H =4 . 5
×
,
e
10 10 N He T 1 / 2
ν e He =4 . 6
×
.
(2.1)
e
Electron-Ions
For the effective electron-ion collision frequency we use the expression [22]
ln 215
1 / 3 .
N 1 / 3 T i
N
T 3 / 2
T e
ν ei =5 . 5
(2.2)
T e + T i
e
Here, T e and T i are electron and ion temperatures in Kelvins (K).
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