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Theory of the Fireball

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4. ABSORPTION coEFF1c1ms<br />

a. Infrared / / .<br />

The main absorption in <strong>the</strong> infrared is due to free-free electron<br />

transitions. These are treated incorrectly in <strong>the</strong> paper by Meyerott et<br />

16<br />

al., in whicn it is assumed that such transitions occur only in <strong>the</strong><br />

field <strong>of</strong> ions. At. tke important temperatures <strong>of</strong> 8000' or less, <strong>the</strong> degree<br />

<strong>of</strong> ionization is or less. Therefore, <strong>the</strong> free-free transitions in<br />

<strong>the</strong> field <strong>of</strong> neutral atoms and molecules are much more important than<br />

those in <strong>the</strong> field <strong>of</strong> ions, even though each individual atom contributes<br />

far less than each ion.<br />

The effectiveness <strong>of</strong> neutrals in inducing free-free transitions has<br />

18<br />

been measured and interpreted by Taylor and Kivel at<br />

laboratory. As compared to one' ion, <strong>the</strong> effectiveness<br />

tant neutral species is<br />

N2 : 2.2 f 0.3 X<br />

N: 0.9 f 0.h x lo-=!<br />

0: Oe2 f 0.3 X lo-=!<br />

<strong>the</strong> Avco-Everett<br />

<strong>of</strong> <strong>the</strong> most impor-<br />

Thus nitrogen gives about <strong>the</strong> same contribution wne<strong>the</strong>r molecular or<br />

atomic, and <strong>the</strong> contribution <strong>of</strong> oxygen is very small. As a result, one<br />

atom <strong>of</strong> air is equivalent to about a = 0.8 X ion (<strong>of</strong> unit charge).<br />

The free-free absorption coefficient in cm'l is <strong>the</strong>n<br />

cLf f<br />

= 0.87 x 10 (%) 2(e-)(hv)-3<br />

= 7.0 T '-I/* (b) 2( e-) (hv) -3<br />

1<br />

I

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