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Theory of the Fireball

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From y = 1.18,<br />

y=l-A<br />

Y=<br />

-1<br />

2.2 - 0*4/y<br />

X 2.2-0.4/y<br />

12.2 - x<br />

1-85<br />

11.2<br />

and <strong>the</strong> iso<strong>the</strong>rmal sphere disappears for<br />

l/1 . e6<br />

x = 12.2 = 3.811-<br />

2<br />

For <strong>the</strong>se higher altitudes, <strong>the</strong>n, <strong>the</strong> time when <strong>the</strong> iso<strong>the</strong>rmal sphere<br />

(6 -18)<br />

(6.20)<br />

disappears is a fixed multiple <strong>of</strong> <strong>the</strong> time when it is first reached by<br />

<strong>the</strong> cooling wave. This multiple depends only on y, and on <strong>the</strong> ratio<br />

Hc/Hl <strong>of</strong> internal to external ent'nalpy at time ta. Tne pressure at <strong>the</strong><br />

time x is<br />

2<br />

1/3<br />

-1.2<br />

P2 = PaX2 .= 1.0 ($) (6.21)<br />

For sea level, f (x) increases more slovly (<strong>the</strong> pressure decreases<br />

more slovly) with time; hence it takes somewhat longer to use q <strong>the</strong> iso-<br />

tnemal sphere. Conversely, t'ne pressure at <strong>the</strong> time t = t x will have<br />

2 aa<br />

decreased by a smaller factor from pa.<br />

For <strong>the</strong> simple case <strong>of</strong> nigher altitude, we can use (6.19) to calcu-<br />

late <strong>the</strong> fraction <strong>of</strong> <strong>the</strong> mass y 3 which -<br />

will still be in <strong>the</strong> iso<strong>the</strong>rmal

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