Theory of the Fireball
Theory of the Fireball
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