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R. Meyer J. Köhler A. Homburg Explosives

R. Meyer J. Köhler A. Homburg Explosives

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Solid Propellant Rockets<br />

by incorporating special accelerating or retarding additives. The propellant<br />

charge must be carefully examined for cracks, since in their<br />

presence the combustion will not proceed uniformly. If case-bonded<br />

charges are employed, adequate cohesion between the wall of the<br />

combustion chamber and the propellant charge (W Case Bonding)<br />

must be ensured.<br />

The advantages of solid rockets are the short time needed for the<br />

actuation, long storage life, and a simple design.<br />

The burning process in the rocket motor is influenced by:<br />

the thermodynamic performance values of the propellant (W Thermodynamic<br />

Calculation of Decomposition Reactions), the burning characteristics<br />

of the propellant grain (W Burning Rate), depending on its<br />

shape, and by the pressure influence on the burning rate. The pressure<br />

exponent can be zero in the case of modern propellants (“Plateau”,<br />

“Mesa”, W Burning Rate). The pressure function of the burning<br />

rate cannot be described by a universal equation, but within smaller<br />

pressure ranges the equation of Saint-Robert or Vieille equation is<br />

applicable:<br />

r = a pa (1)<br />

r: rate of burning normal to the burning surface<br />

p: pressure<br />

a: pressure exponent<br />

a: constant<br />

(W also Burning Rate, Charbonnier equation.) At any time during the<br />

reaction, equilibrium must exist between the gas produced<br />

r · fT · r (2)<br />

fT: burning surface<br />

r: density of propellant<br />

and the gas discharged through the nozzle<br />

p · fm · CD<br />

(3)<br />

fm: nozzle cross section<br />

CD: mass flow coefficient<br />

The ratio fm/fT = nozzle cross section to the burning surface at any<br />

time is called W Propellant Area Ratio (“Klemmung”) K; the equations<br />

(2) and (3) are considered to be equal: equation (1) can be<br />

rearranged to<br />

p = a<br />

CD<br />

290<br />

†K 1<br />

1–a (4)<br />

Equation (4) allows plotting of the gas pressure-time diagram, if a, CD<br />

and a are known and the course of the propellant area ratio K with the<br />

burning time can be assumed. Modification of the pressuretime diagram<br />

may be caused by the pressure falling off along the propellant

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