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ESA Document - Emits - ESA

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s<br />

HMM<br />

Assessment Study<br />

Report: CDF-20(A)<br />

February 2004<br />

page 178 of 422<br />

The materials used within the debris and insulation shielding are selected and sized so that both<br />

functions (impact and thermal) can perform optimally under their respective loads. Low<br />

conductivity materials are therefore integrated: the open cell foam (three layers of 10 cm thick,<br />

preferred to closed cells for their better thermal behaviour under vacuum), the Kevlar fabric (5<br />

layers) and the Nextel AF10 ceramic fabric (3 layers) offering also adequate and stable (material<br />

inorganic, therefore no degradation against time to be expected) thermo-optical properties<br />

(measured values: alp=0.24, eps=0.88).<br />

Figure 3-37: Debris shielding/thermal protection (L), Max. Temp. of external layer (Nextel) (R)<br />

Assuming a three-axis-stabilized spacecraft, the temperature evolution of a permanently<br />

illuminated surface (Nextel AF10) is shown in Figure 3-37. Note that beyond a certain range, a<br />

correction appears necessary to come to acceptable temperatures at the hull internal structure<br />

(see following paragraph). The spinning of the spacecraft to homogenize temperatures is not<br />

considered (solar array pointing constraints).<br />

3.3.3.4.6 Thermostatic system<br />

Certain surfaces that cannot be protected by insulating means (docking system for the MAV) are<br />

treated (oxidation anodic, alodine) to minimise heat losses. On the internal face, coils<br />

(circulating fluid from primary loop) thermostatically control the temperature (condensation<br />

avoidance) and the heat exchanges (control of the heat losses). An adequate redistribution of the<br />

rejected heat (thermostatic coils) therefore reduces the use of heater power to the minimum.<br />

When not directly accessible to fluid lines, externally mounted elements will require the use of<br />

strip heaters combined to an adequate insulation.

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