MISSION PLAN - PDS Small Bodies Node
MISSION PLAN - PDS Small Bodies Node
MISSION PLAN - PDS Small Bodies Node
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8<br />
10<br />
flare, no shielding<br />
6<br />
10<br />
4<br />
10<br />
2<br />
10<br />
250 mil<br />
36 mil<br />
60 mil<br />
100 mil<br />
0<br />
10<br />
-2<br />
10<br />
-4<br />
10<br />
-6<br />
10<br />
Heavy -Ion Peak Flux (/cm 2/day)<br />
(Omni-Directional)<br />
GCR 25 mil<br />
GCR 500 mil<br />
Shielding is an aluminum sphere of given radius.<br />
-8<br />
10 100 mil of Al = 0.686 g/cm2<br />
500 mil<br />
1000 mil<br />
-10<br />
10<br />
1 10 100<br />
LET (MeV-cm 2/mg)<br />
Figure 2.3-6b Heavy-ion Flux from a 95% Solar Flare at 1 AU and<br />
for Adams’ 90% Worst Case GCR<br />
2.3.3.3 Micrometeoroid<br />
Cumulative micrometeoroid fluence levels as a function of time from Launch is shown in<br />
Table 2.3-7. These selected times correspond approximately to each of the three<br />
aphelions and to the end of mission. The integral fluence is provided as a function of<br />
particle mass. The numbers correspond to 1-sigma levels of the JPL micrometeoroid<br />
environmental model. The 1-sigma uncertainty of the model assumes log-normal<br />
distribution, thus the 2-sigma and 3-sigma levels are 3 and 9 times of the numbers shown.<br />
Table 2.3-7 STARDUST Mission Micrometeoroid Environment<br />
Time: L+376.4 d L+1188.7 d L+2091.4 d L+2533.6 d<br />
MASS (grams) FLUENCE (particles/m 2 )<br />
3.16E-03 9.292E-04 2.340E-03 4.492E-03 4.790E-03<br />
5.62E-03 4.545E-04 1.145E-03 2.198E-03 2.344E-03<br />
1.00E-02 2.223E-04 5.605E-04 1.076E-03 1.147E-03<br />
1.78E-02 1.039E-04 2.621E-04 5.031E-04 5.365E-04<br />
3.16E-02 4.860E-05 1.226E-04 2.353E-04 2.509E-04<br />
5.62E-02 2.273E-05 5.734E-05 1.100E-04 1.173E-04<br />
1.00E-01 1.063E-05 2.682E-05 5.147E-05 5.489E-05<br />
1.78E-01 4.940E-06 1.247E-05 2.393E-05 2.551E-05<br />
3.16E-01 2.296E-06 5.796E-06 1.112E-05 1.186E-05<br />
38