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Phase II Final Report - NASA's Institute for Advanced Concepts

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Planetary Exploration Using Biomimetics<br />

An Entomopter <strong>for</strong> Flight on Mars<br />

Table 4-2: Parameters <strong>for</strong> Altimetry Analysis (Continued)<br />

Signal-to-noise ratio (dB) 10<br />

Interpulse period, T (ms) 1<br />

Pulse repetition frequency, (kpps) 1<br />

Following the analysis procedure outlined above, the required peak and average transmitter<br />

powers are shown in Figure 4-18 <strong>for</strong> an operating frequency of 18 GHz. The peak and average<br />

powers <strong>for</strong> a 10-m altitude are 3.9 µW and 1.6 pW, respectively. The peak and average powers<br />

<strong>for</strong> a 200-m altitude are 630 mW and 252 nW, respectively. Note: The required peak power has<br />

increased significantly compared to the obstacle-detection results due to the increased range resolution.<br />

The required peak and average powers are plotted as a function of operating frequency<br />

in Figures 4-19 and 4-20, respectively. These plots show that by decreasing the range resolution,<br />

and thus decreasing the pulse width (see Equation 4-16), the frequency dependence is altered<br />

compared to the obstacle-detection results. These plots also show that a reduction in required<br />

power can be achieved by operating below about 2 GHz. However, using the chosen pulsewidth,<br />

physically realizable operating frequencies are limited to values greater than 1.25 GHz to maintain<br />

a bandwidth greater than twice the operating frequency.<br />

0.1 1 0.01<br />

1.10 3<br />

1.10 4<br />

1.10<br />

1.10 6<br />

5<br />

1.10 7<br />

1.10<br />

1.10 9<br />

8<br />

1.10 10<br />

1.10 11<br />

1.10<br />

1.10 13<br />

12<br />

1.10 14<br />

0 50 100 150 200<br />

Range (m)<br />

Peak<br />

Average<br />

Figure 4-18: Peak and Average Transmitter Power Required <strong>for</strong> Altimetry at 18 GHz<br />

as a function of Altitude<br />

Power (W)<br />

Peak and average powers at 18 GHz<br />

<strong>Phase</strong> <strong>II</strong> <strong>Final</strong> <strong>Report</strong><br />

254

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