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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 />

where ƒd is the radial component of the relative velocity (positive <strong>for</strong> decreasing range), ν is the<br />

radial component of relative velocity, and λ is the radiated wavelength.<br />

For example, were 95 GHz chosen as the radar carrier frequency, the wavelength would be,<br />

λ = c ÷ ƒ<br />

Equation 4-2<br />

= 3E10 cm/s ÷ 95E9 Hz<br />

˜ 0.3 cm<br />

The Doppler shift resulting from rover plat<strong>for</strong>m motion when the rover is traveling at 2 m/s is<br />

ƒ d (plat<strong>for</strong>m)<br />

= 2(2m/s)(100cm/m) ÷ 0.3 cm<br />

˜ 1.333 kHz<br />

Equation 4-3<br />

A low-pass filter with adequate roll-off below 2 kHz will effectively prevent any plat<strong>for</strong>m<br />

motion from being detected; however, knowing that 1.333 kHz is the offset due to plat<strong>for</strong>m<br />

motion, the rover can apply the cosine of this value to all Doppler returns depending on their<br />

angle relative to the plat<strong>for</strong>m motion. In this way, rover plat<strong>for</strong>m motion can be completely<br />

eliminated from the measurement of the surrounding terrain and Entomopters.<br />

Were the Entomopter to be flying straight and level with one-meter wings (tip-to-tip) flapping at<br />

a frequency of 10 Hz over a 180° angle, the returned 95 GHz carrier frequency would be modulated<br />

at a 10 Hz rate with the frequency excursion of the Doppler signal depending upon the orientation<br />

of the Entomopter to the rover's radar. For example, in the simplest case where the<br />

Entomopter is flying parallel to the rover at the moment the radar scans across it, the received<br />

Doppler (corrected <strong>for</strong> rover plat<strong>for</strong>m motion) would be:<br />

Wing radial advance distance (m) = 2(0.5)sin (45) = 0.35 m<br />

Assuming a linear acceleration, a distance of 0.35 m would be covered in 0.025 seconds, yielding<br />

a radial velocity of 14.142 m/s.<br />

ƒd (45° downbeat) = 2 (14.142m/s)(100cm/m) ÷ 0.3 cm ˜ 9.428 kHz.<br />

ƒd (midflap) = 2 (0m/s)(100cm/m) ÷ 0.3 cm= 0 Hz.<br />

ƒd (135° downbeat)= 2 (-14.142m/s)(100cm/m) ÷ 0.3 cm ˜ -9.428 kHz.<br />

Note that the negative sign on the 135° case is due to the fact that the wing is moving radially<br />

away from the radar, and the Doppler shift will be subtracted from the returned carrier. Since all<br />

parts of the wing are moving at different radial rates from the root to the tip, the Doppler signature<br />

will range from 0 Hz to a maximum of roughly those shown above (assuming that the wing<br />

is accelerating linearly as it flaps).<br />

There<strong>for</strong>e, the demodulated and rectified Doppler return from the Entomopter wing under the<br />

specified flight conditions would be a unique (<strong>for</strong> Mars) frequency modulated (FM) signature<br />

that varies from 0 to roughly 9 kHz every 0.5 seconds. Such a signal would be unambiguously<br />

that of the Entomopter; which Entomopter is being detected is another question, however.<br />

232<br />

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

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