Abstract
An origami-based foldable and reconfigurable Reflectarray Antenna (RA) with multiple apertures is proposed for CubeSat applications. The proposed configuration consists of a central RA embedded in folding panels using Lamina Emergent Torsional (LET) joints based on compliant mechanisms. Depending on the folding direction of these panels (forward or backward), a new RA aperture is formed. The proposed RA along with its folding panels and hinges is fabricated using only a single PCB. A prototype of such an RA with two foldable panels is fabricated and measured. This RA operates in the Ku-band at 16 GHz and provides two pencil beams pointing at ( $\theta = 30^{\circ }$ , $\varphi = 0^{\circ }$ ) and ( $\theta = -30^{\circ }$ , $\varphi = 0^{\circ }$ ), and a dual-beam pointing at ( $\theta = +27^{\circ }$ , $\varphi = 0^{\circ }$ ) and ( $\theta = -29^{\circ }$ , $\varphi = 0^{\circ }$ ). The proposed RA provides a gain of 25 dB and 19 dB in its single- and dual-beam operations, respectively. For CubeSat applications, the key advantages of this RA are its small stowed volume, reconfigurable EM performance, beamsteering capabilities, monolithic construction, low fabrication cost, and reduced complexity.
Highlights
CUBESAT missions for low-earth orbit have seen significant growth over the last decade offering new opportunities to expand space exploration
In order to better understand the work proposed in this paper, we review previous foldable reflectarray designs, and surrogate hinges
Other constraints imposed were that the width, W, of the Lamina Emergent Torsional (LET) array had to be equal to the width of the panels, warray, and that the LET array length, L, needed to be less than or equal to a specified length, l, see Fig. 6
Summary
Abdul-Sattar Kaddour1, Member, IEEE, Carlos A. Velez1, Student Member, IEEE, Muhammad Hamza1, Student Member, IEEE, Nathan Brown2, Collin Ynchausti2, Spencer Magleby2, Larry L. Howell2, and Stavros V. Georgakopoulos1, Senior Member, IEEE This research was supported by the Air Force Office of Scientific Research under grants FA9550-18-1-0191 and FA9550-19-1-0290.
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