Austin Fikes’s research while affiliated with California Institute of Technology and other places

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Publications (22)


Wireless power transfer in space using flexible, lightweight, coherent arrays
  • Article

November 2024

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41 Reads

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4 Citations

Acta Astronautica

Alex Ayling

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Austin Fikes

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[...]

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Ali Hajimiri

Popup Arrays for Large Space-Borne Apertures

August 2024

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39 Reads

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6 Citations

IEEE Transactions on Antennas and Propagation

Large apertures in space are critical for high-power and high-bandwidth applications spanning wireless power transfer (WPT) and communication, however progress on this front is stunted by the geometric limitations of rocket flight. We present a light and flexible 10GHz array, which is composed of dipole antennas co-cured to a glass-fiber composite. The arrays can dynamically conform to new shapes and are flexible enough to fold completely flat, coil into a rocket payload, and pop back up upon deployment in orbit. The array is amenable to scalable, automated manufacturing - a requirement for the massive production necessary for large apertures. Moreover, the arrays passed the standard gamut of space-qualification testing: the antennas can survive mechanical stress, extreme temperatures, high-frequency temperature cycling, and prolonged stowage in the flattened configuration. The elements exhibit excellent electromagnetic performance: a return ratio better than -10dB over ≈1.5GHz, a single lobe half-power beamwidth of greater than 110° suitable for broad beamforming, >92% efficiency, and excellent manufacturing consistency. Moreover, its mechanical durability vis-a-vis extreme temperatures and protracted stowage lends itself to demanding space applications. This lightweight and scalable array is equipped to serve a host of new space-based radio-frequency technologies and applications which leverage large, stowable and durable array apertures.


Space solar power generation: a viable system proposal and technoeconomic analysis
  • Preprint
  • File available

July 2024

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267 Reads

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1 Citation

This paper presents a distributed space solar power generation and transmission system that converts solar insolation into microwave power and beams it to Earth. This system, composed of a power station of large, close-flying modules residing in Geostationary Orbit, can form dynamically programmable focal points on Earth to provide dispatchable power on demand. Modules are composed of flexible phased array sheets hosting a self-synchronizing network of integrated circuits and antennas which convert DC power from photovoltaic cells into radiated RF energy. The sheets are coiled into a compact payload, launched, and deployed in orbit. Presented herein is a detailed technoeconomic analysis of the proposed system, with investigations into such areas as mass, cost to produce and launch, and a levelized cost of energy (LCOE). This analysis demonstrates that the proposed 10GHz system can generate dispatchable power on the ground at 6.641c/kWh---competitive with the cheapest clean energy sources available today.

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Fig. 1 Caltech's vision for space solar power. Left: operation concept shown in three stages. Right: system hierarchy with relevant details.
Fig. 3 Losses in the SSP system tracked throughout the entire system using the estimated medium-term efficiencies provided in the "middle" column of Table 1. This figure does not include "geometric" losses, which vary during the orbit and are represented by the metric ¯ η geom , which is an average over a full orbit period.
Fig. 4 A. Individual (frequency-dependent) system efficiencies. B. Average end-to-end system efficiency ( ¯ η system ). C. Input power contours. D. Contours for the AC power fed to the grid. E. Total cost contours. F. LCOE contours. G/H/I. Loss contours for α ∈ {0.3, 1.0, 3.0}. J. Power density on the ground contours. K. Optimal power station diameter at each frequency. L. Optimum total cost and LCOE over frequency, assuming ideal power station diameter at each frequency. Plots d-l only display f ≤ 50 GHz because low efficiencies make higher frequencies undesirable.
Cost Projections for a SSP system in GEO that generates 76-164 MW. Sums or important values are labeled in bold.
Space Solar Power Generation: A Viable System Proposal and Technoeconomic Analysis

January 2024

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160 Reads


Popup Arrays for Large Space-Borne Apertures

August 2023

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530 Reads

Large apertures in space are critical for high-power and high-bandwidth applications spanning wireless power transfer (WPT) and communication, however progress on this front is stunted by the geometric limitations of rocket flight. Here, we present a light and flexible 10GHz array, which is composed of dipole antennas co-cured to a glass-fiber composite. The arrays are designed to dynamically conform to new shapes and to be flexible enough to fold completely flat, coil, and pop back up upon deployment. The design was chosen to be amenable to scalable, automated manufacturing - a requirement for the massive production necessary for large apertures. Moreover, the arrays passed the standard gamut of required space-qualification testing: the antennas can survive mechanical stress, extreme temperatures, high-frequency temperature cycling, and prolonged stowage in the flattened configuration. The elements exhibit excellent electromagnetic performance - with a return ratio better than -10dB over a bandwidth of 1.5GHz and a single lobe half-power beam width of greater than 110110^\circ suitable for broad range beamforming and with excellent manufacturing consistency. Moreover, its mechanical durability vis-a-vis extreme temperatures and protracted stowage lends itself to demanding space applications. This lightweight and scalable array is equipped to serve a host of new space-based radio-frequency technologies and applications which leverage large, stowable and durable array apertures.


Fig. 4. Model for the generalized N -path filter.
Fig. 8. (a) Proposed SC-LPF to be used as the filter kernel for the N -path filter. The corresponding continuous-time approximate network is valid under certain conditions, which are met for the implemented filter. By varying the magnitude of the feedback factor, a more desirable response can be obtained. (b) Root locus of the 3rd-order SC-LPF as the K value in the feedback factor is varied, and pole placement for K = 0.4. The dashed lines correspond to 0 < K < 1. (c) Group delay response of the same filter as K is varied. The dashed lines correspond to acceptable variation for GD < 0.1 UI. The filter responses are given for the prototype filter with bandwidth normalized to 1 rad/s.
Fig. 21. (a) Measured single-tone linearity. (b) Measured two-tone linearity.
A 28-GHz, Multi-Beam, Decentralized Relay Array

May 2023

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127 Reads

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6 Citations

IEEE Journal of Solid-State Circuits

Multi-beam relays can be used to overcome the non-line-of-sight (NLOS) issues in millimeter-wave (mm-wave) communication networks that serve many users in an obstruction-rich environment. We demonstrate a modular multi-beam relay array at 28 GHz, which is scalable and fully decentralized. The individual branches of the array are independent and do not need to share a timing reference or be physically located on the same substrate. Multi-beam capability is facilitated by a multi-channel baseband signal conditioning chain that includes a reconfigurable, passive, inductorless, 3rd-order N -path filter with programmable frequency-independent phase shift. This baseband signal conditioning chain enables beams concurrently multiplexed in spatial and frequency domains. We present the theory, design, and operation of the custom RFIC, which enables independent multi-beam relaying. Multiple RFICs are used to create relay arrays. A four-element relay array demonstrates three independently steered beams that utilize the full array aperture with a total wireless throughput of 625 Mb/s.


Fig. 1 Example applications that are enabled by flexible smart antennas. a Lightweight deployable space structures. b Ad-hoc deployable antenna arrays. c Dynamic conformal surfaces. d Wearable conformal surfaces.
Fig. 3 Antenna sheet structure. a This single layer antenna sheet is assembled on the back side of the base-design multi-layer flexible sheet. b Printed antenna patterns and c antenna feed assembly. d Aluminum heat-spreaders. e Power receiver board with an example consumer device (a commercial pulse-oximeter) attached to it.
Fig. 4 Antenna sheet array measurements. a Beam-steering, b deformation correction, c RF-DC wireless power transfer of about 80 mW at 1 m away from the transmitter to a small rectenna array. d Measured output voltage on a 50 Ω resistor, 1 m away from the array (top), angular power density (bottom-left) and expected power delivery distribution to the remote receiver at ~1.6 m away from the array (bottom-right).
Fig. 5 Flexible and robust active antenna design. a Flexible sheets boards with (b) Discrete patch antennas. c The antenna feed via is used for impedance matching. d High voltage (up to 6 V) power delivery strap with local voltage regulator. e Low-profile heat spreaders.
Fig. 6 Flexible array measurements, demonstrating bend radii <23 cm. Figures a-d include pre-and post-focusing 2-D near-field radiation patterns (left), beam-steering of the main lobe (center), and array formation (right). a 2-D beam-steering with flexible array in planar configuration. b 2-D beam-steering with flexible array in convex configuration. c 2-D beam-steering with flexible array in concave configuration. d 2-D beam-steering with flexible array conformed to a doubly curved shape. e Outdoor deployment and focusing to power an LED indicator. The LED is on when the receiver is at the focus point (right) and off when moved away from it (left).
Flexible active antenna arrays

October 2022

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560 Reads

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23 Citations

npj Flexible Electronics

Complex and dynamic control of radiated fields are advantageous for flexible radio systems, which naturally move, roll, bend, twist, deform, and vibrate. Practical challenges hinder the proliferation of these antenna arrays. This work shows how using radio-frequency microchips reduces system component count, decreases mass to ~0.1 g cm ⁻² , and increases functionality and mechanical flexibility. We develop a general platform for large scale flexible arrays and demonstrate two different 256-elements, 30 × 30 cm ² flexible arrays. By varying supply distribution methods and radiators we show how performance can be optimized for maximum power delivery or physical flexibility. The demonstrated systems conform to curved surfaces with radii of curvatures as low as 23 cm and wirelessly deliver ~ 80 mW of DC power to a 6.7 cm × 11 cm-receiver over one meter away. This paves the way towards the integration of smart arrays in flexible wearables and deployable lightweight airborne systems.


The Caltech Space Solar Power Demonstration One Mission

October 2022

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2,692 Reads

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12 Citations

This paper describes Caltech's Space Solar Power Demonstration One (SSPD-1) payload and upcoming mission on Momentus Space Vigoride 5. SSPD-1 is comprised of three experiments each of which demonstrates the performance of a key technology piece in the space environment. We describe the goals of SSPD-1. The three experiments-Alba, DOLCE and MAPLE are discussed. The launch of SSPD-1 is scheduled for November 6, 2022 on Space X's Transporter 6 mission.



A lightweight space-based solar power generation and transmission satellite

June 2022

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444 Reads

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14 Citations

We propose a novel design for a lightweight, high-performance space-based solar power array combined with power beaming capability for operation in geosynchronous orbit and transmission of power to Earth. We use a modular configuration of small, repeatable unit cells, called tiles, that each individually perform power collection, conversion, and transmission. Sunlight is collected via lightweight parabolic concentrators and converted to DC electric power with high efficiency III-V photovoltaics. Several CMOS integrated circuits within each tile generates and controls the phase of multiple independently-controlled microwave sources using the DC power. These sources are coupled to multiple radiating antennas which act as elements of a large phased array to beam the RF power to Earth. The power is sent to Earth at a frequency chosen in the range of 1-10 GHz and collected with ground-based rectennas at a local intensity no larger than ambient sunlight. We achieve significantly reduced mass compared to previous designs by taking advantage of solar concentration, current CMOS integrated circuit technology, and ultralight structural elements. Of note, the resulting satellite has no movable parts once it is fully deployed and all beam steering is done electronically. Our design is safe, scalable, and able to be deployed and tested with progressively larger configurations starting with a single unit cell that could fit on a cube satellite. The design reported on here has an areal mass density of 160 g/m2 and an end-to-end efficiency of 7-14%. We believe this is a significant step forward to the realization of space-based solar power, a concept once of science fiction.


Citations (19)


... The concept of wireless power transfer (WPT) can be traced back to the groundbreaking work of Nicola Tesla in the late 19th century [1]. Over the past two decades, numerous WPT platforms have been proposed, including microwaves [2,3], acoustics [4,5], and non-radiative methods [6][7][8][9]. Among these platforms, near-field magnetic resonant coupling WPT has gained significant attention due to its high efficiency, power capacity, and flexibility [6]. ...

Reference:

Dispersive gains enhance wireless power transfer with asymmetric resonance
Wireless power transfer in space using flexible, lightweight, coherent arrays
  • Citing Article
  • November 2024

Acta Astronautica

... The space solar power concept, first proposed by Isaac Asimov in his short story, "Reason" [21], envisions a solar power station in orbit around the Earth, unaffected by day/night cycles or inclement weather and having nearly 24/7 access to sunlight year-round. Caltech's proposed implementation consists of a planar, sheet-like power station coated with flexible photovoltaics that uses a microwave phased array to beam the collected power to Earth [22]. Because the microwave regime is minimally effected by the atmosphere 1 the power station can efficiently beam power regardless of weather conditions, providing clean solar power 1 While atmospheric attenuation is very low at microwave frequencies, the effect of the atmosphere is further minimized since the beam travels vertically through the atmosphere. ...

Space solar power generation: a viable system proposal and technoeconomic analysis

... If the number of radiators in an array is fixed, the spacing between them must change as the array shifts between planar and spherical shapes. Thus, arrays of rigid tiles can only change shape if gaps are introduced between the tiles or tiles are removed from the surface [3]. ...

Frontiers in Flexible and Shape-Changing Arrays

... These include systems operating on both Earth [1], [2], [3], [4], [5], [6] and in space [7], [8]. Space solar power [7], [8], [9], [10], [11], [12], [13], [14], [15], [16], [17], [18], [19], [20] is promising as an alternative source of clean energy that can help address the growing challenges caused by climate change. The space solar power concept, first proposed by Isaac Asimov in his short story, "Reason" [21], envisions a solar power station in orbit around the Earth, unaffected by day/night cycles or inclement weather and having nearly 24/7 access to sunlight year-round. ...

A lightweight space-based solar power generation and transmission satellite

... In MIMO systems, MAs optimize performance not only by adjusting the positions of individual antennas at the singleelement level but also by moving each antenna within the array at the array level. The emergence of flexible substrates has enabled the deformation of array structures, leading to the development of flexible antenna arrays that allow for the movement of array antennas [30]- [34]. The evolution of MAs from single-element to array-level systems represents a significant advancement in wireless communication technology. ...

Flexible active antenna arrays

npj Flexible Electronics

... Space is an increasingly ripe realm for RF applications including space solar power [1], [2], [3], [4], [5], [6], [7], communications [8], [9], [10], and the traditional remote sensing applications [11], [12]. These applications demand high bandwidth and/or high power efficiency but are currently limited by the aperture size that can be deployed [13]; large apertures in space are challenging because of the crucial requirement that they fit within the fairing of the launch vehicle. ...

The Caltech Space Solar Power Project: Design, Progress, and Future Direction

... Both concepts aim to converge solar rays with huge collectors and transfer then the energy back to Earth. The first real mission demonstrating the transfer of energy to the planet is the Caltech experiment: the Space Solar Power Demonstrator (SSPD-1) 4 launched in January 2023. A different concept instead is the constellation of LEO reflectors, conceived by ESA and Thales Alenia Space (SOLARIS project): SBSP (Space-Based Solar Power) 5 . ...

The Caltech Space Solar Power Demonstration One Mission

... in center frequency and bandwidth. This work substantially expands the treatment offered in [15] in several areas: explanation of the theory of operation for the multi-beam enabling baseband circuitry; full circuit details and simulation results of the receive path, baseband, transmit path, and on-chip reference distribution of the IC; and additional measurements results. ...

Multi-beam, Scalable 28 GHz Relay Array with Frequency and Spatial Division Multiple Access Using Passive, High-Order N-Path Filters
  • Citing Conference Paper
  • June 2022