Phillip Walkemeyer
Jet Propulsion Laboratory
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Publication
Featured researches published by Phillip Walkemeyer.
Journal of Mechanical Design | 2013
Shannon A. Zirbel; Robert J. Lang; Mark Thomson; Deborah A. Sigel; Phillip Walkemeyer; Brian P. Trease; Spencer P. Magleby; Larry L. Howell
The purpose of this work is to create deployment systems with a large ratio of stowed-to-deployed diameter. Deployment from a compact form to a final flat state can be achieved through origami-inspired folding of panels. There are many models capable of this motion when folded in a material with negligible thickness; however, when the application requires the folding of thick, rigid panels, attention must be paid to the effect of material thickness not only on the final folded state, but also during the folding motion (i.e., the panels must not be required to flex to attain the final folded form). The objective is to develop new methods for deployment from a compact folded form to a large circular array (or other final form). This paper describes a mathematical model for modifying the pattern to accommodate material thickness in the context of the design, modeling, and testing of a deployable system inspired by an origami six-sided flasher model. The model is demonstrated in hardware as a 1/20th scale prototype of a deployable solar array for space applications. The resulting prototype has a ratio of stowed-to-deployed diameter of 9.2 (or 1.25 m deployed outer diameter to 0.136 m stowed outer diameter). INTRODUCTION The purpose of this work is to develop deployment systems that unfold from a compact form to a large array. This work ∗Corresponding author: [email protected] is motivated by the need for compactly folded solar arrays for space applications. A large ratio of stowed-to-deployed diameter enables large solar arrays to be launched in their compact, folded configuration and then deployed in space to a much larger surface area. For our objectives, a design with synchronous deployment was desired to simplify actuation and deployment. Deployment from a compact form to a final flat state can be achieved through origami-inspired folding of panels. There are many models capable of this motion when folded in paper or other materials with negligible thickness; however, when the application requires the folding of thick, rigid panels, material thickness can inhibit the folding motion. To be rigid-foldable, the panels must not be required to flex to attain the final folded form. This paper describes the approach for modifying the design of an origami six-sided flasher model to accommodate material thickness. This work builds on existing models to present a unique design that is rigid-foldable through two different methods. In the first method, the panels are allowed to flex along their diagonals. In the second method, the panels are affixed to a flexible membrane with discrete gap spacing between the panels. Both folding solutions enable the model to be rigid-foldable.
Archive | 2014
W. Keats Wilkie; Jerry E. Warren; Lucas G. Horta; Karen H. Lyle; Jer-Nan Juang; Justin D. Littell; Robert G. Bryant; Mark Thomson; Phillip Walkemeyer; Daniel V. Guerrant; Dale A. Lawrence; S. Chad Gibbs; Earl H. Dowell; Andrew F. Heaton
The recent successful flight of the JAXA IKAROS solar sail has renewed interest within NASA in spinning solar sail concepts for high-performance solar sailing. The heliogyro solar sail, in particular, is being re-examined as a potential game-changing architecture for future solar sailing missions. In this paper, we present an overview of ongoing heliogyro technology development and feasibility assessment activities within NASA. In particular, a small-scale heliogyro solar sail technology demonstration concept will be described. We will also discuss ongoing analytical and experimental heliogyro structural dynamics and controls investigations and provide an outline of future heliogyro development work directed toward enabling a low-cost heliogyro technology demonstration mission ca. 2020.
Sensors | 2015
Hyeong Jae Lee; Stewart Sherrit; Luis Phillipe Tosi; Phillip Walkemeyer; Tim Colonius
We consider piezoelectric flow energy harvesting in an internal flow environment with the ultimate goal powering systems such as sensors in deep oil well applications. Fluid motion is coupled to structural vibration via a cantilever beam placed in a converging-diverging flow channel. Two designs were considered for the electromechanical coupling: first; the cantilever itself is a piezoelectric bimorph; second; the cantilever is mounted on a pair of flextensional actuators. We experimentally investigated varying the geometry of the flow passage and the flow rate. Experimental results revealed that the power generated from both designs was similar; producing as much as 20 mW at a flow rate of 20 L/min. The bimorph designs were prone to failure at the extremes of flow rates tested. Finite element analysis (FEA) showed fatigue failure was imminent due to stress concentrations near the bimorph’s clamped region; and that robustness could be improved with a stepped-joint mounting design. A similar FEA model showed the flextensional-based harvester had a resonant frequency of around 375 Hz and an electromechanical coupling of 0.23 between the cantilever and flextensional actuators in a vacuum. These values; along with the power levels demonstrated; are significant steps toward building a system design that can eventually deliver power in the Watts range to devices down within a well.
ieee aerospace conference | 2012
Kerry Klein; Mircea Badescu; Nicolas Haddad; Lori Shiraishi; Phillip Walkemeyer
A low mass Sample Acquisition Tool (SAT) has been developed that can be used autonomously to percussively core, fracture, and capture rock cores. The tool was developed as part of the Integrated Mars Sample Acquisition and Handling (IMSAH) architecture allowing for end to end sample capture and caching as it relates to the proposed Mars Sample Return (MSR) campaign. The key element of the tool design, as it pertains to the IMSAH architecture, is the ability to drill and capture rock cores directly into a sample tube. In doing so, the sample tube becomes the handling element within the IMSAH sample handling chain significantly reducing the possibility of sample contamination and uncertainty related to handling a sample of unknown geometry. In order to validate the tools unit level functionality a series of verification and validation tests have been performed utilizing a rock test suite that encompasses a variety of rock types that are analogous to Martian rocks and have been used in the past to qualify Martian surface sampling hardware. The results of the testing have shown the tool can successfully generate, fracture, and capture rock cores within a sample tube for all of the rocks within the proposed test suite. Additionally, the tool does so while maintaining torque margins of no less than 50% for all mechanisms with an average power consumption of no greater than 90W and a tool mass of less than 6kg.
Proceedings of SPIE | 2014
Stewart Sherrit; Phillip Walkemeyer; Jeffrey L. Hall; Hyeong Jae Lee; Tim Colonius; Phillipe Tosi; Namhyo Kim; Kai Sun; Thomas Gary Corbett; Alvaro Jose Arrazola
There is a need for a long-life power generation scheme that could be used downhole in an oil well to produce 1 Watt average power. There are a variety of existing or proposed energy harvesting schemes that could be used in this environment but each of these has its own limitations. The vibrating piezoelectric structure is in principle capable of operating for very long lifetimes (decades) thereby possibly overcoming a principle limitation of existing technology based on rotating turbo-machinery. In order to determine the feasibility of using piezoelectrics to produce suitable flow energy harvesting, we surveyed experimentally a variety of nozzle configurations that could be used to excite a vibrating piezoelectric structure in such a way as to enable conversion of flow energy into useful amounts of electrical power. These included reed structures, spring mass-structures, drag and lift bluff bodies and a variety of nozzles with varying flow profiles. Although not an exhaustive survey we identified a spline nozzle/piezoelectric bimorph system that experimentally produced up to 3.4 mW per bimorph. This paper will discuss these results and present our initial analyses of the device using dimensional analysis and constitutive electromechanical modeling. The analysis suggests that an order-of-magnitude improvement in power generation from the current design is possible.
AIAA SPACE 2014 Conference and Exposition | 2014
Paul G. Backes; Christopher McQuin; Mircea Badescu; Anthony Ganino; Nicholas Wiltsie; Scott Moreland; Phillip Walkemeyer; Charles M. Dandino; Roger Smith; Michael Williamson; Dennis Wai; Robert G. Bonitz; Alejandro San Martin; Brian H. Wilcox
Paul Backes, 1 Christopher McQuin, Mircea Badescu, Anthony Ganino, Harish Manohara, Youngsam Bae, Risaku Toda, Nicholas Wiltsie, Scott Moreland, Jesse Grimes-York, Phillip Walkemeyer, Eric Kulczycki, Charles Dandino, Russell Smith, Michael Williamson, Dennis Wai, Robert Bonitz, Alejandro San Martin, and Brian Wilcox Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, 91109
ieee aerospace conference | 2013
Mircea Badescu; Robert Bonitz; Anthony Ganino; Nicolas Haddad; Phillip Walkemeyer; Paul G. Backes; Lori Shiraishi; Erick Kulczycki; Norman Aisen; Charles M. Dandino; Brett S. Cantrell; William Gallagher; Jesse Shevin
The 2011 Decadal Survey for planetary science released by the National Research Council of the National Academies identified Comet Surface Sample Return (CSSR) as one of five high priority potential New Frontiers-class missions in the next decade. The main objectives of the research described in this publication are: develop a concept for an end-to-end system for collecting and storing a comet sample to be returned to Earth; design, fabricate and test a prototype Dynamic Acquisition and Retrieval Tool (DART) capable of collecting 500 cc sample in a canister and ejecting the canister with a predetermined speed; identify a set of simulants with physical properties at room temperature that suitably match the physical properties of the comet surface as it would be sampled. We propose the use of a DART that would be launched from the spacecraft to impact and penetrate the comet surface. After collecting the sample, the sample canister would be ejected at a speed greater than the comets escape velocity and captured by the spacecraft, packaged into a return capsule and returned to Earth. The DART would be composed of an inner tube or sample canister, an outer tube, a decelerator, a means of capturing and retaining the sample, and a mechanism to eject the canister with the sample for later rendezvous with the spacecraft. One of the significant unknowns is the physical properties of the comet surface. Based on new findings from the recent Deep Impact comet encounter mission, we have limited our search of solutions for sampling materials to materials with 10 to 100 kPa shear strength in loose or consolidated form. As the possible range of values for the comet surface temperature is also significantly different than room temperature and testing at conditions other than the room temperature can become resource intensive, we sought sample simulants with physical properties at room temperature similar to the expected physical properties of the comet surface material. The chosen DART configuration, the efforts to identify a test simulant and the properties of these simulants, and the results of the preliminary testing will be described in this paper.
international geoscience and remote sensing symposium | 2016
Shannon T. Brown; Paolo Focardi; Amarit Kitiyakara; Frank Maiwald; Lance Milligan; Oliver Montes; Sharmila Padmanabhan; Richard Redick; Damon Russel; Vin Bach; Phillip Walkemeyer
The Compact Ocean Wind Vector Radiometer (COWVR) is new type of conical sensor ideal for small satellite implementation. This paper provides an overview of the COWVR sensor, mission and provides perspectives for the future of this technology to enable low-cost sustainable passive microwave observations into the next decade.
Proceedings of SPIE | 2015
Stewart Sherrit; Hyeong Jae Lee; Phillip Walkemeyer; Tyler Winn; Luis Phillipe Tosi; Tim Colonius
Power generation schemes that could be used downhole in an oil well to produce about 1 Watt average power with long-life (decades) are actively being developed. A variety of proposed energy harvesting schemes could be used to extract energy from this environment but each of these has their own limitations that limit their practical use. Since vibrating piezoelectric structures are solid state and can be driven below their fatigue limit, harvesters based on these structures are capable of operating for very long lifetimes (decades); thereby, possibly overcoming a principle limitation of existing technology based on rotating turbo-machinery. An initial survey [1] identified that spline nozzle configurations can be used to excite a vibrating piezoelectric structure in such a way as to convert the abundant flow energy into useful amounts of electrical power. This paper presents current flow energy harvesting designs and experimental results of specific spline nozzle/ bimorph design configurations which have generated suitable power per nozzle at or above well production analogous flow rates. Theoretical models for non-dimensional analysis and constitutive electromechanical model are also presented in this paper to optimize the flow harvesting system.
Proceedings of SPIE | 2011
N. J. Kasdin; David N. Spergel; Robert J. Vanderbei; Douglas Lisman; Stuart B. Shaklan; Mark Thomson; Phillip Walkemeyer; V. Bach; E. Oakes; Eric Cady; Stefan Martin; Luis Marchen; Bruce A. Macintosh; R. E. Rudd; J. Mikula; D. Lynch
External occulters provide the starlight suppression needed for detecting and characterizing exoplanets with a much simpler telescope and instrument than is required for the equivalent performing coronagraph. In this paper we describe progress on our Technology Development for Exoplanet Missions project to design, manufacture, and measure a prototype occulter petal. We focus on the key requirement of manufacturing a precision petal while controlling its shape within precise tolerances. The required tolerances are established by modeling the effect that various mechanical and thermal errors have on scatter in the telescope image plane and by suballocating the allowable contrast degradation between these error sources. We discuss the deployable starshade design, representative error budget, thermal analysis, and prototype manufacturing. We also present our metrology system and methodology for verifying that the petal shape meets the contrast requirement. Finally, we summarize the progress to date building the prototype petal.