Larry Hess
Goddard Space Flight Center
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Featured researches published by Larry Hess.
Proceedings of SPIE | 2007
Mary Li; T. Adachi; Christine A. Allen; Sachidananda R. Babu; Sateesh Bajikar; Michael Beamesderfer; Ruth Bradley; Nick Costen; Kevin L. Denis; Audrey J. Ewin; David Franz; Larry Hess; Ron Hu; Kamili M. Jackson; Murzy D. Jhabvala; Dan Kelly; Todd King; Gunther Kletetschka; Alexander S. Kutyrev; Bernard A. Lynch; Stephen E. Meyer; Timothy M. Miller; S. H. Moseley; Vilem Mikula; Brent Mott; Lance Oh; James Pontius; David A. Rapchun; Chris Ray; Scott Schwinger
We have developed microshutter array systems at NASA Goddard Space Flight Center for use as multi-object aperture arrays for a Near-Infrared Spectrometer (NIRSpec) instrument. The instrument will be carried on the James Webb Space Telescope (JWST), the next generation of space telescope, after the Hubble Space Telescope retires. The microshutter arrays (MSAs) are designed for the selective transmission of light from objected galaxies in space with high efficiency and high contrast. Arrays are close-packed silicon nitride membranes with a pixel size close to 100x200 μm. Individual shutters are patterned with a torsion flexure permitting shutters to open 90 degrees with minimized stress concentration. In order to enhance optical contrast, light shields are made on each shutter to prevent light leak. Shutters are actuated magnetically, latched and addressed electrostatically. The shutter arrays are fabricated using MEMS bulk-micromachining and packaged utilizing a novel single-sided indium flip-chip bonding technology. The MSA flight system consists of a mosaic of 2 x 2 format of four fully addressable 365 x 171 arrays. The system will be placed in the JWST optical path at the focal plane of NIRSpec detectors. MSAs that we fabricated passed a series of qualification tests for flight capabilities. We are in the process of making final flight-qualified MSA systems for the JWST mission.
Proceedings of SPIE | 2009
Stephanie A. Getty; Mary Li; Larry Hess; Nick Costen; Todd King; Patrick A. Roman; William B. Brinckerhoff; Paul R. Mahaffy
A carbon nanotube (CNT) field emission electron gun has been fabricated and assembled as an electron impact ionization source for a miniaturized time-of-flight mass spectrometer (TOF-MS). The cathode consists of a patterned array of CNT towers grown by catalyst-assisted thermal chemical vapor deposition. An extraction grid is precisely integrated in close proximity to the emitter tips (20-35 μm spacing), and an anode is located at the output to monitor the ionization beam current. Ultra-clean MEMS integration techniques were employed in an effort to achieve three improvements, relative to previous embodiments: reduced extraction voltage during operation to be resonant with gas ionization energies, enhanced current transmission through the grid, and a greater understanding of the fundamental current fluctuations due to adsorbate-assisted tunneling. Performance of the CNT electron gun will be reported, and implications for in situ mass spectrometry in planetary science will be discussed.
Proceedings of SPIE, the International Society for Optical Engineering | 2007
Mary J. Li; Tomoko Adachi; Christine A. Allen; Sachi Babu; Sateesh Bajikar; Michael Beamesderfer; Ruth Bradley; Kevin L. Denis; Nick Costen; Audrey J. Ewin; Dave Franz; Larry Hess; Ron Hu; Kamili M. Jackson; Murzy D. Jhabvala; Dan Kelly; Todd King; Gunther Kletetschka; Alexander S. Kutyrev; Barney Lynch; Timothy M. Miller; Harvey Moseley; Vilem Mikula; Brent Mott; Lance Oh; James Pontius; Dave Rapchun; Chris Ray; Knute Ray; Eric Schulte
A complex MEMS device, microshutter array system, is being developed at NASA Goddard Space Flight Center for use as an aperture array for a Near-Infrared Spectrometer (NirSpec). The instrument will be carried on the James Webb Space Telescope (JWST), the next generation of space telescope after Hubble Space Telescope retires. The microshutter arrays (MSAs) are designed for the selective transmission of light with high efficiency and high contrast. Arrays are close-packed silicon nitride membranes with a pixel size close to 100x200 &mgr;m. Individual shutters are patterned with a torsion flexure permitting shutters to open 90 degrees with a minimized mechanical stress concentration. Light shields are made on to each shutter for light leak prevention so to enhance optical contrast. Shutters are actuated magnetically, latched and addressed electrostatically. The shutter arrays are fabricated using MEMS bulk-micromachining technologies and packaged using single-sided indium flip-chip bonding technology. The MSA flight concept consists of a mosaic of 2 x 2 format of four fully addressable 365 x 171 arrays placed in the JWST optical path at the focal plane.
Micro- and Nanotechnology: Materials, Processes, Packaging, and Systems III | 2006
Mary J. Li; Tomoko Adachi; Christine A. Allen; Sachi Babu; Sateesh Bajikar; Michael Beamesderfer; Ruth Bradley; Kevin L. Denis; Nick Costen; Audrey J. Ewin; David Franz; Larry Hess; Ron Hu; Kamili M. Jackson; Murzy D. Jhabvala; Dan Kelly; Todd King; Gunther Kletetschka; Alexander S. Kutyrev; Barney Lynch; Timothy M. Miller; Harvey Moseley; Vilem Mikula; Brent Mott; Lance Oh; James Pontius; David A. Rapchun; Chris Ray; Eric Schulte; Scott Schwinger
MEMS microshutter arrays (MSAs) are being developed at NASA Goddard Space Flight Center for use as an aperture array for the Near-Infrared Spectrometer (NirSpec). The instruments will be carried on the James Webb Space Telescope (JWST), the next generation of space telescope after Hubble Space Telescope retires. The microshutter arrays are designed for the selective transmission of light with high efficiency and high contrast. Arrays are close-packed silicon nitride membranes with a pixel size of 105x204 μm. Individual shutters are patterned with a torsion flexure permitting shutters to open 90 degrees with a minimized mechanical stress concentration. Light shields are made on each shutter for light leak prevention to enhance optical contrast. Shutters are actuated magnetically, latched and addressed electrostatically. The shutter arrays are fabricated using MEMS technologies. Single-side indium flip chip bonding is performed to attach microshutter arrays to substrates.
Proceedings of SPIE | 2005
Daniel P. Kelly; Wen-Hsien Chuang; Larry Hess; Ron Hu; Murzy D. Jhabvala; Todd King; Mary J. Li; James Loughlin; S. Harvey Moseley; Chris Ray; Yun Zheng
We report on methods to minimize thermally-induced deformation in a MEMS-based reconfigurable aperture. The device is an enabling component of the Near-Infrared Spectrometer, a principle instrument on NASA’s James Webb Space Telescope. The Microshutter Array consists of 384x175 individually addressable shutters which can be magnetically rotated 90° into the plane of the array and electrostatically latched open. Each shutter is a 100x200 μm rectangular membrane suspended by a small neck region and torsion flexure. The primary materials in the shutter are a 5000Å Si3N4 layer for mechanical rigidity, 2000Å Al for opacity and electrostatic latching, and 2200Å Co90Fe10 for magnetic actuation. This multi-layer stack presents a challenge due to the operating temperatures required for the device: both room temperature (300K) and cryogenic temperature (30K). Thermal expansion of the materials causes the shutters to bow out of plane excessively, which can prevent actuation of the shutters, cause damage to portions of the array, and allow light leakage around closed shutters. Here we present our investigation of several methods to prevent microshutter bowing including deposition of additional materials on the shutters to create a symmetrical layer stack and replacing the current stack with low-coefficient of thermal expansion materials. Using shutter-size suspended cantilever beams as a rapid-development test bed, we have reduced out-of-plane bowing between 300K and 30K to 10% or better. We are currently applying these results to microshutter arrays to develop shutters that remain flat from room temperature to cryogenic temperature while retaining the required mechanical, optical, and magnetic properties.
Storage and Retrieval for Image and Video Databases | 2005
Mary J. Li; Nadine Acuna; Edward Amatucci; Michael Beamesderfer; Ray Boucarut; Sachi Babu; Sateesh Bajikar; Audrey J. Ewin; Rainer K. Fettig; David Franz; Larry Hess; Ron Hu; Murzy D. Jhabvala; Dan Kelly; Gunther Kletetschka; Carl Kotechi; Alexander S. Kutyrev; James Loughlin; Bernard A. Lynch; Harvey Moseley; Brent Mott; William F. Newell; Lance Oh; David A. Rapchun; Chris Ray; Carol Sappington; Eric Schulte; Scott Schwinger; Wayne Smith; Stephen Snodgrass
Archive | 2006
Denis Kevin; Edward Amatucci; Michael Beamesderfer; Sateesh Bajikar; Audrey J. Ewin; Rainer K. Fettig; Dave Franz; Larry Hess; Murzy D. Jhabvala; Dan Kelly; Todd King; Gunther Kletetschkar; Alexander S. Kutyrev; Mary J. Li; Jim Loughlin; Harvey Moseley; Lance Oh; Chris Ray; Eric Schulte; Wayne Smith; Steve Snodgrass; Veronica Valeriano; Yun Zheng; Chris Zincke
Archive | 2013
Murzy D. Jhabvala; K. Choi; Dan Kelly; Larry Hess; Audrey J. Ewin; A. La; A. Wacynski; J. Sun; T. Adachi; Nick Costen; Q. Ni; Stephen Snodgrass; Roger Foltz
Archive | 2012
Murzy D. Jhabvala; Audrey J. Ewin; Larry Hess; Thomas M. Hartmann; Anh T. La
Archive | 2009
Stephanie A. Getty; Mary Li; Nick Costen; Larry Hess; Steve Feng; Todd King; William B. Brinckerhoff; P. Mahaffy; Daniel P. Glavin