Terahertz Integrated Electronic and Hybrid Electronic–Photonic Systems
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EPA Handbook: Optical and Remote Sensing for Measurement and Monitoring of Emissions Flux of Gases and Particulate Matter
EPA Handbook: Optical and Remote Sensing for Measurement and Monitoring of Emissions Flux of Gases and Particulate Matter EPA 454/B-18-008 August 2018 EPA Handbook: Optical and Remote Sensing for Measurement and Monitoring of Emissions Flux of Gases and Particulate Matter U.S. Environmental Protection Agency Office of Air Quality Planning and Standards Air Quality Assessment Division Research Triangle Park, NC EPA Handbook: Optical and Remote Sensing for Measurement and Monitoring of Emissions Flux of Gases and Particulate Matter 9/1/2018 Informational Document This informational document describes the emerging technologies that can measure and/or identify pollutants using state of the science techniques Forward Optical Remote Sensing (ORS) technologies have been available since the late 1980s. In the early days of this technology, there were many who saw the potential of these new instruments for environmental measurements and how this technology could be integrated into emissions and ambient air monitoring for the measurement of flux. However, the monitoring community did not embrace ORS as quickly as anticipated. Several factors contributing to delayed ORS use were: • Cost: The cost of these instruments made it prohibitive to purchase, operate and maintain. • Utility: Since these instruments were perceived as “black boxes.” Many instrument specialists were wary of how they worked and how the instruments generated the values. • Ease of use: Many of the early instruments required a well-trained spectroscopist who would have to spend a large amount of time to setup, operate, collect, validate and verify the data. • Data Utilization: Results from path integrated units were different from point source data which presented challenges for data use and interpretation. -
The Near-Infrared Multi-Band Ultraprecise Spectroimager for SOFIA
NIMBUS: The Near-Infrared Multi-Band Ultraprecise Spectroimager for SOFIA Michael W. McElwaina, Avi Mandella, Bruce Woodgatea, David S. Spiegelb, Nikku Madhusudhanc, Edward Amatuccia, Cullen Blaked, Jason Budinoffa, Adam Burgassere, Adam Burrowsd, Mark Clampina, Charlie Conroyf, L. Drake Demingg, Edward Dunhamh, Roger Foltza, Qian Gonga, Heather Knutsoni, Theodore Muencha, Ruth Murray-Clayf, Hume Peabodya, Bernard Rauschera, Stephen A. Rineharta, Geronimo Villanuevaj aNASA Goddard Space Flight Center, Greenbelt, MD, USA; bInstitute for Advanced Study, Princeton, NJ, USA; cYale University, New Haven, CT, USA; dPrinceton University, Princeton, NJ, USA; eUniversity of California, San Diego, La Jolla, CA, USA; fHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA; gUniversity of Maryland, College Park, MD, USA; hLowell Observatory, Flagstaff, AZ, USA; iCalifornia Institute of Technology, Pasadena, CA; jCatholic University of America, Washington, DC, USA. ABSTRACT We present a new and innovative near-infrared multi-band ultraprecise spectroimager (NIMBUS) for SOFIA. This design is capable of characterizing a large sample of extrasolar planet atmospheres by measuring elemental and molecular abundances during primary transit and occultation. This wide-field spectroimager would also provide new insights into Trans-Neptunian Objects (TNO), Solar System occultations, brown dwarf atmospheres, carbon chemistry in globular clusters, chemical gradients in nearby galaxies, and galaxy photometric redshifts. NIMBUS would be the premier ultraprecise -
All-Metal Terahertz Metamaterial Absorber and Refractive Index Sensing Performance
hv photonics Communication All-Metal Terahertz Metamaterial Absorber and Refractive Index Sensing Performance Jing Yu, Tingting Lang * and Huateng Chen Institute of Optoelectronic Technology, China Jiliang University, Hangzhou 310018, China; [email protected] (J.Y.); [email protected] (H.C.) * Correspondence: [email protected] Abstract: This paper presents a terahertz (THz) metamaterial absorber made of stainless steel. We found that the absorption rate of electromagnetic waves reached 99.95% at 1.563 THz. Later, we ana- lyzed the effect of structural parameter changes on absorption. Finally, we explored the application of the absorber in refractive index sensing. We numerically demonstrated that when the refractive index (n) is changing from 1 to 1.05, our absorber can yield a sensitivity of 74.18 µm/refractive index unit (RIU), and the quality factor (Q-factor) of this sensor is 36.35. Compared with metal–dielectric–metal sandwiched structure, the absorber designed in this paper is made of stainless steel materials with no sandwiched structure, which greatly simplifies the manufacturing process and reduces costs. Keywords: metamaterial absorber; stainless steel; refractive index sensing; sensitivity 1. Introduction Metamaterials are new artificial materials that are periodically arranged according to certain subwavelength dimensions [1,2]. Owing to their unique properties of perfect absorption, perfect transmission, and stealth, metamaterials show promising applications Citation: Yu, J.; Lang, T.; Chen, H. in sensors [3–11], absorbers [12,13], imaging [14,15], etc. Among them, in biomolecular All-Metal Terahertz Metamaterial sensing, metamaterial devices are spurring unprecedented interest as a diagnostic protocol Absorber and Refractive Index for cancer and infectious diseases [10,11]. -
Hyperspectral Imaging for Predicting the Internal Quality of Kiwifruits
www.nature.com/scientificreports OPEN Hyperspectral Imaging for Predicting the Internal Quality of Kiwifruits Based on Variable Received: 18 April 2016 Accepted: 11 July 2017 Selection Algorithms and Published: xx xx xxxx Chemometric Models Hongyan Zhu1, Bingquan Chu1, Yangyang Fan1, Xiaoya Tao2, Wenxin Yin1 & Yong He1 We investigated the feasibility and potentiality of determining frmness, soluble solids content (SSC), and pH in kiwifruits using hyperspectral imaging, combined with variable selection methods and calibration models. The images were acquired by a push-broom hyperspectral refectance imaging system covering two spectral ranges. Weighted regression coefcients (BW), successive projections algorithm (SPA) and genetic algorithm–partial least square (GAPLS) were compared and evaluated for the selection of efective wavelengths. Moreover, multiple linear regression (MLR), partial least squares regression and least squares support vector machine (LS-SVM) were developed to predict quality attributes quantitatively using efective wavelengths. The established models, particularly SPA-MLR, SPA-LS-SVM and GAPLS-LS-SVM, performed well. The SPA-MLR models for frmness (Rpre = 0.9812, RPD = 5.17) and SSC (Rpre = 0.9523, RPD = 3.26) at 380–1023 nm showed excellent performance, whereas GAPLS-LS-SVM was the optimal model at 874–1734 nm for predicting pH (Rpre = 0.9070, RPD = 2.60). Image processing algorithms were developed to transfer the predictive model in every pixel to generate prediction maps that visualize the spatial distribution of frmness and SSC. Hence, the results clearly demonstrated that hyperspectral imaging has the potential as a fast and non-invasive method to predict the quality attributes of kiwifruits. Fruit quality represents a combination of properties and attributes that determine the suitability of the fruit to be eaten as fresh or stored for a reasonable period without deterioration and confer a value regarding consum- er’s satisfaction1, 2. -
Comparison of Hyperspectral Imaging and Near-Infrared Spectroscopy to Determine Nitrogen and Carbon Concentrations in Wheat
remote sensing Article Comparison of Hyperspectral Imaging and Near-Infrared Spectroscopy to Determine Nitrogen and Carbon Concentrations in Wheat Iman Tahmasbian 1,* , Natalie K. Morgan 2, Shahla Hosseini Bai 3, Mark W. Dunlop 1 and Amy F. Moss 2 1 Department of Agriculture and Fisheries, Queensland Government, Toowoomba, QLD 4350, Australia; Scopus affiliation ID: 60028929; [email protected] 2 School of Environmental and Rural Science, University of New England, Armidale, NSW 2351, Australia; [email protected] (N.K.M.); [email protected] (A.F.M.) 3 Centre for Planetary Health and Food Security, School of Environment and Science, Griffith University, Brisbane, QLD 4111, Australia; s.hosseini-bai@griffith.edu.au * Correspondence: [email protected] Abstract: Hyperspectral imaging (HSI) is an emerging rapid and non-destructive technology that has promising application within feed mills and processing plants in poultry and other intensive animal industries. HSI may be advantageous over near infrared spectroscopy (NIRS) as it scans entire samples, which enables compositional gradients and sample heterogenicity to be visualised and analysed. This study was a preliminary investigation to compare the performance of HSI with that of NIRS for quality measurements of ground samples of Australian wheat and to identify the most important spectral regions for predicting carbon (C) and nitrogen (N) concentrations. In total, 69 samples were scanned using an NIRS (400–2500 nm), and two HSI cameras operated in Citation: Tahmasbian, I.; Morgan, 400–1000 nm (VNIR) and 1000–2500 nm (SWIR) spectral regions. Partial least square regression N.K; Hosseini Bai, S.; Dunlop, M.W; (PLSR) models were used to correlate C and N concentrations of 63 calibration samples with their Moss, A.F Comparison of spectral reflectance, with 6 additional samples used for testing the models. -
Hyperspectral Imaging with a TWINS Birefringent Interferometer
Vol. 27, No. 11 | 27 May 2019 | OPTICS EXPRESS 15956 Hyperspectral imaging with a TWINS birefringent interferometer 1,2,4 3,4 3 A. PERRI, B. E. NOGUEIRA DE FARIA, D. C. TELES FERREIRA, D. 1 1 1,2 1,2 3 COMELLI, G. VALENTINI, F. PREDA, D. POLLI, A. M. DE PAULA, G. 1,2 1, CERULLO, AND C. MANZONI * 1IFN-CNR, Dipartimento di Fisica, Politecnico di Milano, Piazza Leonardo da Vinci 32, I-20133 Milano, Italy 2NIREOS S.R.L., Via G. Durando 39, 20158 Milano, Italy 3Departamento de Física, Universidade Federal de Minas Gerais, 31270-901 Belo Horizonte-MG, Brazil 4The authors contributed equally to the work *[email protected] Abstract: We introduce a high-performance hyperspectral camera based on the Fourier- transform approach, where the two delayed images are generated by the Translating-Wedge- Based Identical Pulses eNcoding System (TWINS) [Opt. Lett. 37, 3027 (2012)], a common- path birefringent interferometer that combines compactness, intrinsic interferometric delay precision, long-term stability and insensitivity to vibrations. In our imaging system, TWINS is employed as a time-scanning interferometer and generates high-contrast interferograms at the single-pixel level. The camera exhibits high throughput and provides hyperspectral images with spectral background level of −30dB and resolution of 3 THz in the visible spectral range. We show high-quality spectral measurements of absolute reflectance, fluorescence and transmission of artistic objects with various lateral sizes. © 2019 Optical Society of America under the terms of the OSA Open Access Publishing Agreement 1. Introduction A great deal of physico-chemical information on objects can be obtained by measuring the spectrum of the light they emit, scatter or reflect. -
And H-Band Spectra of Globular Clusters in The
A&A 543, A75 (2012) Astronomy DOI: 10.1051/0004-6361/201218847 & c ESO 2012 ! Astrophysics Integrated J-andH-band spectra of globular clusters in the LMC: implications for stellar population models and galaxy age dating!,!!,!!! M. Lyubenova1,H.Kuntschner2,M.Rejkuba2,D.R.Silva3,M.Kissler-Patig2,andL.E.Tacconi-Garman2 1 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany e-mail: [email protected] 2 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany 3 National Optical Astronomy Observatory, 950 North Cherry Ave., Tucson, AZ, 85719 USA Received 19 January 2012 / Accepted 1 May 2012 ABSTRACT Context. The rest-frame near-IR spectra of intermediate age (1–2 Gyr) stellar populations aredominatedbycarbonbasedabsorption features offering a wealth of information. Yet, spectral libraries that include the near-IR wavelength range do not sample a sufficiently broad range of ages and metallicities to allowforaccuratecalibrationofstellar population models and thus the interpretation of the observations. Aims. In this paper we investigate the integrated J-andH-band spectra of six intermediate age and old globular clusters in the Large Magellanic Cloud (LMC). Methods. The observations for six clusters were obtained with the SINFONI integral field spectrograph at the ESO VLT Yepun tele- scope, covering the J (1.09–1.41 µm) and H-band (1.43–1.86 µm) spectral range. The spectral resolution is 6.7 Å in J and 6.6 Å in H-band (FWHM). The observations were made in natural seeing, covering the central 24"" 24"" of each cluster and in addition sam- pling the brightest eight red giant branch and asymptotic giant branch (AGB) star candidates× within the clusters’ tidal radii. -
Hyperspectral Microscopy for Early and Rapid Detection Of
HYPERSPECTRAL MICROSCOPY FOR EARLY AND RAPID DETECTION OF SALMONELLA SEROTYPES by MATTHEW BRENT EADY (Under the Direction of Bosoon Park) ABSTRACT Optical microbial detection methodologies have shown the potential as early and rapid pathogen detection methods. This proof-of-concept project explores the use of hyperspectral microscopy as a potential method for early and rapid classification of five Salmonella serotypes. Darkfield hyperspectral microscope images were collected at early incubation times of 6, 8, 10, and 12 hrs., then compared to 24 hrs. incubation. Hypercube data collected from cells were analyzed through multivariate data analysis (MVDA) methods to assess classification ability of early incubation times. A separate experiment was conducted to explore the ability of analyzing hyperspectral data collected from only informative spectral bands as opposed to the original 89 spectral bands. MVDA showed that incubation times as early as 8 hours had near identical spectra and classification abilities compared to 24 hours; while the original 89-point spectrum could be reduced to 3 selected spectral bands and maintain high serotype classification accuracy. INDEX WORDS: Salmonella, hyperspectral microscopy, early detection, rapid detection, multivariate data HYPERSPECTRAL MICROSCOPY FOR EARLY AND RAPID DETECTION OF SALMONELLA SEROTYPES by MATTHEW BRENT EADY BSA, The University of Georgia, 2011 A Thesis Submitted to the Graduate Faculty of The University of Georgia in Partial Fulfillment of the Requirements for the Degree MASTER OF -
Reconfigurable Terahertz Metamaterial Using Split-Ring Meta
applied sciences Article Reconfigurable Terahertz Metamaterial Using Split-Ring Meta-Atoms with Multifunctional Electromagnetic Characteristics Yuhang Liao and Yu-Sheng Lin * State Key Laboratory of Optoelectronic Materials and Technologies, School of Electronics and Information Technology, Sun Yat-Sen University, Guangzhou 510275, China; [email protected] * Correspondence: [email protected]; Tel.: +86-188-0205-4660 Received: 1 July 2020; Accepted: 29 July 2020; Published: 30 July 2020 Abstract: We propose a reconfigurable terahertz (THz) metamaterial (RTM) to investigate its multifunctional electromagnetic characteristics by moving the meta-atoms of split-ring resonator (SRR) array. It shows the preferable and capable adjustability in the THz frequency range. The electromagnetic characteristics of the proposed RTM device are compared and analyzed by moving the meta-atoms in different polarized transverse magnetic (TM) and transverse electric (TE) modes. The symmetrical meta-atoms of RTM device exhibit a resonant tuning range of several tens of GHz and the asymmetrical meta-atoms of RTM device exhibit the better tunability. Therefore, an RTM device with reconfigurable meta-atoms possesses the resonance shifting, polarization switching, electromagnetically induced transparency (EIT) switching and multiband to single-band switching characteristics. This proposed RTM device provides the potential possibilities for the use of THz-wave optoelectronics with tunable resonance, EIT analog and tunable multiresonance characteristics. Keywords: metamaterial; terahertz; optical switching; electromagnetically induced transparency; resonator 1. Introduction In the last two decades, there has been increasing interest in terahertz (THz) metamaterial optics spanning the spectrum range of 0.1 THz to 10 THz [1,2]. Metamaterials are not natural materials. It means that they are artificially designed [3] and engineered to span the whole electromagnetic spectrum, including visible [4–6], infrared [7–12], THz [13–23] and microwaves [24]. -
The H-Band Emitting Region of the Luminous Blue Variable P Cygni: Spectrophotometry and Interferometry of the Wind
The Astrophysical Journal, 769:118 (12pp), 2013 June 1 doi:10.1088/0004-637X/769/2/118 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A. THE H-BAND EMITTING REGION OF THE LUMINOUS BLUE VARIABLE P CYGNI: SPECTROPHOTOMETRY AND INTERFEROMETRY OF THE WIND N. D. Richardson1,9,10, G. H. Schaefer2,D.R.Gies1,10, O. Chesneau3,J.D.Monnier4, F. Baron1,4, X. Che4, J. R. Parks1, R. A. Matson1,10, Y. Touhami1,D.P.Clemens5, E. J. Aldoretta1,10, N. D. Morrison6, T. A. ten Brummelaar2, H. A. McAlister1,S.Kraus7,S.T.Ridgway8, J. Sturmann2, L. Sturmann2, B. Taylor5, N. H. Turner2, C. D. Farrington2, and P. J. Goldfinger2 1 Center for High Angular Resolution Astronomy, Department of Physics and Astronomy, Georgia State University, P.O. Box 4106, Atlanta, GA 30302-4106, USA; [email protected] 2 The CHARA Array, Georgia State University, P.O. Box 3965, Atlanta, GA 30302-3965, USA 3 Nice Sophia-Antipolis University, CNRS UMR 6525, Observatoire de la Coteˆ d’Azur, BP 4229, F-06304 Nice Cedex 4, France 4 Department of Astronomy, University of Michigan, 941 Dennison Bldg., Ann Arbor, MI 48109-1090, USA 5 Institute for Astrophysical Research, Boston University, 725 Commonwealth Ave., Boston, MA 02215, USA 6 Ritter Astrophysical Research Center, Department of Physics and Astronomy, University of Toledo, 2801 W. Bancroft, Toledo, OH 43606, USA 7 University of Exeter, Astrophysics Group, Stocker Road, Exeter, EX4 4QL, UK 8 National Optical Astronomical Observatory, 950 North Cherry Ave., Tucson, AZ 85719, USA Received 2013 February 7; accepted 2013 April 3; published 2013 May 14 ABSTRACT We present the first high angular resolution observations in the near-infrared H band (1.6 μm) of the luminous blue variable star P Cygni. -
Stellar Spectra in the Hband
110 Wing and Jørgensen, JAAVSO Volume 31, 2003 Stellar Spectra in the H Band Robert F. Wing Department of Astronomy, Ohio State University, Columbus, OH 43210 Uffe G. Jørgensen Niels Bohr Institute, and Astronomical Observatory, University of Copenhagen, DK-2100 Copenhagen, Denmark Presented at the 91st Annual Meeting of the AAVSO, October 26, 2002 [Ed. note: Since this paper was given, the AAVSO has placed 5 near-IR SSP-4 photometers with observers around the world; J and H observations of program stars are being obtained and added to the AAVSO International Database.] Abstract The H band is a region of the infrared centered at wavelength 1.65 microns in a clear window between atmospheric absorption bands. Cool stars such as Mira variables are brightest in this band, and the amplitudes of the light curves of Miras are typically 5 times smaller in H than in V. Since the AAVSO is currently exploring the possibility of distributing H-band photometers to interested members, it is of interest to examine the stellar spectra that these photometers would measure. In most red giant stars, the strongest spectral features in the H band are a set of absorption bands due to the CO molecule. Theoretical spectra calculated from model atmospheres are used to illustrate the pronounced flux peak in H which persists over a wide range of temperature. The models also show that the light in the H band emerges from deeper layers of the star’s atmosphere than the light in any other band. 1. Introduction When multicolor photometry in the infrared was first standardized in the 1960s, Harold Johnson and his colleagues acquired filters to match the windows in the atmospheric absorption and named them with letters of the alphabet (Johnson 1966). -
Near–Infrared Classification Spectroscopy: <I>H</I>–Band Spectra of Fundamental MK Standards
Smith ScholarWorks Astronomy: Faculty Publications Astronomy 11-20-1998 Near–Infrared Classification Spectroscopy: H–band Spectra of Fundamental MK Standards Michael R. Meyer University of Massachusetts Amherst Suzan Edwards Smith College, [email protected] Kenneth H. Hinkle Kitt Peak National Stephen E. Strom University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.smith.edu/ast_facpubs Part of the Astrophysics and Astronomy Commons Recommended Citation Meyer, Michael R.; Edwards, Suzan; Hinkle, Kenneth H.; and Strom, Stephen E., "Near–Infrared Classification Spectroscopy: H–band Spectra of Fundamental MK Standards" (1998). Astronomy: Faculty Publications, Smith College, Northampton, MA. https://scholarworks.smith.edu/ast_facpubs/15 This Article has been accepted for inclusion in Astronomy: Faculty Publications by an authorized administrator of Smith ScholarWorks. For more information, please contact [email protected] THE ASTROPHYSICAL JOURNAL, 508:397È409, 1998 November 20 ( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A. NEAR-INFRARED CLASSIFICATION SPECTROSCOPY: H-BAND SPECTRA OF FUNDAMENTAL MK STANDARDS MICHAEL R. MEYER1 Five College Astronomy Department, University of Massachusetts, Amherst, MA 01003; mmeyer=as.arizona.edu SUZAN EDWARDS Five College Astronomy Department, Smith College, Northampton, MA 01063; edwards=makapuu.ast.smith.edu KENNETH H. HINKLE Kitt Peak NationalObservatory,2 National Optical Astronomy Observatories, Tucson, AZ 85721; hinkle=noao.edu AND STEPHEN E. STROM Five College Astronomy Department, University of Massachusetts, Amherst, MA 01003; sstrom=tsaile.phast.umass.edu Received 1998 April 7; accepted 1998 June 26 ABSTRACT We present a catalog of H-band spectra for 85 stars of approximately solar abundance observed at a resolving power of 3000 with the KPNO Mayall 4 m Fourier Transform Spectrometer.