VIIRS) Sensor Data Record (SDR) User's Guide (Version 1.2

Total Page:16

File Type:pdf, Size:1020Kb

VIIRS) Sensor Data Record (SDR) User's Guide (Version 1.2 NOAA Technical Report NESDIS 142 Visible Infrared Imaging Radiometer Suite (VIIRS) Sensor Data Record (SDR) User’s Guide Version 1.2 Washington, D.C. 10 September 2013 U.S. DEPARTMENT OF COMMERCE National Oceanic and Atmospheric Administration National Environmental Satellite, Data, and Information Service NOAA TECHNICAL REPORTS National Environmental Satellite, Data, and Information Service The National Environmental Satellite, Data, and Information Service (NESDIS) manages the Nation’s civilian Earth-observing satellite systems, as well as global national data bases for meteorology, oceanography, geophysics, and solar-terrestrial sciences. From these sources, it develops and disseminates environmental data and information products critical to the protection of life and property, national defense, the national economy, energy development and distribution, global food supplies, and the development of natural resources. Publication in the NOAA Technical Report series does not preclude later publication in scientific journals in expanded or modified form. The NESDIS series of NOAA Technical Reports is a continuation of the former NESS and EDIS series of NOAA Technical Reports and the NESC and EDS series of Environmental Science Services Administration (ESSA) Technical Reports. An electronic copy of this report may be obtained at: https://cs.star.nesdis.noaa.gov/NCC/VIIRS A limited number of copies of earlier reports are available by contacting, NOAA/NESDIS/STAR, 5830 University Research Ct, Suite 2600, College Park, Maryland 20740, Phone: 301 683-3490. A partial listing of more recent reports appears below: NESDIS 111 An Algorithm for Correction of Lunar Contamination in AMSU-A Data. Seiichiro Kigawa and Tsan Mo, December 2002. NESDIS 112 Sampling Errors of the Global Mean Sea Level Derived from TOPEX/Poseidon Altimetry. Chang-Kou Tai and Carl Wagner, December 2002. NESDIS 113 Proceedings of the International GODAR Review Meeting: Abstracts. Sponsors: Intergovernmental Oceanographic Commission, U.S. National Oceanic and Atmospheric Administration, and the European Community, May 2003. NESDIS 114 Satellite Rainfall Estimation Over South America: Evaluation of Two Major Events. Daniel A. Vila, Roderick A. Scofield, Robert J. Kuligowski, and J. Clay Davenport, May 2003. NESDIS 115 Imager and Sounder Radiance and Product Validations for the GOES-12 Science Test. Donald W. Hillger, Timothy J. Schmit, and Jamie M. Daniels, September 2003. NESDIS 116 Microwave Humidity Sounder Calibration Algorithm. Tsan Mo and Kenneth Jarva, October 2004. NESDIS 117 Building Profile Plankton Databases for Climate and EcoSystem Research. Sydney Levitus, Satoshi Sato, Catherine Maillard, Nick Mikhailov, Pat Cadwell, Harry Dooley, June 2005. NESDIS 118 Simultaneous Nadir Overpasses for NOAA-6 to NOAA-17 Satellites from 1980 and 2003 for the Intersatellite Calibration of Radiometers. Changyong Cao, Pubu Ciren, August 2005. NESDIS 119 Calibration and Validation of NOAA 18 Instruments. Fuzhong Weng and Tsan Mo, December 2005. NESDIS 120 The NOAA/NESDIS/ORA Windsat Calibration/Validation Collocation Database. Laurence Connor, February 2006. NESDIS 121 Calibration of the Advanced Microwave Sounding Unit-A Radiometer for METOP-A. Tsan Mo, August 2006. NOAA Technical Report NESDIS 142 Visible Infrared Imaging Radiometer Suite (VIIRS) Sensor Data Record (SDR) User’s Guide Version 1.2 Changyong Cao1, Xiaoxiong (Jack) Xiong2, Robert Wolfe2, Frank DeLuccia3, Quanhua (Mark) Liu1, Slawomir Blonski1, Guoqing (Gary) Lin2, Masahiro Nishihama2, Dave Pogorzala1, Hassan Oudrari2, and Don Hillger1 1NOAA/NESDIS/STAR College Park, MD 20740 2NASA/GSFC Greenbelt, MD 20771 3The Aerospace Corporation Los Angeles, CA 90009 Washington, DC September 2013 U.S. DEPARTMENT OF COMMERCE John Bryson, Secretary National Oceanic and Atmospheric Administration Dr. Jane Lubchenco, Under Secretary of Commerce for Oceans and Atmosphere and NOAA Administrator National Environmental Satellite, Data, and Information Service Mary Kicza, Assistant Administrator Revision History Revision Date Brief Summary of Changes Version 0.9(draft) 01 August 2011 Baseline document draft Version 1.0 20 December 2011 Baseline document Version 1.1 19 February 2013 Updated geometric description, 11 April 2013 made corrections to several other Sections Version 1.2 10 September 2013 Re-baseline for the Tech Report ID Note: For the latest versions of this document, please visit http://www.start.nesdis.noaa.gov/jpss/VIIRS, or http://ncc.nesdis.noaa.gov in the VIIRS section of the Calibration Knowledge Base (CKB). iv 1. INTRODUCTION..................................................................................................... 1 1.1 PURPOSE OF THIS GUIDE ...................................................................................... 2 1.2 VIIRS HERITAGE ................................................................................................. 2 2. AN OVERVIEW OF THE VIIRS INSTRUMENT ............................................... 4 2.1 VIIRS DESIGN ..................................................................................................... 4 2.1.1 VIIRS Special Geometric Features ................................................................. 7 2.2 VIIRS SPECTRAL BANDS ..................................................................................... 9 2.3 VIIRS ONBOARD CALIBRATION AND RADIOMETRIC PERFORMANCE................. 11 2.4 VIIRS POSTLAUNCH CALIBRATION/VALIDATION .............................................. 13 3. VIIRS DATA RECORDS....................................................................................... 15 3.1 RAW DATA RECORDS (RDR) ............................................................................. 15 3.2 SENSOR DATA RECORDS (SDR)......................................................................... 16 3.3 ENVIRONMENTAL DATA RECORDS (EDR) ......................................................... 17 3.4 QUALITY FLAGS, GRANULE AND AGGREGATION-LEVEL METADATA ................. 18 4. DATA PROCESSING AND RADIOMETRIC CALIBRATION ...................... 20 4.1 DATA PROCESSING FLOW .................................................................................. 21 4.1.1 SDR Algorithms Overview ............................................................................ 22 4.1.2 Calibration Algorithms and Coefficients for the TEBs ................................. 22 4.1.3 Calibration Algorithms and Coefficients for the RSBs ................................. 24 4.1.4 Day-Night-Band (DNB) ................................................................................ 26 4.2 LOOK UP TABLES (LUTS).................................................................................. 27 5. GEOLOCATION AND GEOMETRIC PERFORMANCE ............................... 28 5.1 GEOLOCATION ALGORITHM ............................................................................... 28 5.2 BAND-TO-BAND REGISTRATION (BBR) ............................................................. 31 5.3 SPATIAL RESPONSE, SPATIAL RESOLUTION, AND IMAGE QUALITY .................... 32 6. DATA DISTRIBUTION, ACCESS, AND DISPLAY .......................................... 35 6.1 DISTRIBUTION AND ACCESS ............................................................................... 35 6.2 DATA FILES AND SOFTWARE TOOLS .................................................................. 35 6.3 DIRECT READOUT (DRO) .................................................................................. 36 7. REFERENCES ........................................................................................................ 37 8. ACKNOWLEDGEMENTS ................................................................................... 38 9. APPENDIX: ACRONYMS (AND ABBREVIATIONS) USED IN THIS REPORT .......................................................................................................................... 39 i 1. Introduction The Joint Polar Satellite System (JPSS) is our nation's next generation polar-orbiting operational environmental satellite system, procured by the National Oceanic and Atmospheric Administration (NOAA) through the National Aeronautics and Space Administration (NASA). JPSS will provide continuity of critical observations for accurate weather forecasting, reliable severe storm outlooks, global measurements of atmospheric, oceanic, and land surface variables such as atmospheric temperature and water vapor profiles, clouds, sea surface temperatures, vegetation, fire, aerosols, ocean color, and others. The JPSS was established in year 2010 as a result of restructuring the National Polar- orbiting Operational Environmental Satellite System (NPOESS), to provide the continuity for NOAA’s polar-orbiting operational environmental satellite system (POES). As a result of the restructuring, NOAA and NASA were instructed by the U.S. President’s Office of Science and Technology to develop a mission that addresses afternoon orbit (~1:30 PM local equator crossing time at ascending node) data collection with a 16-day repeat cycle, while the EUMETSAT is responsible for the mid-morning orbit with their MetOp series which carry both NOAA and EUMETSAT instruments, and the U.S. Department of Defense (DoD) would be responsible for the early morning orbit. Development and subsequent operation of a shared Common Ground System (CGS) will supersede the Interface Data Processing Segment (IDPS) while the IDPS continues uninterrupted before the CGS takes over. In the early days of planning for NPOESS, it was deemed
Recommended publications
  • Mitigation of Terrestrial Radar Interference in L-Band Spaceborne Microwave Radiometers
    Mitigation of Terrestrial Radar Interference in L-Band Spaceborne Microwave Radiometers J.R. Piepmeier and F.A. Pellerano Microwave Instrument Technology Branch NASA's Goddard Space Flight Center Greenbelt, MD 2 1 146 Email: [email protected] Abstract-Terrestrial radars operating in the 1215-1400 MHz Hydros missions [lo]. Given the impacts, three aspects to radio-location and navigation spectrum allocation are important mitigation are proposed: survivability, operability, and excis- for air traffic safety, homeland security, and national defense. For ability; or SOE. Survivability deals with avoiding damage low-frequency observations of soil moisture and ocean salinity, Earth-observing microwave radiometers are allocated Earth- from RFI. This means proper filtering and limiting. A ra- Exploration Satellite Service (EESS) spectrum for operating at diometer achieves operability when it can measure, without 1400-1427 MHz. The proximity of powerful long-range radars to error, the antenna or brightness temperature in the presence of the passive allocation makes observing a challenge. Three aspects interference. Selective receivers operating in quite spectrum of mitigation to RFI are discussed in this paper: survivability, are required for operability. When filtering and frequency operability, and excisability (SOE). Modeling and simulations of NASA's Hydros and Aquarius radiometers were performed selection is not enough to avoid interference, then the RFI to examine the impacts of radar interference. The results are might be excisable. A number of techniques have been pro- applied to the three aspects of mitigation SOE and the affects posed and demonstrated recently [Ill-[14]. These fall into on the radiometer requirements are discussed. three basic categories: temporal, spectral, and statistical - some techniques are a combination of two or more.
    [Show full text]
  • Terahertz Induced Non-Linear Electron Dynamics in Nanoantenna Coated Semiconductors at the Sub-Picosecond Timescale
    AN ABSTRACT OF THE DISSERTATION OF Andrew Stickel for the degree of Doctor of Philosophy in Physics presented on August 10, 2016. Title: Terahertz Induced Non-linear Electron Dynamics in Nanoantenna Coated Semiconductors at the Sub-picosecond Timescale Abstract approved: Yun-Shik Lee This dissertation is an exploration of the material response to Terahertz (THz) radiation. Specifically we will explore the ultrafast electron dynamics in the non- perturbative regime in semiconductors that have been patterned with nanoantenna arrays using broadband, high intensity, THz radiation. Three main semiconductor materials will be studied in this work. The first is VO2 which undergoes a phase transition from an insulator, when it is below 67◦ C, to a metal, when it is above 67◦ C. The second and third materials are Si and GaAs which are two of the most commonly used semiconductors. We study the insulator to metal transition (IMT) of VO2 and its response to high field THz radiation. The near room temperature IMT for VO2 makes it a very promising material for electrical and photonic applications. We demonstrate that with high field THz the IMT transition can be triggered. This transition is induced on a sub-cycle timescale. We also demonstrate a THz field dependent reduction in the transition temperature for the IMT when transitioning from both below Tc to above as well as from above Tc to below. This transition is not equal for the above and below cases and leads to a narrowing of the hysteresis curve of the IMT. The thin film Fresnel coefficients, along with a phenomenological model developed for the nanoantenna patterned VO2, are also used to calculate the sheet conductivity of the VO2 sample.
    [Show full text]
  • Disarmament Conference'
    University of Nebraska at Omaha DigitalCommons@UNO Kabul Times Digitized Newspaper Archives 7-28-1965 Kabul Times (July 28, 1965, vol. 4, no. 104) Bakhtar News Agency Follow this and additional works at: https://digitalcommons.unomaha.edu/kabultimes Part of the International and Area Studies Commons Recommended Citation Bakhtar News Agency, "Kabul Times (July 28, 1965, vol. 4, no. 104)" (1965). Kabul Times. 1025. https://digitalcommons.unomaha.edu/kabultimes/1025 This Newspaper is brought to you for free and open access by the Digitized Newspaper Archives at DigitalCommons@UNO. It has been accepted for inclusion in Kabul Times by an authorized administrator of DigitalCommons@UNO. For more information, please contact [email protected]. ~!'. - _. .,.. -::'~ _:.~---- ';'- ' . _.: . ---~ _._ ....... :$2:_ 3 ;c: ... ce,,~ -. : ': ': . :; ',-'•.f - . -. ..:. " -' , -.'. -. .: -~. - . - . .. ,: - '. ••.t • - -.:- --.:'~ '~-' ...- '. -. .. -. ." ..- - -- • : : '- . " . .. --- '" .. , , : -­ - . -... _. :-. -: :-- - . '. ., . -. ~ - ' . .. - . '. , . , · ., .' .- ---. ~ . ,; __ 7-_ ..- • -. - .. - • < ,.., ,- .. :. '.' , . if '. NEWS STALLS . -.... -, . ~ -"- - ~. THE WEATHER "-". .., . KABUL TIMES JULY 27, 1965 Yesterday'S Tempera&are . ~, < • , .'t,. Max, + 31'C, Minimum 12°C· I·,' .: ..~ , Sun sets· today at 6:54 P.DL Belgian En-voy He.r-e.NamedI '- , ,Nasser De'njes VARAIr Force· suD. rjses tomorrow at 5:03 am· - Tomorrow's Outlook: Cloudy ~ -.. KA~UL, 27.~The .' ".' ',' 'Tr'ied To'Bomb His~Re$idence' July Ministry . of 'Foreign Affairs smd :yesterday j VOL. rv,NO. 104 KABUL'WEDNESDAY,. .JULY ·28"(ASA'D:··6~1344;··S.H.) :: .,:, -:'.:'. , . =;:.0 .....- . :"'-, '. '.;-- / . s . .(DPA):~ ~~~~~~_~~~~~ ,_~ ~".~~~.~~~c~,~~:~._.~~.~.~:~~~~~~~~~~~~.~.~_~.~.,~:=.~~.C=E~.A~.!~:! ~.:~~~ '·:.ALExANDRIA, JulY' ·27) that Jean Leroy, .the Belgian Am­ e' . , .. , .. .. pRESIDENT Gamal Abci~l.Nasser.1?f.t~e uAR has ~tegori. bassado!' in N~w DeIhi, -has been '. , cally d~n1ed th!lt an attelJi:)t~~ been made by aU' force, appointed to act siniultaneously as ·1Ii......· ,.
    [Show full text]
  • A Study of the Fundamental Vibration-Rotation Bands in the Infrared Spectra of St I Bene and Deutero-Stibene
    A STUDY OF THE FUNDAMENTAL VIBRATION-ROTATION BANDS IN THE INFRARED SPECTRA OF ST I BENE AND DEUTERO-STIBENE DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By William Howard Haynle, S.F., M*Sc« The Ohio State University 1961 Approved byi «w-<'s i wi[//// Adviser ACKNOWLfcDGLlEHTS It gives me pleasure to acknowledge the help and oooperation extended to me by many persons during the course of this investiga­ tion* For advice on the theory of molecular structure and sugges­ tions on the interpretation of the experimental data I am indebted to Professors K* H* Nielsen and E* E* Bell* I am very grateful to Professor J. 0* Lord of the Department of Metallurgy for help in preparing a suitable alloy, and to Professor A* B. Garrett of the Department of Chemistry for advice concerning the chemical proce­ dures involved in generating the samples. My thanks are due to Mr* William Ward for help in obtaining the data* I am particularly Indebted to Professor R* A* Oetjen for his advice and encouragement over the past five years* Finally, I wish to express my sincere gratitude to Gloria Westphal Haynle who has checked the proof and verified all of the calculations* Her help and encouragement have been invaluable* 0 2 2 1 < > 2 TABLE OF CONTENTS Fag® Introduction ................................ 1 Summary of Theoretical Work ........................ 5 Experimental W o r k ............................................... 18 Analysis of the Absorption Spectra of SbH and SbD_ ........... 26 3 3 Appendix......................................................... 55 Bibliography ..................................................
    [Show full text]
  • A Comprehensive Review on Food Applications of Terahertz Spectroscopy and Imaging Leili Afsah-Hejri , Parvaneh Hajeb, Parsa Ara, and Reza J
    A Comprehensive Review on Food Applications of Terahertz Spectroscopy and Imaging Leili Afsah-Hejri , Parvaneh Hajeb, Parsa Ara, and Reza J. Ehsani Abstract: Food product safety is a public health concern. Most of the food safety analytical and detection methods are expensive, labor intensive, and time consuming. A safe, rapid, reliable, and nondestructive detection method is needed to assure consumers that food products are safe to consume. Terahertz (THz) radiation, which has properties of both microwave and infrared, can penetrate and interact with many commonly used materials. Owing to the technological developments in sources and detectors, THz spectroscopic imaging has transitioned from a laboratory-scale technique into a versatile imaging tool with many practical applications. In recent years, THz imaging has been shown to have great potential as an emerging nondestructive tool for food inspection. THz spectroscopy provides qualitative and quantitative information about food samples. The main applications of THz in food industries include detection of moisture, foreign bodies, inspection, and quality control. Other applications of THz technology in the food industry include detection of harmful compounds, antibiotics, and microorganisms. THz spectroscopy is a great tool for characterization of carbohydrates, amino acids, fatty acids, and vitamins. Despite its potential applications, THz technology has some limitations, such as limited penetration, scattering effect, limited sensitivity, and low limit of detection. THz technology is still expensive, and there is no available THz database library for food compounds. The scanning speed needs to be improved in the future generations of THz systems. Although many technological aspects need to be improved, THz technology has already been established in the food industry as a powerful tool with great detection and quantification ability.
    [Show full text]
  • Arxiv:1512.01105V1 [Astro-Ph.GA] 3 Dec 2015
    Accepted to the Astrophysical Journal on November 30, 2015 A Preprint typeset using LTEX style emulateapj v. 5/2/11 THE CHANDRA COSMOS LEGACY SURVEY: OPTICAL/IR IDENTIFICATIONS S. Marchesi1,2,3, F. Civano1,2, M. Elvis2, M. Salvato4, M. Brusa3,5, A. Comastri5, R. Gilli5, G. Hasinger6, G. Lanzuisi3,5, T. Miyaji7,8, E. Treister9, C.M. Urry1, C. Vignali3,5, G. Zamorani5, V. Allevato10, N. Cappelluti5, C. Cardamone11, A. Finoguenov10, R. E. Griffiths12, A. Karim13, C. Laigle14, S. M. LaMassa1, K. Jahnke15, P. Ranalli16, K. Schawinski17, E. Schinnerer18,19, J. D. Silverman20, V. Smolcic21, H. Suh6,2, B. Trakhtenbrot17 Accepted to the Astrophysical Journal on November 30, 2015 ABSTRACT We present the catalog of optical and infrared counterparts of the Chandra COSMOS-Legacy Survey, a 4.6 Ms Chandra program on the 2.2 deg2 of the COSMOS field, combination of 56 new overlapping observations obtained in Cycle 14 with the previous C-COSMOS survey. In this Paper we report the i, K, and 3.6 µm identifications of the 2273 X-ray point sources detected in the new Cycle 14 observations. We use the likelihood ratio technique to derive the association of optical/infrared (IR) counterparts for 97% of the X-ray sources. We also update the information for the 1743 sources detected in C-COSMOS, using new K and 3.6 µm information not available when the C-COSMOS analysis was performed. The final catalog contains 4016 X-ray sources, 97% of which have an op- tical/IR counterpart and a photometric redshift, while ≃54% of the sources have a spectroscopic redshift.
    [Show full text]
  • X-Ray Properties of Young Stars and Stellar Clusters 313
    Feigelson et al.: X-Ray Properties of Young Stars and Stellar Clusters 313 X-Ray Properties of Young Stars and Stellar Clusters Eric Feigelson and Leisa Townsley Pennsylvania State University Manuel Güdel Paul Scherrer Institute Keivan Stassun Vanderbilt University Although the environments of star and planet formation are thermodynamically cold, sub- stantial X-ray emission from 10–100 MK plasmas is present. In low-mass pre-main-sequence stars, X-rays are produced by violent magnetic reconnection flares. In high-mass O stars, they are produced by wind shocks on both stellar and parsec scales. The recent Chandra Orion Ultra- deep Project, XMM-Newton Extended Survey of Taurus, and Chandra studies of more distant high-mass star-forming regions reveal a wealth of X-ray phenomenology and astrophysics. X- ray flares mostly resemble solar-like magnetic activity from multipolar surface fields, although extreme flares may arise in field lines extending to the protoplanetary disk. Accretion plays a secondary role. Fluorescent iron line emission and absorption in inclined disks demonstrate that X-rays can efficiently illuminate disk material. The consequent ionization of disk gas and irradiation of disk solids addresses a variety of important astrophysical issues of disk dynam- ics, planet formation, and meteoritics. New observations of massive star-forming environments such as M 17, the Carina Nebula, and 30 Doradus show remarkably complex X-ray morpholo- gies including the low-mass stellar population, diffuse X-ray flows from blister HII regions, and inhomogeneous superbubbles. X-ray astronomy is thus providing qualitatively new insights into star and planet formation. 1. INTRODUCTION ment of the stellar surface by electron beams.
    [Show full text]
  • Living & Ulvac
    LIVING & ULVAC Communication Infrastructure Front Line for Diffusion of Cellular Phones Further acceleration via Development of High-performance Microwave Communication Devices Reporting from Toshiba Corporation Social Infrastructure Systems Company Microwave Solid-State Engineering Department, Komukai Complex Application field of Microwave SATCOM/VSAT Marine Radar Weather Radar Fixed Wireless Access Digital Broadcasting TTL FPU Fixed Wireless Access SNG FPU STL TSL WiMAX Fixed Wireless Access Industrial-Use Mobile Phone Data from Toshiba Corporation Social Infrastructure Systems Company VSAT: Very Small Aperture Terminal STL: Studio to Transmitter Link SATCOM: Satellite Communication TSL: Transmitter to Studio Link WiMAX: Worldwide Interoperability for Microwave Access FPU: Field Pickup Unit SNG: Satellite News Gathering ITS: Intelligent Transport Systems TTL: Transmitter to Transmitter Link LIVING & ULVAC 10 ULVAC | No.64 More than 1.75 billion cellular phones are manufactured annually worldwide (2012 survey by Gartner, Inc.), and 94.5% of households in Japan have one or more cellular phones (2012 survey by the Ministry of Internal Affairs and Communications). In particular, it would be no‥exaggeration‥to‥say‥that‥almost‥everyone‥in‥their‥twenties‥and‥almost‥all‥university‥students‥have‥a‥cellular‥phone.‥In‥addition,‥it‥may‥ be safely said that today, a cellular phone is also a must-have item for elderly people. Originally, wireless communication was achieved with wireless communication equipment that made use of short wave radio frequencies to connect two parties directly. Wireless com- Communication Infrastructure Front Line munication via cellular phones is significantly different from wireless communication of the past in that cellular phones connect two com- for Diffusion of Cellular Phones municating parties via communication stations, which are connected via a wired communication network.
    [Show full text]
  • Standard Photometric Systems
    7 Aug 2005 11:27 AR AR251-AA43-08.tex XMLPublishSM(2004/02/24) P1: KUV 10.1146/annurev.astro.41.082801.100251 Annu. Rev. Astron. Astrophys. 2005. 43:293–336 doi: 10.1146/annurev.astro.41.082801.100251 Copyright c 2005 by Annual Reviews. All rights reserved STANDARD PHOTOMETRIC SYSTEMS Michael S. Bessell Research School of Astronomy and Astrophysics, The Australian National University, Weston, ACT 2611, Australia; email: [email protected] KeyWords methods: data analysis, techniques: photometric, spectroscopic, catalogs ■ Abstract Standard star photometry dominated the latter half of the twentieth century reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity and large dynamic range of photomultiplier tubes compared to photographic plates. As the quantum efficiency of photodetectors improved and the wavelength range extended further to the red, standard systems were modified and refined, and deviations from the original systems proliferated. The revolutionary shift to area detectors for all optical and IR observations forced further changes to standard systems, and the precision and accuracy of much broad- and intermediate-band photometry suffered until more suitable observational techniques and standard reduction procedures were adopted. But the biggest revolution occurred with the production of all-sky photometric surveys. Hipparcos/Tycho was space based, but most, like 2MASS, were ground-based, dedicated survey telescopes. It is very likely that in the future, rather than making a measurement of an object in some standard photometric system, one will simply look up the magnitudes and colors of most objects in catalogs accessed from the Virtual Observatory.
    [Show full text]
  • HORIBA Webinar Proteins
    © 2012 HORIBA Scientific. All rights reserved. © 2012 HORIBA Scientific. All rights reserved. Raman Spectroscopy for proteins Catalina DAVID Ph.D.– application scientist © 2012 HORIBA Scientific. All rights reserved. Outline Raman spectroscopy in few words What is Raman spectroscopy ? What is the information we can get? Basics of Raman analysis of proteins Raman spectrum of proteins Environmental effects on the protein Raman spectrum Contributions to the protein Raman spectrum UV Resonances Raman for proteins Polarization measurements for proteins Low-frequency measurements for proteins Conclusions © 2012 HORIBA Scientific. All rights reserved. Raman Spectroscopy in few words © 2012 HORIBA Scientific. All rights reserved. What is Raman Spectroscopy Raman effect = Inelastic Light Scattering λλλ λλλ diff < laser anti-Stokes Raman molecule or crystal λλλ λλλ diff = laser Rayleigh Diffusion λλλ laser Excitation λλλ λλλ diff > laser Stokes Raman The frequency ( ν = 1/ λ) difference between the incident and the scattered light characterises the molecule vibration. ννν ννν ννν scattered = laser ±±± vibration © 2012 HORIBA Scientific. All rights reserved. What is the information we can get Band position: Chemical species, crystal phases, alloy compositions Frequency Shift: Strain, temperature Intensity: Concentration Linewidth: Structural disorder A Raman spectrum provides a fingerprint which represents the set of bonds present in the material: vibrational frequencies are characteristic of chemical bonds or groups of bonds Vibrational frequencies are sensitive to details of the structure and local environment of a molecule, such as symmetry, crystal phase, polymer morphology, solvents, interactions, … Relative intensities corresponds principally to the species concentration but it can be related to the orientation of the material or molecule with respect to the incoming laser polarization.
    [Show full text]
  • Maritime Radar Performance
    Solid State Navigation and Situation Awareness Radar Radar 2008 1904 1948- present 19001900 19501950 20002000 Origins of Commercial Marine Radar Kelvin Hughes New Marine Radar 1948 Type 1 • First UK Type Approved Marine Radar – 11th August 1948 • Specification – Upmast Transmitter/Receiver – Antenna Rotation: 30RPM – Peak Power:- 30kW – RF Frequency:- 9.434GHz - 9.524GHz – PRF:- 1kHz – Pulse Width: 0.2μs – Azimuth Beamwidth:- 1.5° – Elevation Beamwidth:- 27° Sensor Improvements Advances in Sensor Technology Low Noise Front Ends FET Modulators Improved Magnetron Life Current Sensors at Peak of Performance However……… Magnetron - Short Pulse Spectrum Little improvement in 0 performance in clutter -10 -20 Customers & Regulators -30 -40 demand detection of smaller -50 targets -60 Power (dBc/Hz) Power -70 Customers want more reliable -80 -90 systems -100 2 4 6 8 10 12 14 16 Frequency (GHz) Pressure from ITU to restrict radar bandwidth and out of band emissions SharpEye Introduction • First ‘New Technology’ Marine Navigation Radar for 60 years • Conforms to requirements of IMO & IEC • ‘Family’ of Products – Built-in Flexibility through design and part selection – Considered future enhancements during concept/design phase – 100% PV Funded Development • Performance/Cost Trade-Off – Minimum performance IEC 62388 (new radar standard - July 2008) • More performance expected but not at expense of production cost/quality • Achieve performance through innovation – Economies of scale • Re-use of components/sub-assemblies throughout product range • Reliability and Maintainability high on our priorities SharpEye World’s 1st Solid State Marine Navigation Radar Features include: •Solid state transmitter •Coherent transmitter and receiver •Pulse compression •Digital signal processing •Interference suppression •Low voltage operation What sets Sharpeye apart • Incorporates advantages in semi-conductor based radars but at a cost that competes with conventional magnetron systems • Sharpeye incorporates low power RF architecture.
    [Show full text]
  • Measurement of the Band-To-Band Registration of the SNPP VIIRS Imaging System from On-Orbit Data
    IEEE JSTARS-2016-00373 1 Measurement of the Band-to-Band Registration of the SNPP VIIRS Imaging System from On-Orbit Data James C. Tilton, Senior Member, IEEE, Guoqing (Gary) Lin and Bin Tan different due to differences in spectral responses at different Abstract — The Visible Infrared Imaging Radiometer Suite wavelengths. To overcome this problem we use the Normalized (VIIRS) instrument was launched 28 October 2011 onboard the Mutual Information (NMI) method for image registration [3, 4, Suomi National Polar‐orbiting Partnership (SNPP) satellite. The 5, 6]. The NMI method relies on the statistical dependency VIIRS instrument is a whiskbroom system with 22 spectral and between two images to determine their correlation. Both thermal bands split between 16 moderate resolution bands (M- bands), five imagery resolution bands (I-bands) and a day-night positive and negative radiometric correlations between the band. In this study we measure the along-scan and along-track images contribute positively to the statistical dependency band-to-band registration between the I-bands and M-bands from between the images. In contrast, positive and negative on-orbit data. This measurement is performed by computing the radiometric correlations tend to cancel each other out in the Normalized Mutual Information (NMI) between shifted image cross-correlation method. band pairs and finding the amount of shift required (if any) to Wang, et al [7] recently reported on an approach for produce the peak in NMI value. Subpixel accuracy is obtained by utilizing bicubic interpolation. The product of the NMI peak slope measuring the band-to-band registration (BBR) of VIIRS and the NMI peak value is shown to be a better criterion for reflective solar bands based on lunar observations.
    [Show full text]