Waves of the Electromagnetic Spectrum
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
Microwave Communications and Radar
2/26 6.014 Lecture 14: Microwave Communications and Radar A. Overview Microwave communications and radar systems have similar architectures. They typically process the signals before and after they are transmitted through space, as suggested in Figure L14-1. Conversion of the signals to electromagnetic waves occurs at the output of a power amplifier, and conversion back to signals occurs at the detector, after reception. Guiding-wave structures connect to the transmitting or receiving antenna, which are generally one and the same in monostatic radar systems. We have discussed antennas and multipath propagation earlier, so the principal novel mechanisms we need to understand now are the coupling of these electromagnetic signals between antennas and circuits, and the intervening propagating structures. Issues we must yet address include transmission lines and waveguides, impedance transformations, matching, and resonance. These same issues also arise in many related systems, such as lidar systems that are like radar but use light beams instead, passive sensing systems that receive signals emitted by the environment either naturally (like thermal radiation) or by artifacts (like motors or computers), and data recording systems like DVD’s or magnetic disks. The performance of many systems of interest is often limited in part by our ability to couple energy efficiently from one port to another, and our ability to filter out deleterious signals. Understanding these issues is therefore an important part of such design effors. The same issues often occur in any system utilizing high-frequency signals, whether or not they are transmitted externally. B. Radar, Lidar, and Passive Systems Figure L14-2 illustrates a standard radar or lidar configuration where the transmitted power Pt is focused toward a target using an antenna with gain Gt. -
Radiant Heating with Infrared
W A T L O W RADIANT HEATING WITH INFRARED A TECHNICAL GUIDE TO UNDERSTANDING AND APPLYING INFRARED HEATERS Bleed Contents Topic Page The Advantages of Radiant Heat . 1 The Theory of Radiant Heat Transfer . 2 Problem Solving . 14 Controlling Radiant Heaters . 25 Tips On Oven Design . 29 Watlow RAYMAX® Heater Specifications . 34 The purpose of this technical guide is to assist customers in their oven design process, not to put Watlow in the position of designing (and guaranteeing) radiant ovens. The final responsibility for an oven design must remain with the equipment builder. This technical guide will provide you with an understanding of infrared radiant heating theory and application principles. It also contains examples and formulas used in determining specifications for a radiant heating application. To further understand electric heating principles, thermal system dynamics, infrared temperature sensing, temperature control and power control, the following information is also available from Watlow: • Watlow Product Catalog • Watlow Application Guide • Watlow Infrared Technical Guide to Understanding and Applying Infrared Temperature Sensors • Infrared Technical Letter #5-Emissivity Table • Radiant Technical Letter #11-Energy Uniformity of a Radiant Panel © Watlow Electric Manufacturing Company, 1997 The Advantages of Radiant Heat Electric radiant heat has many benefits over the alternative heating methods of conduction and convection: • Non-Contact Heating Radiant heaters have the ability to heat a product without physically contacting it. This can be advantageous when the product must be heated while in motion or when physical contact would contaminate or mar the product’s surface finish. • Fast Response Low thermal inertia of an infrared radiation heating system eliminates the need for long pre-heat cycles. -
Understanding Infrared Light
TEACHER/PARENT ACTIVITY MANUAL Joint Polar Satellite System Understanding Infrared Light This activity educates students about the electromagnetic spectrum, or different forms of light detected by Earth observing satellites. The Joint Polar Satellite System (JPSS), a collaborative effort between NOAA and NASA, detects various wavelengths of the electromagnetic spectrum including infrared light to measure the temperature of Earth’s surface, oceans, and atmosphere. The data from these measurements provide the nation with accurate weather forecasts, hurricane warnings, wildfire locations, and much more! Provided is a list of materials that can be purchased to complete several learning activities, including simulating infrared light by constructing homemade infrared goggles. Learning Objectives Next Generation Science Standards (Grades 5–8) Performance Disciplinary Description Expectation Core Ideas 4-PS4-1 PS4.A: • Waves, which are regular patterns of motion, can be made in water Waves and Their Wave Properties by disturbing the surface. When waves move across the surface of Applications in deep water, the water goes up and down in place; there is no net Technologies for motion in the direction of the wave except when the water meets a Information Transfer beach. (Note: This grade band endpoint was moved from K–2.) • Waves of the same type can differ in amplitude (height of the wave) and wavelength (spacing between wave peaks). 4-PS4-2 PS4.B: An object can be seen when light reflected from its surface enters the Waves and Their Electromagnetic eyes. Applications in Radiation Technologies for Information Transfer 4-PS3-2 PS3.B: Light also transfers energy from place to place. -
Ultraviolet – Visible Spectroscopy for Determination of Α- and Β-Acids in Beer Hops Katharine Chau Lab Partner: Logan Bi
Ultraviolet – Visible Spectroscopy for Determination of α- and β-acids in Beer Hops Katharine Chau Lab Partner: Logan Billings TA: Kevin Fischer Date lab performed: 3/20/2018 Date report submitted: 4/9/2018 ABSTRACT: In this experiment, the content of α- and β-acids in beer hops is found through UV-Vis spectroscopic analysis. Three samples will be prepared by extracting finely grained hops through methanol and diluting with methanolic NaOH. The spectrums obtained give a constant overall shape. The experiment was done to find out the concentration of the third component from degraded α- and β-acids that is also existing in the hops samples with the help of the calculated concentrations of α- and β-acids. From the calculated results, the average concentration of the third component in all three samples was 0.061 g/L. INTRODUCTION: UV-Vis spectroscopy is a useful absorption or reflectance spectroscopy that helps determine the quantity of analytes by detecting the absorptivity or reflectance of a sample under ultra-violet to visible light wavelength range (1). In this experiment, the absorptivity of the samples were measured and the content of different components were determined from the spectrum. In this lab, UV-Vis spectroscopy was used in to obtain absorbance spectrums of α- and β- acids found in difference hops samples. The structures of α- and β-acids are shown as the Fig. 1 below. Figure 1. Structures of major α- and β-acids found in hops By understanding the content of α-acid in the hops, the bitterness flavor of beer can be controlled since the bitterness is formed by the iso-form of α-acid through isomization of α-acid. -
Relationship Between X-Ray and Ultraviolet Emission of Flares From
A&A 431, 679–686 (2005) Astronomy DOI: 10.1051/0004-6361:20041201 & c ESO 2005 Astrophysics Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton U. Mitra-Kraev1,L.K.Harra1,M.Güdel2, M. Audard3, G. Branduardi-Raymont1 ,H.R.M.Kay1,R.Mewe4, A. J. J. Raassen4,5, and L. van Driel-Gesztelyi1,6,7 1 Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK e-mail: [email protected] 2 Paul Scherrer Institut, Würenlingen & Villigen, 5232 Villigen PSI, Switzerland 3 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA 4 SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 5 Astronomical Institute “Anton Pannekoek”, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands 6 Observatoire de Paris, LESIA, 92195 Meudon, France 7 Konkoly Observatory, 1525 Budapest, Hungary Received 30 April 2004 / Accepted 30 September 2004 Abstract. We present simultaneous ultraviolet and X-ray observations of the dMe-type flaring stars AT Mic, AU Mic, EV Lac, UV Cet and YZ CMi obtained with the XMM-Newton observatory. During 40 h of simultaneous observation we identify 13 flares which occurred in both wave bands. For the first time, a correlation between X-ray and ultraviolet flux for stellar flares has been observed. We find power-law relationships between these two wavelength bands for the flare luminosity increase, as well as for flare energies, with power-law exponents between 1 and 2. We also observe a correlation between the ultraviolet flare energy and the X-ray luminosity increase, which is in agreement with the Neupert effect and demonstrates that chromospheric evaporation is taking place. -
Ultraviolet and Green Light Cause Different Types of Damage in Rat Retina
Ultraviolet and Green Light Cause Different Types of Damage in Rat Retina Theo G. M. F. Gorgels? and Dirk van Norren*^ Purpose. To assess the influence of wavelength on retinal light damage in rat with funduscopy and histology and to determine a detailed action spectrum. Methods. Adult Long Evans rats were anesthetized, and small patches of retina were exposed to narrow-band irradiations in the range of 320 to 600 nm using a Xenon arc and Maxwellian view conditions. After 3 days, the retina was examined with funduscopy and prepared for light microscopy. Results. The dose that produced a change just visible in fundo was determined for each wavelength. This threshold dose for funduscopic damage increased monotonically from 0.35 J/cm2 at 320 nm to 1600 J/cm2 at 550 nm. At 600 nm, exposure of more than 3000J/cnr did not cause funduscopic damage. Morphologic changes in retinas exposed to threshold doses at wavelengths from 320 to 440 nm were similar and consisted of pyknosis of photorecep- tors. Retinas exposed to threshold doses of 470 to 550 nm had different morphologic appear- ances. Retinal pigment epithelial cells were swollen, and their melanin had lost the characteris- tic apical distribution. Some pyknosis was found in photoreceptors. Conclusions. Damage sensitivity in rat increases enormously from visible to ultraviolet wave- lengths. Compelling evidence is presented that two morphologically distinct types of damage occur in the rat retina, depending on the wavelength. Because two types also have been described in monkey, a remarkable similarity seems to exist across species. Invest Ophthahnol VisSci. -
Radar, Without Tears
Radar, without tears François Le Chevalier1 May 2017 Originally invented to facilitate maritime navigation and avoid icebergs, at the beginning of the last century, radar took off during the Second World War, especially for aerial surveillance and guidance from the ground or from aircraft. Since then, it has continued to expand its field of employment. 1 What is it, what is it for? Radar is used in the military field for surveillance, guidance and combat, and in the civilian area for navigation, obstacle avoidance, security, meteorology, and remote sensing. For some missions, it is irreplaceable: detecting flying objects or satellites, several hundred kilometers away, monitoring vehicles and convoys more than 100 kilometers round, making a complete picture of a planet through its atmosphere, measuring precipitations, marine currents and winds at long ranges, detecting buried objects or observing through walls – as many functions that no other sensor can provide, and whose utility is not questionable. Without radar, an aerial or terrestrial attack could remain hidden until the last minute, and the rain would come without warning to Roland–Garros and Wimbledon ... Curiously, to do this, the radar uses a physical phenomenon that nature hardly uses: radio waves, which are electromagnetic waves using frequencies between 1 MHz and 100 GHz – most radars operating with wavelength ( = c / f, being the wavelength, c the speed of light, 3.108 m/s, and f the frequency) between 300 m and 3 mm (actually, for most of them, between 1m and 1cm): wavelengths on a human scale ... Indeed, while the optical domain of electromagnetic waves, or even the ultraviolet and infrared domains, are widely used by animals, while the acoustic waves are also widely used by marine or terrestrial animals, there is practically no example of animal use of this vast part, known as "radioelectric", of the electromagnetic spectrum (some fish, Eigenmannia, are an exception to this rule, but they use frequencies on the order of 300 Hz, and therefore very much lower than the "radar" frequencies). -
Absorption of Light Energy Light, Energy, and Electron Structure SCIENTIFIC
Absorption of Light Energy Light, Energy, and Electron Structure SCIENTIFIC Introduction Why does the color of a copper chloride solution appear blue? As the white light hits the paint, which colors does the solution absorb and which colors does it transmit? In this activity students will observe the basic principles of absorption spectroscopy based on absorbance and transmittance of visible light. Concepts • Spectroscopy • Visible light spectrum • Absorbance and transmittance • Quantized electron energy levels Background The visible light spectrum (380−750 nm) is the light we are able to see. This spectrum is often referred to as “ROY G BIV” as a mnemonic device for the order of colors it produces. Violet has the shortest wavelength (about 400 nm) and red has the longest wavelength (about 650–700 nm). Many common chemical solutions can be used as filters to demonstrate the principles of absorption and transmittance of visible light in the electromagnetic spectrum. For example, copper(II) chloride (blue), ammonium dichromate (orange), iron(III) chloride (yellow), and potassium permanganate (red) are all different colors because they absorb different wave- lengths of visible light. In this demonstration, students will observe the principles of absorption spectroscopy using a variety of different colored solutions. Food coloring will be substituted for the orange and yellow chemical solutions mentioned above. Rare earth metal solutions, erbium and praseodymium chloride, will be used to illustrate line absorption spectra. Materials Copper(II) chloride solution, 1 M, 85 mL Diffraction grating, holographic, 14 cm × 14 cm Erbium chloride solution, 0.1 M, 50 mL Microchemistry solution bottle, 50 mL, 6 Potassium permanganate solution (KMnO4), 0.001 M, 275 mL Overhead projector and screen Praseodymium chloride solution, 0.1 M, 50 mL Red food dye Water, deionized Stir rod, glass Beaker, 250-mL Tape Black construction paper, 12 × 18, 2 sheets Yellow food dye Colored pencils Safety Precautions Copper(II) chloride solution is toxic by ingestion and inhalation. -
Estimating Fire Properties by Remote Sensing
Estimating Fire Properties by Remote Sensing1. Philip J. Riggan USDA Forest Service Pacific Southwest Research Station 4955 Canyon Crest Drive Riverside, CA 92507 909 680 1534 [email protected] James W. Hoffman Space Instruments, Inc. 4403 Manchester Avenue, Suite 203 Encinitas, CA 92024 760 944 7001 [email protected] James A. Brass NASA Ames Research Center Moffett Federal Airfield, CA 94035 650 604 5232 [email protected] Abstract---Contemporary knowledge of the role of fire in the TABLE OF CONTENTS global environment is limited by inadequate measurements of the extent and impact of individual fires. Observations by 1. INTRODUCTION operational polar-orbiting and geostationary satellites provide an 2. ESTIMATING FIRE PROPERTIES indication of fire occurrence but are ill-suited for estimating the 3. ESTIMATES FROM TWO CHANNELS temperature, area, or radiant emissions of active wildland and 4. MULTI-SPECTRAL FIRE IMAGING agricultural fires. Simulations here of synthetic remote sensing 5. APPLICATIONS FOR FIRE MONITORING pixels comprised of observed high resolution fire data together with ash or vegetation background demonstrate that fire properties including flame temperature, fractional area, and INTRODUCTION radiant-energy flux can best be estimated from concurrent radiance measurements at wavelengths near 1.6, 3.9, and 12 µm, More than 30,000 fire observations were recorded over central Successful observations at night may be made at scales to at Brazil during August 1999 by Advanced Very High Resolution least I km for the cluster of fire data simulated here. During the Radiometers operating aboard polarorbiting satellites of the U.S. daytime, uncertainty in the composition of the background and National Oceanic and Atmospheric Administration. -
25 Geometric Optics
CHAPTER 25 | GEOMETRIC OPTICS 887 25 GEOMETRIC OPTICS Figure 25.1 Image seen as a result of reflection of light on a plane smooth surface. (credit: NASA Goddard Photo and Video, via Flickr) Learning Objectives 25.1. The Ray Aspect of Light • List the ways by which light travels from a source to another location. 25.2. The Law of Reflection • Explain reflection of light from polished and rough surfaces. 25.3. The Law of Refraction • Determine the index of refraction, given the speed of light in a medium. 25.4. Total Internal Reflection • Explain the phenomenon of total internal reflection. • Describe the workings and uses of fiber optics. • Analyze the reason for the sparkle of diamonds. 25.5. Dispersion: The Rainbow and Prisms • Explain the phenomenon of dispersion and discuss its advantages and disadvantages. 25.6. Image Formation by Lenses • List the rules for ray tracking for thin lenses. • Illustrate the formation of images using the technique of ray tracking. • Determine power of a lens given the focal length. 25.7. Image Formation by Mirrors • Illustrate image formation in a flat mirror. • Explain with ray diagrams the formation of an image using spherical mirrors. • Determine focal length and magnification given radius of curvature, distance of object and image. Introduction to Geometric Optics Geometric Optics Light from this page or screen is formed into an image by the lens of your eye, much as the lens of the camera that made this photograph. Mirrors, like lenses, can also form images that in turn are captured by your eye. 888 CHAPTER 25 | GEOMETRIC OPTICS Our lives are filled with light. -
Band Radar Models FR-2115-B/2125-B/2155-B*/2135S-B
R BlackBox type (with custom monitor) X/S – band Radar Models FR-2115-B/2125-B/2155-B*/2135S-B I 12, 25 and 50* kW T/R up X-band, 30 kW I Dual-radar/full function remote S-band inter-switching I SXGA PC monitor either CRT or color I New powerful processor with LCD high-speed, high-density gate array and I Optional ARP-26 Automatic Radar sophisticated software Plotting Aid (ARPA) on 40 targets I New cast aluminum scanner gearbox I Furuno's exclusive chart/radar overlay and new series of streamlined radiators technique by optional RP-26 VideoPlotter I Shared monitor utilization of Radar and I Easy to create radar maps PC systems with custom PC monitor switching system The BlackBox radar system FR-2115-B, FR-2125-B, FR-2155-B* and FR-2135S-B are custom configured by adding a user’s favorite display to the blackbox radar package. The package is based on a Furuno standard radar used in the FR-21x5-B series with (FURUNO) monitor which is designed to comply with IMO Res MSC.64(67) Annex 4 for shipborne radar and A.823 (19) for ARPA performance. The display unit may be selected from virtually any size of multi-sync PC monitor, either a CRT screen or flat panel LCD display. The blackbox radar system is suitable for various ships which require no specific type approval as a SOLAS compliant radar. The radar is available in a variety of configurations: 12, 25, 30 and 50* kW output, short or long antenna radiator, 24 or 42 rpm scanner, with standard Electronic Plotting Aid (EPA) and optional Automatic Radar Plotting Aid (ARPA).