REVERSIBLE COLOR MODIFICATION of BLUE ZIRCON by LONG-WAVE ULTRAVIOLET RADIATION Nathan D
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
HIGHLIGHTS and BREAKTHROUGHS Sapphire, A
1 HIGHLIGHTS AND BREAKTHROUGHS 2 Sapphire, a not so simple gemstone 3 F. LIN SUTHERLAND1* 4 1Geoscience, Australian Museum, 1 William Street, Sydney, NSW 2010, Australia. 5 *E-mail: [email protected] 6 Abstract: Sapphire is a gemstone of considerable reach and is much researched. It still delivers scientific surprises, as exemplified by a 7 recent paper in American Mineralogist that re-interprets the origin of needle-like rutile inclusions that form “silk” in sapphires. 8 Understanding of variations in sapphire genesis continues to expand. Keywords: Sapphire, inclusions, trace elements, genesis 9 Sapphire as a gem variety of corundum has wide use in the gem trade as one of the more historically valuable colored gem stones 10 (CGS) and is mined from a great variety of continental gem deposits across the world. A masterly compendium on this gemstone and its 11 ramifications is recently available (Hughes 2017). As a gem, sapphire ranges through all the colors of corundum, except where 12 sufficient Cr enters its α-alumina crystal structure and causes the red color of the variety ruby. Sapphire, as a key pillar in a wide 13 economic network of gem enhancing treatments, jewelry and other manufacturing enterprises, has elicited numerous scientific and 14 gemological enquiries into its internal nature and natural genesis and subsequent treatments. A further use of sapphire as a synthetic 15 material with a great variety of purposes also has triggered a proliferation of detailed studies on its growth, properties and other element 16 substitutional effects (Dobrovinski et al. 2009). Even with this vast range of studies, this apparently simple gemstone still yields 17 controversies and breakthroughs in understanding its genetic formation. -
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. -
Compilation of Reported Sapphire Occurrences in Montana
Report of Investigation 23 Compilation of Reported Sapphire Occurrences in Montana Richard B. Berg 2015 Cover photo by Richard Berg. Sapphires (very pale green and colorless) concentrated by panning. The small red grains are garnets, commonly found with sapphires in western Montana, and the black sand is mainly magnetite. Compilation of Reported Sapphire Occurrences, RI 23 Compilation of Reported Sapphire Occurrences in Montana Richard B. Berg Montana Bureau of Mines and Geology MBMG Report of Investigation 23 2015 i Compilation of Reported Sapphire Occurrences, RI 23 TABLE OF CONTENTS Introduction ............................................................................................................................1 Descriptions of Occurrences ..................................................................................................7 Selected Bibliography of Articles on Montana Sapphires ................................................... 75 General Montana ............................................................................................................75 Yogo ................................................................................................................................ 75 Southwestern Montana Alluvial Deposits........................................................................ 76 Specifi cally Rock Creek sapphire district ........................................................................ 76 Specifi cally Dry Cottonwood Creek deposit and the Butte area .................................... -
Do Zircon and Monazite Consistently Record Garnet Growth in High-Grade Rocks?
Geophysical Research Abstracts Vol. 21, EGU2019-5915-1, 2019 EGU General Assembly 2019 © Author(s) 2019. CC Attribution 4.0 license. Do zircon and monazite consistently record garnet growth in high-grade rocks? Lorraine Tual (1,2), Ellen Kooijman (1), Melanie Schmitt (1), and Matthijs Smit (2) (1) Department of Geosciences, Swedish Museum of Natural History, Stockholm, Sweden ([email protected]), (2) Department of Earth, Ocean, and Atmospheric Sciences, University of British Columbia, Vancouver, Canada Garnet Lu-Hf ages are used to monitor the systematics of rare earth elements (REE) and age record in accessory minerals. We performed in-situ LA-(MC-)ICPMS U-(Th-)Pb dating and REE analysis on zircon and monazite in two contrasting high-grade rock samples: dry felsic granulite xenoliths from the Pamir, Tajikistan and fluid-rich, ultrahigh-pressure (UHP) migmatites from the Western Gneiss Region (WGR), Norway. In parallel, garnet from the same samples were subjected to REE analysis and dated by Lu-Hf. The datasets are compared to see whether, and to what extent, REE systematics in accessory phases can be correlated with garnet growth. Garnet in the hydrous UHP migmatite contains abundant zircon and monazite inclusions. The Gd/Yb values and U-(Th-)Pb ages of these inclusions show significant dispersion and do not systematically correlate. Highest Gd/Yb values occur at 420-410 and c. 420 Ma for monazite and zircon, respectively. Garnet in this rock yielded a Lu-Hf garnet bulk age of c. 422 Ma. The data obtained from the dry Pamir xenoliths show a different pattern. Accessory minerals grew in distinct pulses between 50 and 11 Ma, and indicate garnet growth between 42-37 Ma [1]. -
Radiohalos and Diamonds: Are Diamonds Really for Ever?
The Proceedings of the International Conference on Creationism Volume 6 Print Reference: Pages 323-334 Article 28 2008 Radiohalos and Diamonds: Are Diamonds Really for Ever? Mark H. Armitage Andrew A. Snelling Answers in Genesis Follow this and additional works at: https://digitalcommons.cedarville.edu/icc_proceedings DigitalCommons@Cedarville provides a publication platform for fully open access journals, which means that all articles are available on the Internet to all users immediately upon publication. However, the opinions and sentiments expressed by the authors of articles published in our journals do not necessarily indicate the endorsement or reflect the views of DigitalCommons@Cedarville, the Centennial Library, or Cedarville University and its employees. The authors are solely responsible for the content of their work. Please address questions to [email protected]. Browse the contents of this volume of The Proceedings of the International Conference on Creationism. Recommended Citation Armitage, Mark H. and Snelling, Andrew A. (2008) "Radiohalos and Diamonds: Are Diamonds Really for Ever?," The Proceedings of the International Conference on Creationism: Vol. 6 , Article 28. Available at: https://digitalcommons.cedarville.edu/icc_proceedings/vol6/iss1/28 In A. A. Snelling (Ed.) (2008). Proceedings of the Sixth International Conference on Creationism (pp. 323–334). Pittsburgh, PA: Creation Science Fellowship and Dallas, TX: Institute for Creation Research. Radiohalos and Diamonds: Are Diamonds Really for Ever? Mark H. Armitage, M.S. Ed.S., Microspecialist, 587 Ventu Park Road 304, Thousand Oaks, CA 91320 Andrew A. Snelling, Ph.D., Director of Research, Answers in Genesis, P.O. Box 510, Hebron, KY 41048 Abstract Radiohalos were first reported in diamonds more than a decade ago. -
Murostar-Katalog-2018-2019.Pdf
Material B2B Großhandel für Piercing- und Tattoo- B2B Wholesale for body piercing and Unsere Qualität ist Ihre Zufriedenheit Our quality is your satisfaction About Us studios, sowie Schmuck- und Juwelier- tattoo studios as well as jewelry stores vertriebe Oberste Priorität hat bei uns die reibungslose Abwicklung Our top priority is to provide a smooth transaction and fast Titan Produkte entsprechen dem Grad 23 (Ti6AL 4V Eli) und Titanium products correspond to titanium grade 23 (Ti6Al und schnelle Lieferung Ihrer Ware. Daher verlassen ca. 95 % delivery. Therefore, approximately 95% of all orders are sind generell hochglanzpoliert. Sterilisierbar. 4V Eli) and are generally high polished. For sterilization. aller Aufträge unser Lager noch am selben Tag. shipped out on the same day. Black Titan besteht grundsätzlich aus Titan Grad 23 (Ti6AL Black Titanium is composed of titanium grade 23 (Ti6Al 4V Unser dynamisches, kundenorientiertes Team sowie ausge- Our dynamic, customer-oriented team and excellent expe- 4V Eli) und ist zusätzlich mit einer PVD Titanium Beschich- Eli) and is additionally equipped with a PVD Black Titanium zeichnete Erfahrungswerte garantieren Ihnen einen hervor- rience guarantee excellent service and expert advice. tung geschwärzt. Sterilisierbar. Coating. For sterilization. ragenden Service und kompetente Beratung. Steel Schmuck besteht grundsätzlich aus Chirurgenstahl Steel jewelry is composed of 316L Surgical Steel and is also Sie bestellen schnell und unkompliziert online, telefo- Your order can be placed quickly and easily online, by 316L und ist ebenfalls hochglanzpoliert. Sterilisierbar. high polished. For sterilization. nisch, per Fax oder Email mittels unseres einfachen Ex- phone, fax or email using our simple Express Number press-Nummern-Systems ohne Angabe von Farb- oder Grö- System only without providing colors or sizes. -
Xcited from Its Ground State to an Electronic Excited State
Chapter 1: UV-Visible & Fluorescence Spectroscopy This chapter covers two methods of spectroscopic characterization: UV-Visible absorption spectroscopy (often abbreviated as UV-Vis) and fluorescence emission spectroscopy. These two methods are measured over the same range of wavelengths, but are caused by two different phenomena. In both cases, the wavelengths used are the near-ultraviolet range (200 to 400 nm) and the visible range (400 to 750 nm). These two regions are typically considered together as a single category because there is a common physical basis for the behavior of a compound in both UV and visible light. UV-Vis measures the absorption of light in this range, while fluorescence measures the light emitted by a sample in this range after absorbing light at a higher energy than it is emitting. 1.1 UV-Visible Spectroscopy UV-Visible absorption spectroscopy involves measuring the absorbance of light by a compound as a function of wavelength in the UV-visible range. When a molecule absorbs a photon of UV-Vis light, the molecule is excited from its ground state to an electronic excited state. In other words, an electron is promoted from the HOMO (Highest-energy Occupied Molecular Orbital) of the molecule to the LUMO (Lowest-energy Unoccupied Molecular Orbital) of the molecule. The HOMO is commonly a π orbital of a conjugated functional group and the LUMO is commonly a π* orbital of the conjugated functional group. The smaller the energy difference between HOMO and LUMO, the less energy is needed and the longer the wavelength that will be absorbed (Figure 1-1). -
Learn More About X-Rays, CT Scans and Mris (Pdf)
What is the difference between X-Rays, CT Scans, and MRIs? X-Rays are a form of electromagnetic radiation, like light. They are less energetic than gamma rays, and more energetic than ultraviolet light. Because they pass easily through soft tissue, like organs and muscles, but not so easily through hard tissue like bones and teeth, we are most familiar with them being used to look at skeletal structures. Sometimes a person ingests or has injected an X-ray opaque fluid that will fill a space of interest for X-ray imaging. This is called an angiogram. A nuclear scan uses an injected gamma ray emitting substance that accumulates in the organ of interest and a special camera records the gamma rays. A CT Scan is usually a series of X-rays taken from different directions that are then assembled into a three dimensional model of the subject in a computer. CT stands for computed tomography, and tomography means a picture of a slice. Where an X-ray may show edges of soft tissues all stacked on top of each other, the computer in a CT scan can figure out how those edges relate to each other in depth, and so the image has much more soft tissue usability. Another kind of CT scan uses positrons. I have to mention this because positrons are antimatter electrons (Yes, antimatter does exist and it is useful!) In Positon Emission Tomography (PET) a positron emitting radionuclide (radioactive material) is attached to a metabolically useful molecule. This is introduced to the tissue, and as emitted positrons decompose they emit gamma rays which can be traced by the machine and computer back to their points of origin, and an image is formed. -
24 Electromagnetic Waves.Pdf
CHAPTER 24 | ELECTROMAGNETIC WAVES 861 24 ELECTROMAGNETIC WAVES Figure 24.1 Human eyes detect these orange “sea goldie” fish swimming over a coral reef in the blue waters of the Gulf of Eilat (Red Sea) using visible light. (credit: Daviddarom, Wikimedia Commons) Learning Objectives 24.1. Maxwell’s Equations: Electromagnetic Waves Predicted and Observed • Restate Maxwell’s equations. 24.2. Production of Electromagnetic Waves • Describe the electric and magnetic waves as they move out from a source, such as an AC generator. • Explain the mathematical relationship between the magnetic field strength and the electrical field strength. • Calculate the maximum strength of the magnetic field in an electromagnetic wave, given the maximum electric field strength. 24.3. The Electromagnetic Spectrum • List three “rules of thumb” that apply to the different frequencies along the electromagnetic spectrum. • Explain why the higher the frequency, the shorter the wavelength of an electromagnetic wave. • Draw a simplified electromagnetic spectrum, indicating the relative positions, frequencies, and spacing of the different types of radiation bands. • List and explain the different methods by which electromagnetic waves are produced across the spectrum. 24.4. Energy in Electromagnetic Waves • Explain how the energy and amplitude of an electromagnetic wave are related. • Given its power output and the heating area, calculate the intensity of a microwave oven’s electromagnetic field, as well as its peak electric and magnetic field strengths Introduction to Electromagnetic Waves The beauty of a coral reef, the warm radiance of sunshine, the sting of sunburn, the X-ray revealing a broken bone, even microwave popcorn—all are brought to us by electromagnetic waves.