Exploring the Similarities and Dissimilarities of Identical Twins in Theatrical Solo Performance
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Adult Contemporary Radio at the End of the Twentieth Century
University of Kentucky UKnowledge Theses and Dissertations--Music Music 2019 Gender, Politics, Market Segmentation, and Taste: Adult Contemporary Radio at the End of the Twentieth Century Saesha Senger University of Kentucky, [email protected] Digital Object Identifier: https://doi.org/10.13023/etd.2020.011 Right click to open a feedback form in a new tab to let us know how this document benefits ou.y Recommended Citation Senger, Saesha, "Gender, Politics, Market Segmentation, and Taste: Adult Contemporary Radio at the End of the Twentieth Century" (2019). Theses and Dissertations--Music. 150. https://uknowledge.uky.edu/music_etds/150 This Doctoral Dissertation is brought to you for free and open access by the Music at UKnowledge. It has been accepted for inclusion in Theses and Dissertations--Music by an authorized administrator of UKnowledge. For more information, please contact [email protected]. STUDENT AGREEMENT: I represent that my thesis or dissertation and abstract are my original work. Proper attribution has been given to all outside sources. I understand that I am solely responsible for obtaining any needed copyright permissions. I have obtained needed written permission statement(s) from the owner(s) of each third-party copyrighted matter to be included in my work, allowing electronic distribution (if such use is not permitted by the fair use doctrine) which will be submitted to UKnowledge as Additional File. I hereby grant to The University of Kentucky and its agents the irrevocable, non-exclusive, and royalty-free license to archive and make accessible my work in whole or in part in all forms of media, now or hereafter known. -
Abstract Observation Overview Nustar HXR Imaging Microflare
Imaging and Spectroscopy of Six NuSTAR MicroFlares SH11D-2898 Contact: J. Duncan1, L. Glesener1, I. Hannah2, D. Smith3, B. Grefenstette4 (1Univ, of Minnesota; 2Univ. of Glasgow; 3UC Santa Cruz; 4California Institute of Technology) [email protected] Abstract MicroFlare Time Evolution Hard X-ray (HXR) emission in solar flares originates from regions of high temperature plasma, as well as from non-thermal particle populations [1]. Both of these sources of HXR radiation make solar observation in this band important for study of • NuSTAR observed 6 MicroFlares during this observation. Time evolution is shown in both raw and normalized NuSTAR flare energetics. NuSTAR is the first HXR telescope with direct focusing optics, giving it a dramatic increase in sensitivity countsLivetime acrosscorrection several applied energy ranges for each flare. Counts are livetime-corrected (NuSTAR livetime ranged from 1-14%). Livetime correction applied over previous indirect imaging methods. Here we present NuSTAR observation of six microflares from one solar active Livetime correction applied 5 5 6 5×10 4×10 2.0 10 5 × 4×10 5 region during a period of several hours on May 29th, 2018. In conjunction with simultaneous data from SDO/AIA, data 3×10 5 2-4 keV 2-4 keV 6 3×10 1.5 10 Orbit1, Flare B 4-6 keV 2×105 4-6 keV × 5 counts 2 10 2-4 keV × Orbit1, Flare A 6-8 keV counts Orbit1, Flare C 6-8 keV from this observation has been used to create flare-time images showing the spatial extent of HXR emission. Additionally, 5 5 1 10 1×10 8-10 keV × 8-10 keV 6 4-6 keV 1.0×10 (Left) Estimated GOES A5 flare, with 0 0 1.2 1.2 16:07 16:08 16:09 16:10 16:11 16:46 16:48 16:50 16:52 16:54 NuSTAR lightcurves show time evolution in four different HXR energy ranges over the course of each flare. -
Build a Spacecraft Activity
UAMN Virtual Family Day: Amazing Earth Build a Spacecraft SMAP satellite. Image: NASA. Discover how scientists study Earth from above! Scientists use satellites and spacecraft to study the Earth from outer space. They take pictures of Earth's surface and measure cloud cover, sea levels, glacier movements, and more. Materials Needed: Paper, pencil, craft materials (small recycled boxes, cardboard pieces, paperclips, toothpicks, popsicle sticks, straws, cotton balls, yarn, etc. You can use whatever supplies you have!), fastening materials (glue, tape, rubber bands, string, etc.) Instructions: Step 1: Decide what you want your spacecraft to study. Will it take pictures of clouds? Track forest fires? Measure rainfall? Be creative! Step 2: Design your spacecraft. Draw a picture of what your spacecraft will look like. It will need these parts: Container: To hold everything together. Power Source: To create electricity; solar panels, batteries, etc. Scientific Instruments: This is the why you launched your satellite in the first place! Instruments could include cameras, particle collectors, or magnometers. Communication Device: To relay information back to Earth. Image: NASA SpacePlace. Orientation Finder: A sun or star tracker to show where the spacecraft is pointed. Step 3: Build your spacecraft! Use any craft materials you have available. Let your imagination go wild. Step 4: Your spacecraft will need to survive launching into orbit. Test your spacecraft by gently shaking or spinning it. How well did it hold together? Adjust your design and try again! Model spacecraft examples. Courtesy NASA SpacePlace. Activity adapted from NASA SpacePlace: spaceplace.nasa.gov/build-a-spacecraft/en/ UAMN Virtual Early Explorers: Amazing Earth Studying Earth From Above NASA is best known for exploring outer space, but it also conducts many missions to investigate Earth from above. -
Nustar and XMM-Newton Observations of the Hard X-Ray Spectrum of Centaurus A
Downloaded from orbit.dtu.dk on: Sep 27, 2021 NuSTAR and XMM-Newton Observations of the Hard X-Ray Spectrum of Centaurus A Fürst, F.; Müller, C.; Madsen, K. K.; Lanz, L.; Rivers, E.; Brightman, M.; Arevalo, P.; Balokovi, M.; Beuchert, T.; Boggs, S. E. Total number of authors: 31 Published in: The Astrophysical Journal Link to article, DOI: 10.3847/0004-637X/819/2/150 Publication date: 2016 Document Version Publisher's PDF, also known as Version of record Link back to DTU Orbit Citation (APA): Fürst, F., Müller, C., Madsen, K. K., Lanz, L., Rivers, E., Brightman, M., Arevalo, P., Balokovi, M., Beuchert, T., Boggs, S. E., Christensen, F. E., Craig, W. W., Dauser, T., Farrah, D., Graefe, C., Hailey, C. J., Harrison, F. A., Kadler, M., King, A., ... Zhang, W. W. (2016). NuSTAR and XMM-Newton Observations of the Hard X-Ray Spectrum of Centaurus A. The Astrophysical Journal, 819(2), [150]. https://doi.org/10.3847/0004- 637X/819/2/150 General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Users may download and print one copy of any publication from the public portal for the purpose of private study or research. You may not further distribute the material or use it for any profit-making activity or commercial gain You may freely distribute the URL identifying the publication in the public portal If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. -
Physics of the Cosmic Microwave Background Anisotropy∗
Physics of the cosmic microwave background anisotropy∗ Martin Bucher Laboratoire APC, Universit´eParis 7/CNRS B^atiment Condorcet, Case 7020 75205 Paris Cedex 13, France [email protected] and Astrophysics and Cosmology Research Unit School of Mathematics, Statistics and Computer Science University of KwaZulu-Natal Durban 4041, South Africa January 20, 2015 Abstract Observations of the cosmic microwave background (CMB), especially of its frequency spectrum and its anisotropies, both in temperature and in polarization, have played a key role in the development of modern cosmology and our understanding of the very early universe. We review the underlying physics of the CMB and how the primordial temperature and polarization anisotropies were imprinted. Possibilities for distinguish- ing competing cosmological models are emphasized. The current status of CMB ex- periments and experimental techniques with an emphasis toward future observations, particularly in polarization, is reviewed. The physics of foreground emissions, especially of polarized dust, is discussed in detail, since this area is likely to become crucial for measurements of the B modes of the CMB polarization at ever greater sensitivity. arXiv:1501.04288v1 [astro-ph.CO] 18 Jan 2015 1This article is to be published also in the book \One Hundred Years of General Relativity: From Genesis and Empirical Foundations to Gravitational Waves, Cosmology and Quantum Gravity," edited by Wei-Tou Ni (World Scientific, Singapore, 2015) as well as in Int. J. Mod. Phys. D (in press). -
GALEX: Galaxy Evolution Explorer
GALEX: Galaxy Evolution Explorer Barry F. Madore Carnegie Observatories, Pasadena CA 91101 Abstract. We review recent scientific results from the Galaxy Evolution Explorer with special emphasis on star formation in nearby resolved galaxies. INTRODUCTION The Satellite The Galaxy Evolution Explorer (GALEX) is a NASA Small Explorer class mission. It consists of a 50 cm-diameter, modified Ritchey-Chrétien telescope with four operating modes: Far-UV (FUV) and Near-UV (NUV) imaging, and FUV and NUV spectroscopy. Æ The telescope has a 3-m focal length and has Al-MgF2 coatings. The field of view is 1.2 circular. An optics wheel can position a CaF2 imaging window, a CaF2 transmission grism, or a fully opaque mask in the beam. Spectroscopic observations are obtained at multiple grism-sky dispersion angles, so as to mitigate spectral overlap effects. The FUV (1528Å: 1344-1786Å) and NUV (2271Å: 1771-2831Å) imagers can be operated one at a time or simultaneously using a dichroic beam splitter. The detector system encorporates sealed-tube microchannel-plate detectors. The FUV detector is preceded by a blue-edge filter that blocks the night-side airglow lines of OI1304, 1356, and Lyα. The NUV detector is preceded by a red blocking filter/fold mirror, which produces a sharper long-wavelength cutoff than the detector CsTe photocathode and thereby reduces both zodiacal light background and optical contamination. The peak quantum efficiency of the detector is 12% (FUV) and 8% (NUV). The detectors are linear up to a local (stellar) count-rate of 100 (FUV), 400 (NUV) cps, which corresponds to mAB 14 15. -
Songs by Title
16,341 (11-2020) (Title-Artist) Songs by Title 16,341 (11-2020) (Title-Artist) Title Artist Title Artist (I Wanna Be) Your Adams, Bryan (Medley) Little Ole Cuddy, Shawn Underwear Wine Drinker Me & (Medley) 70's Estefan, Gloria Welcome Home & 'Moment' (Part 3) Walk Right Back (Medley) Abba 2017 De Toppers, The (Medley) Maggie May Stewart, Rod (Medley) Are You Jackson, Alan & Hot Legs & Da Ya Washed In The Blood Think I'm Sexy & I'll Fly Away (Medley) Pure Love De Toppers, The (Medley) Beatles Darin, Bobby (Medley) Queen (Part De Toppers, The (Live Remix) 2) (Medley) Bohemian Queen (Medley) Rhythm Is Estefan, Gloria & Rhapsody & Killer Gonna Get You & 1- Miami Sound Queen & The March 2-3 Machine Of The Black Queen (Medley) Rick Astley De Toppers, The (Live) (Medley) Secrets Mud (Medley) Burning Survivor That You Keep & Cat Heart & Eye Of The Crept In & Tiger Feet Tiger (Down 3 (Medley) Stand By Wynette, Tammy Semitones) Your Man & D-I-V-O- (Medley) Charley English, Michael R-C-E Pride (Medley) Stars Stars On 45 (Medley) Elton John De Toppers, The Sisters (Andrews (Medley) Full Monty (Duets) Williams, Sisters) Robbie & Tom Jones (Medley) Tainted Pussycat Dolls (Medley) Generation Dalida Love + Where Did 78 (French) Our Love Go (Medley) George De Toppers, The (Medley) Teddy Bear Richard, Cliff Michael, Wham (Live) & Too Much (Medley) Give Me Benson, George (Medley) Trini Lopez De Toppers, The The Night & Never (Live) Give Up On A Good (Medley) We Love De Toppers, The Thing The 90 S (Medley) Gold & Only Spandau Ballet (Medley) Y.M.C.A. -
Search for the Common Power Law Spectrum in Parker Solar Probe's IS
Search for the Common Power Law Spectrum in Parker Solar Probe’s IS☉IS-EPILo Data Asher Merrill Advisors: Dr. Jonathan Niehof and Dr. Nathan Schwadron Abstract I investigate the first year and a half of Parker Solar Probe's data to Analysis find evidence of the common power law spectrum of ions proposed by Gloeckler et. al. (2000) within 0.3 AU. I find weak evidence to suggest the existence of a common spectrum of protons from ~60 keV to 200 keV Event Selection inside the region being studied. Further work is required to elucidate the It is necessary to identify solar wind events in order to phenomena in this region that determine the shape of the solar wind have significant counting statistics above background. Solar spectra. wind events were identified by eye. Fitting Fisk & Gloeckler (2006) suggest a model of compressional acceleration in solar wind turbulence that predicts a Introduction functional dependence of flux on energy as shown above. For each event, the flux was averaged along time, and then a fit to The Advanced Composition Explorer and the Ulysses spacecraft this model was applied between ~60 keV and 200 keV, revealed the presence of a common power-law spectrum of ions in the depending on data source. solar wind, the shape of which is independent of solar activity. The highest energy particles in this distribution are a direct interest to human affairs as Analysis of variance of magnetic field vs radial distance. they can serve as the seed population for large, destructive events that can Event Type Analysis Schwadron et. -
Interstellar Probe to Explore the Sun's Influences Propagating Beyond The
Interstellar Probe to Explore the Sun’s Influences Propagating Beyond the Heliosphere Parisa Mostafavi�, G. P. Zank�, D. J. McComas�, L. Burgala4, J. Richardson5, G. Webb2, E. Provornikova1, P. Brandt1 1. Johns Hopkins University Applied Physics Lab, 2. University of Alabama in Huntsville, 3. Princeton University, 4. NASA Goddard Space Flight Center, 5. Massachusetts Institute of Technology Introduction The heliosphere is controlled by the motion of the Sun through the interstellar space. Although humankind has explored the region of space about the Earth quite extensively, the distant heliosphere beyond the planets remains almost entirely unexplored with only the two Voyager spacecraft, New Horizons, and the early Pioneer 10 and 11 spacecraft returning the in-situ observations of this most distant region. Moreover, remote observations of energetic neutral atoms (ENAs) from the Interstellar Boundary Explorer (IBEX) at 1 au and Cassini/INCA at 10 au revealed interesting structure related to the interstellar medium. Voyager 1 and 2 crossed the heliopause in 2012 and 2018, respectively, and are both continue to make in-situ measurements of the very local interstellar medium (VLISM; the nearby region of the LISM affected by physical processes associated with the heliosphere) for the first time. Voyager 1 and 2 have identified and partially answered many interesting questions about the outer heliosphere and the VLISM while raising numerous new questions, many of which have profound implications for the detailed structure and properties of the heliosphere and our place in the galaxy. One particularly interesting topic is the influence of the large-scale disturbances and small-scale turbulences generated by the dynamical Sun on the VLISM. -
Interstellar Heliospheric Probe/Heliospheric Boundary Explorer Mission—A Mission to the Outermost Boundaries of the Solar System
Exp Astron (2009) 24:9–46 DOI 10.1007/s10686-008-9134-5 ORIGINAL ARTICLE Interstellar heliospheric probe/heliospheric boundary explorer mission—a mission to the outermost boundaries of the solar system Robert F. Wimmer-Schweingruber · Ralph McNutt · Nathan A. Schwadron · Priscilla C. Frisch · Mike Gruntman · Peter Wurz · Eino Valtonen · The IHP/HEX Team Received: 29 November 2007 / Accepted: 11 December 2008 / Published online: 10 March 2009 © Springer Science + Business Media B.V. 2009 Abstract The Sun, driving a supersonic solar wind, cuts out of the local interstellar medium a giant plasma bubble, the heliosphere. ESA, jointly with NASA, has had an important role in the development of our current under- standing of the Suns immediate neighborhood. Ulysses is the only spacecraft exploring the third, out-of-ecliptic dimension, while SOHO has allowed us to better understand the influence of the Sun and to image the glow of The IHP/HEX Team. See list at end of paper. R. F. Wimmer-Schweingruber (B) Institute for Experimental and Applied Physics, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 11, 24098 Kiel, Germany e-mail: [email protected] R. McNutt Applied Physics Laboratory, John’s Hopkins University, Laurel, MD, USA N. A. Schwadron Department of Astronomy, Boston University, Boston, MA, USA P. C. Frisch University of Chicago, Chicago, USA M. Gruntman University of Southern California, Los Angeles, USA P. Wurz Physikalisches Institut, University of Bern, Bern, Switzerland E. Valtonen University of Turku, Turku, Finland 10 Exp Astron (2009) 24:9–46 interstellar matter in the heliosphere. Voyager 1 has recently encountered the innermost boundary of this plasma bubble, the termination shock, and is returning exciting yet puzzling data of this remote region. -
A Quality Constrained Themis Daytime Infrared Global Mosaic
47th Lunar and Planetary Science Conference (2016) 2326.pdf A QUALITY CONSTRAINED THEMIS DAYTIME INFRARED GLOBAL MOSAIC. J. R. Hill1 and P. R. Christensen1; 1School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-6305 ([email protected]). Introduction: The 2001 Mars Odyssey spacecraft registration is rarely perfect, offsets are usually small entered orbit around Mars on October 24th, 2001 and relative to the 100 m/pixel resolution of the mosaic. is the longest-operating spacecraft in the history of However, in cases where the Hill et al. [4] daytime Mars exploration. The Thermal Emission Imaging Sys- global mosaic contained images with large offsets (due tem (THEMIS) has been acquiring observations in both to extrapolations over gaps in spacecraft position and infrared and visible wavelengths since the beginning of pointing telemetry, etc), the images were removed and science operations in February 2002. While previously replaced by images with better geometry data. An ex- assembled THEMIS global mosaics have focused only ample of this correction is shown in Figure 1. on spatial coverage, this new daytime global infrared Noisy Images Replaced. The Hill et al. [4] daytime mosaic has been optimized to include only the best global mosaic also contained numerous images with quality images acquired over the first fourteen years of significant noise resulting from low surface tempera- the mission while still maintaining global coverage. tures, atmospheric effects, etc. These poor-quality im- Background: The THEMIS instrument consists of ages were identified and replaced by higher-quality two multispectral imaging subsystems; a ten-band images, where possible, as demonstrated in Figure 2. -
THE LIVING YEARS 1 Timbaland
Artist - Track Count mike & the mechanics - THE LIVING YEARS 1 timbaland - nelly furtado - justin - GIVE IT TO ME 1 wet wet wet - LOVE IS ALL AROUND 1 justin timberlake - MY LOVE 1 john mayer - WAITING ON THE WORLD TO CHANGE 1 duran duran - I DON'T WANT YOUR LOVE 1 tom walker - LEAVE A LIGHT ON 1 a fine frenzy - ALMOST LOVER 1 mariah carey - VISION OF LOVE 1 aura dione - SOMETHING FROM NOTHING 1 linkin park - NEW DIVIDE (from Transformers 2) 1 phil collins - GOING BACK 1 keane - SILENCED BY NIGHT 1 sigala - EASY LOVE 1 murray head - ONE NIGHT IN BANGKOK 1 celine dion - ONE HEART 1 reporter milan - STAJERSKA 1 michael jackson - siedah garrett - I JUST CAN'T STOP LOVING YOU 1 martin garrix feat usher - DON'T LOOK DOWN 1 k'naan - WAVIN' FLAG (OFFICIAL 2010 WORLD CUP SONG) 1 jennifer lopez & pitbull - DANCE AGAIN 1 maroon 5 - THIS SUMMER'S GONNA HURT 1 happy mondays - STEP ON 1 abc - THE NIGHT YOU MURDERED LOVE 1 heart - ALL I WANNA DO IS MAKING LOVE 1 huey lewis & the news - STUCK WITH YOU 1 ultravox - VIENNA 1 queen - HAMMER TO FALL 1 stock aitken waterman - ROADBLOCK 1 yazoo - ONLY YOU 1 billy idol - REBEL YELL 1 ashford & simpson - SOLID 1 loverboy - HEAVEN IN YOUR EYES 1 kaoma - LAMBADA 1 david guetta/sia - LET'S LOVE 1 rita ora/gunna - BIG 1 you me at six - ADRENALINE 1 shakira - UNDERNEATH YOUR CLOTHES 1 gwen stefani - LET ME REINTRODUCE MYSELF 1 cado - VSE, KAR JE TAM 1 atomic kitten - WHOLE AGAIN 1 dionne bromfield feat lil twist - FOOLIN 1 macy gray - STILL 1 sixpence none the richer - THERE SHE GOES 1 maraaya - DREVO 1 will young - FRIDAY'S CHILD 1 christina aguilera - WHAT A GIRL WANTS 1 jan plestenjak - lara - SOBA 102 1 barry white - YOU'RE THE FIRST THE LAST MY EVERYTHING 1 parni valjak - PROKLETA NEDELJA 1 pitbull - GIVE ME EVERYTHING TONIGHT 1 the champs - TEQUILA 1 colonia - ZA TVOJE SNENE OCI 1 nick kamen - I PROMISED MYSELF 1 gina g.