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ASU - GLG - 485
Chondrules and CAI OverviewWhat are they? Why are they important?Calcium-Aluminum InclusionsCAI- (also called refractory inclusions) are important because they are the first solar system solids! Evidence: Mineralogy (condensation diagram) Age (
ASU - GLG - 485
Fine-Grained Rims in Carbonaceous ChondritesOverview Unequilibrated Carbonaceous & Ordinary chondrites Texturally primitive (types 2 & 3) Primary processes Solar nebula condensation Secondary processes (CCs) FeO-rich olivine formation CAI
ASU - GLG - 485
PergamonGeochimica et Cosmochimica Acta, Vol. 60, No. 12, pp. 2243-2256. 1996 Copyright 0 1996 Elsevier Science Ltd Printed in the USA. All rights reserved 0016.7037/96 $15.00 + .OOPI1 SOO16-7037( 96)00073-7The compositionalclassificationof
ASU - GLG - 485
Stable isotopes in meteorites29 March 2004Announcements Turn in HW #2 Turn in outline Pick-up take-home midterm (due next Monday) Next week Reading group 3 Next week Guest lecture on pre-solar materialsIll e-mail an overview article and post
ASU - GLG - 485
Presolar Grains in MeteoritesProbes of the Early Solar System10Abundance Normalized to CICM2 Chondrites10.1Murchison Murry0.01Xe-P6 in diamond Graphite Xe-P3 Xe-P1 Diamond (Xe-HL) Ne-E(H)* SiC3CI-Normalized AbundancesCM2 Chondrites
ASU - GLG - 485
Introduction to MeteoritesIntroduction to MeteoritesHow common are they? Where do they come from? How different is one from another?How common?~40,000 metric tons(per year) of extraterrestrial material reaches the Earths surface. Most of the ma
ASU - GLG - 485
Isotopes in Meteorites and CosmochemistryBackground and Introduction to Radiogenic Isotopes 8 March 2004Significance of isotope chemistryIsotope chemistry is a HUGE part of research on meteorites. It is one of the fastest growing areas because of
ASU - GLG - 485
Stable Isotopes of Hydrogen and Carbon in the Solar System29 March 2004 GLG/CHM485 GLG598Evolution of D/H in Universe All D in universe formed in the Big Bang (initial D/H ~50 x 10-6 or 50 ppm) D consumed in stars. Present ratio is 15 x 10-6 (or
ASU - GLG - 485
Meteorites and CosmochemistryMatrix material in primitive (unequilibrated) chondrites 1 March 2004Introduction to The MatrixWhat is it made of (chemically, physically)? Why is it important? How is it studied? Where did it come from?Definition(s
ASU - GLG - 485
1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E1998M&PS.33.565E
ASU - GLG - 485
The Astrophysical Journal, 522:L133L136, 1999 September 101999. The American Astronomical Society. All rights reserved. Printed in U.S.A.CIRCUMSTELLAR HIBONITE AND CORUNDUM AND NUCLEOSYNTHESIS IN ASYMPTOTIC GIANT BRANCH STARS Byeon-Gak Choi,1 G. J
ASU - GLG - 485
Interplanetary Dust Particles and Comets12 April 2004Dust in the cosmos We know there is dust between the planets because: a) Zodiacal light -a brightening of the sky prior to sunrise in unpolluted areas through light scattering off dust between
ASU - GLG - 485
1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C1998M&PS.33.1201C
ASU - GLG - 485
1.03 Solar System Abundances of the ElementsH. Palme Universitat zu Koln, Germany and A. Jones Universite Paris Sud, France1.03.1 ABUNDANCES OF THE ELEMENTS IN THE SOLAR NEBULA 1.03.1.1 Historical Remarks 1.03.1.2 Solar System Abundances of the
ASU - GLG - 485
P1: FOFSeptember 20, 200019:9Annual ReviewsAR108-11Annu. Rev. Astron. Astrophys. 2000. 38:42783 Copyright c 2000 by Annual Reviews. All rights reservedORGANIC MOLECULES IN THE INTERSTELLAR MEDIUM, COMETS, AND METEORITES: A Voyagefrom Dar
ASU - GLG - 3
THE SOLAR SYSTEM D/H RATIO: OBSERVATIONS AND THEORIESFRANOIS ROBERT1 , DANIEL GAUTIER2 , AND BRANGRE DUBRULLE31 Laboratoire de Minralogie, CNRS-Musum, Musum dHistoire Naturelle, 75005 Paris, France 2 DESPA, URA 264, Observatoire de Meudon, F-92195,
ASU - GLG - 485
THE SOLAR SYSTEM D/H RATIO: OBSERVATIONS AND THEORIESFRANOIS ROBERT1 , DANIEL GAUTIER2 , AND BRANGRE DUBRULLE31 Laboratoire de Minralogie, CNRS-Musum, Musum dHistoire Naturelle, 75005 Paris, France 2 DESPA, URA 264, Observatoire de Meudon, F-92195,
ASU - GLG - 2
letters to natureA stellar origin for the short-lived nuclides in the early Solar SystemS. Sahijpal*, J. N. Goswami*, A. M. Davis, L. Grossman & R. S. Lewis* Physical Research Laboratory, Ahmedabad 380 009, India Enrico Fermi Institute, Univers
ASU - GLG - 485
letters to natureA stellar origin for the short-lived nuclides in the early Solar SystemS. Sahijpal*, J. N. Goswami*, A. M. Davis, L. Grossman & R. S. Lewis* Physical Research Laboratory, Ahmedabad 380 009, India Enrico Fermi Institute, Univers
ASU - GLG - 2
REPORTSTable 3. Hydroaminomethylation of different olens. Reaction conditions: olen, 15 mmol; amine, 15 mmol; [Rh(cod)2]BF4, 0.1 mol %; IPHOS, 0.4 mol %; toluene, 15 ml; THF, 15 ml; PCO, 10 bar; PH2, 50 bar; temperature, 120C; time, 24 hours. Olen A
ASU - GLG - 485
REPORTSTable 3. Hydroaminomethylation of different olens. Reaction conditions: olen, 15 mmol; amine, 15 mmol; [Rh(cod)2]BF4, 0.1 mol %; IPHOS, 0.4 mol %; toluene, 15 ml; THF, 15 ml; PCO, 10 bar; PH2, 50 bar; temperature, 120C; time, 24 hours. Olen A
ASU - GLG - 2
RESEARCH ARTICLEX-rays and Fluctuating X-Winds from ProtostarsFrank H. Shu,* Hsien Shang, Alfred E. Glassgold, Typhoon LeeProtostars emit more x-rays, hard and soft, than young sunlike stars in more advanced stages of formation. The x-ray emissio
ASU - GLG - 485
RESEARCH ARTICLEX-rays and Fluctuating X-Winds from ProtostarsFrank H. Shu,* Hsien Shang, Alfred E. Glassgold, Typhoon LeeProtostars emit more x-rays, hard and soft, than young sunlike stars in more advanced stages of formation. The x-ray emissio
ASU - HHUANG - 38
MAE 384 Numerical Methods for EngineersCourse outline Part I Basic numerical methods (Ch. 1, 3-9 of Gilat & Subramaniam) Overview and numerical errors Nonlinear equations System of linear equations (matrix equation, eigenvalue problem) Curve fitting
Cornell - REUPROJECT - 2008
Time of flight identification of ions around accelerated beamsEric Edwards Michael Ehrlichman Georg Hoffstaetter Ion densities in the beam pipe from scattering on the dilute gas Ions can then effect the motion and emittance of the beam, for exam
Cornell - REUPROJECT - 2008
High Field Q-slope and Superconducting Radio Frequency Cavity TestingJordan WebsterDept of Physics, University of Rochester, Rochester, NY, 14627 (Dated: August 4, 2008) High eld Q-slope is a loss mechanism frequently encountered by superconducting
Cornell - REUPROJECT - 2008
Optimizing Monocapillary Optics for Synchrotron X-ray ApplicationsCHESS & LEPPDonald Bilderback1,2, Sterling Cornaby1, Tom Szebenyi, Heung-Soo Lee1,31CornellHigh Energy Synchrotron Source, 2School of Applied and Engineering Physics, 1,2Cornell
Cornell - REUPROJECT - 2008
R&DfortheInternationalLinearCollider DampingRingsMatthewLawson,JimCrittendenCornellLEPPREU,summer2008Overview TwomainprojectsintheILCR&Deffort LowEmittanceTuning ElectronClouds Emittanceisameasureofbeamsize Electroncloudsseenasthemajorobsta
Cornell - REUPROJECT - 2008
ElectronCloudSimulations andRFAdataanalysisMatthewLawson,JimCrittendenCornellLEPPREU,summer2008ElectronCloudBasics PrimarySource:SynchrotronLight Chargesacceleratedbybeampassage SecondaryElectronsgeneratedfromhighvelocity electronsimpactingthe
Cornell - REUPROJECT - 2008
Cornell REU 2008 ProjectStudying the High Field Q-Reduction in Superconducting RF CavitiesStudent: Jordan Webster Mentor: Matthias LiepeMatthias LiepeJune 2, 2008Superconducting RF around the WorldMatthias LiepeJune 2, 2008Superconducti
Cornell - REUPROJECT - 2008
Application of NEG Coatings on a Metal Surface and Measurements of its RF PropertiesAlexander Brown Department of Physics, Allegheny College, Meadville, PA, 16335 Dated: 7 August 2008 The Energy Recovery Linac (ERL) at Cornell University will requir
Cornell - A - 102
Lecture #38: Exobiology II Exobiology II Life in Extreme Environments Searching for Life in Our Solar System More exotic "niches" on Earth Mars Europa Titan? Elsewhere?The Main PointLife on Earth exists in extreme environments, providing s
Cornell - A - 2
Lecture #38: Exobiology II Exobiology II Life in Extreme Environments Searching for Life in Our Solar System More exotic "niches" on Earth Mars Europa Titan? Elsewhere?The Main PointLife on Earth exists in extreme environments, providing s
Cornell - A - 102
Lecture #15: Mercury: General properties. Surface characteristics. Interior and evolution.The Main PointMercury is a small, atmosphereless terrestrial planet with a large metallic core and evidence for a complex geologic history. Reading: C
Cornell - A - 2
Lecture #15: Mercury: General properties. Surface characteristics. Interior and evolution.The Main PointMercury is a small, atmosphereless terrestrial planet with a large metallic core and evidence for a complex geologic history. Reading: C
Cornell - A - 102
Lecture #2: The Sky and Historical Astronomy General Introduction to the Sky. Coordinates: Getting your bearings. Earth's spin and orbital motion. Constellations & Astrology. Classical astronomy. Modern astronomy.1The Main PointThe movement
Cornell - A - 2
Lecture #2: The Sky and Historical Astronomy General Introduction to the Sky. Coordinates: Getting your bearings. Earth's spin and orbital motion. Constellations & Astrology. Classical astronomy. Modern astronomy.1The Main PointThe movement
Cornell - ASTRO - 1102
Astronomy 1102/1104 Exercise 4Due in section from 27 April Observing the Skies2 February, 2009Your assignment is to attend an observing session at Fuertes Observatory on campus. When you attend, be sure to show your student ID to the astronomer i
Cornell - A - 102
Lecture #11: Earth: Geology and Interior Overview of Earth's basic properties. Earth's Interior and Surface: Composition and Structure. Surface Geologic Processes. Evolution of the Surface.The Main PointEarth is a rocky planet with a differen
Cornell - A - 2
Lecture #11: Earth: Geology and Interior Overview of Earth's basic properties. Earth's Interior and Surface: Composition and Structure. Surface Geologic Processes. Evolution of the Surface.The Main PointEarth is a rocky planet with a differen
Cornell - NS - 338
Deception and Evidence i Final version in Philosophical Perspectives (2005), 19: 375-404 Nicholas SilinsIntroductionSuppose that, whenever Gary has an experience as of two bananas in a bowl, Barry does too, and that whenever Gary believes that th
Cornell - RMF - 25
Index Theory of Continuous Dynamical SystemsRafael FrongilloMay 7, 20040.1. INTRODUCTION10.1IntroductionThe theory of Dynamical Systems, while once purely physical, is now extremely important in almost all of the sciences. There are many
ASU - MAR - 2007
EXECUTIVE SUMMARY ACTION ITEM: ISSUE:Board of Regents Meeting March 8-9, 2007 Agenda Item #12 Page 1 of 7Academic Program and Organizational Change RequestsThe Board is requested to authorize academic program planning for one new program at Ari
Cornell - CEE - 20
CEE 3310 Lecture 41, Dec. 5, 200811Review Flow through a contraction Critical and choked ows The hydraulic jump conservation of linear momentum 1 + y2 = y1 Broad-Crested Weir 1 + 8Fr2 1 2If we ignore energy losses and assume the upstre
Cornell - CEE - 331
CEE 3310 Lecture 41, Dec. 5, 200811Review Flow through a contraction Critical and choked ows The hydraulic jump conservation of linear momentum 1 + y2 = y1 Broad-Crested Weir 1 + 8Fr2 1 2If we ignore energy losses and assume the upstre
Cornell - CEE - 20
CEE 3310 Open Channel Flow78.8Review Laminar vs Turbulent Boundary Layer Turbulent boundaryDrag & Liftlayers stay attached to bodies longer Narrower wake! Lower pressure drag! Open Channel Flow Gravity friction balance.In general w
Cornell - CEE - 331
CEE 3310 Open Channel Flow78.8Review Laminar vs Turbulent Boundary Layer Turbulent boundaryDrag & Liftlayers stay attached to bodies longer Narrower wake! Lower pressure drag! Open Channel Flow Gravity friction balance.In general w
Cornell - CEE - 20
A relative is so impressed with your fluid mechanics skills she asks you to solve one of the great problems of the beer-drinking world the foamy pint. Now, she makes her own beer and puts it into kegs (pressurized containers), which she stores in an
Cornell - CEE - 331
A relative is so impressed with your fluid mechanics skills she asks you to solve one of the great problems of the beer-drinking world the foamy pint. Now, she makes her own beer and puts it into kegs (pressurized containers), which she stores in an
ASU - SEP - 2006
ABOR Meeting September 27-28, 2006 Item #29 Page 1 of 1EXECUTIVE SUMMARYPowerPoint Presentation Spellings ReportINFORMATION ITEM: ISSUE:Commission on the Future of Higher Education The Board will hear a presentation on the final report of the
ASU - MAR - 2007
SOLUTIONS FOR OUR FUTUREAmericas colleges and universities: i ii We teach the people who solve the problems and change the world.SOLUTIONS FOR OUR FUTURE National campaign Organized under auspices of the American Council on Education (ACE), wit
ASU - SEP - 2007
Board of Regents Meeting September 27-28, 2007 Item #30 EXECUTIVE SUMMARY Page 1 of 3 _ ACTION ITEM: Approval of Regents Awards for Outstanding Service to Higher Education The Board is asked to approve the recommendations of the Regents Award Selecti
ASU - V - 12
EPAA Vol. 12 No. 19 Hamrick, Schuh & Shelley: Higher Education Institutional Characterist. Page 1 of 24A peer-reviewed scholar journal Editor: Gene V Glass College of Education Arizona State UniversityCopyright is retained by the first or sole au
ASU - V - 7
Final Report To the Planning Committee Of the State Council of Higher Education for VirginiaAcademic Program Approval and Review Practices In States and Selected Foreign CountriesPrincipal Investigators: Don G. Creamer Steve M. Janosik Chunmei Zh
ASU - V - 13
EDUCATION POLICY ANALYSIS ARCHIVESCopyright is retained by the first or sole author, who grants right of first publication to the Education Policy Analysis Archives. EPAA is published jointly by the Colleges of Education at Arizona State University
ASU - V - 12
EDUCATION POLICY ANALYSIS ARCHIVESA peer -reviewed scholarly journal Editor: Gene V Glass College of Education Arizona State University Copyright is retained by the first or sole author, who grants right of first publication to the Education Policy
ASU - V - 12
E ducation P olicy A nalysis A rchivesA peer-reviewed scholarly journal Editor: Gene V Glass College of Education Arizona State UniversityCopyright is retained by the first or sole author, who grants right of first publication to the Education Poli
ASU - V - 13
EDUCATION POLICY ANALYSIS ARCHIVESA peer-reviewed scholarly journal Editor: Sherman Dorn College of Education University of South Florida Copyright is retained by the first or sole author, who grants right of first publication to the Education Polic
ASU - V - 14
EDUCATION POLICY ANALYSIS ARCHIVESA peer-reviewed scholarly journal Editor: Sherman Dorn College of Education University of South Florida Volume 14 Number 33 December 15, 2006 ISSN 10682341Comparison of the Enrollment Percentages of Magnet and Non
ASU - V - 12
A peer-reviewed scholarly journal Editor: Gene V Glass College of Education Arizona State UniversityCopyright is retained by the first or sole author, who grants right of first publication to the EDUCATION POLICY ANALYSIS ARCHIVES. EPAA is a projec