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Course: DOCS 0, Fall 2009
School: Minnesota
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Minnesota - ME - 3331
IrreversibilityIncrease of Entropy PrincipleHeat, Work and Energy. A First Course in Thermodynamics 2009, F. A. Kulacki Module 30 Slide 1 Irreversibility and the Increase of Entropy PrincipleOverview Irreversibility Increase of entropy princi
Minnesota - IE - 5080
Introduction Examples and Tricks Chvatal-Gomory ProcedureValid InequalitiesBharath RangarajanJan 29, 2009B. RangarajanValid Inequalities01/29/091 / 14From P to PIntroduction Examples and Tricks Chvatal-Gomory ProcedureFor X = {x
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Section 4.6 in textMinimize x1max6x 2- x1, 4x 2, -5x1 , 9 Constraints on x 1, x2. Minimize x1t Constraints on x 1, x2 max 6x2 -x 1, 4x 2,-5x 1 , 9t.t does not interfere with original constraints value for t is determined only by the min/max obje
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University Technology Training CenterMoodle 1.8:GradesUNIVERSITY TECHNOLOGY TRAINING CENTERMoodle 1.8:Grades 2007 Regents of the University of Minnesota University Technology Training Center All Rights Reserved uttc.umn.eduThe University
Caltech - WIN - 03
What do the complex workings of a cell have in common with the relentless unrest of the New York Stock Exchange? Are these dynamic storehouses of information obeying similar laws in terms of the ebb and flow of information, and can they be modeled, a
Caltech - WIN - 03
Markets and Other Noisy Human ArtifactsCan Computation Bring Them Out of the Bronze Age? A Conversation with Yaser S. Abu-Mostafa, K. Mani Chandy, and John O. LedyardSocial systems such as financial markets, political processes, and organizations ag
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progressreportsUnderstanding Material Deformation: Insights into the Inner Workings of Complex Materialsby Ersan stndagIn most engineering calculations, the mechanical performance of structures or components is esti
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Soft Circuitry and Liquid Algorithms- A New Bioengineering Frontier Takes Form A Conversation with Niles Pierce, Paul Sternberg, Erik Winfree, and Barbara WoldBiology computes, that is, living structures store, process, and communicate information i
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newfacultyInflux of Talent: Division Grows by NineSix new professors have joined the Division and Caltech over the past several months, bringing fresh insights and new research directions our way. Also new to the Division are thr
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alumniprofilesIvett Leyva: An Experimentalist with International FlairAeronautics, PhD 99With this issue we are beginning our practice of offering two alumni profilesone of a neophyte (an alum who has recently graduated)
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i n f o r m a t i o ns c i e n c ea n dt e c h n o l o g yCenter for the Mathematics of Information: Information Theory Revisited:Mathematicians and Friends Tackle the Whole Enchilada A Conversation with Emmanuel Candes, Michelle Effros, and
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ideaflowSensing and Responding: Mani Chandy's Biologically Inspired Approach to Crisis ManagementOrganisms receive streams of information from their senses, yet they manage to avoid information overload and system breakdown by ins
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i n f o r m a t i o ns c i e n c ea n dt e c h n o l o g yexert embedded control over macroscopic electromechanical systems, and this has revolutionized technology. Nature, through biological processes, has transformed the earth by exploiting
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She also fondly remembers her friends on campus, who made me a very happy student. At GE I have learned to merge analytical and academic knowledge I gained at Caltech with more practical and experience-based knowledge gained through my first few year
Caltech - G - 080341
Orsay, 11 June 2008Status of the LSCDavid Reitze University of FloridaLIGO-G080341 -00-ZLIGO Scientific Collaboration1General NewsYouve heard exciting progress on E-LIGO, AdvLIGO, Astrowatch, S5 analyses LSC is still growing 634 members
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Locating and Observing Optical Counterparts to Unmodeled Pulses in Gravitational WavesJonah Kanner, Peter Shawhan, Tracy Huard Szabolcs Marka, Jennifer Piscionere David Murphy LOOC UP LIGO-G070827-00-Z Univ. of Maryland Columbia Univ. Carnegie Obser
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LIGO Laboratory / LIGO Scientific CollaborationLIGO-E070250-00-V10/23/2007ELI VENT &amp; SEPTUM INSTALLATION PROCEDURER. WooleyDistribution of this document: Detector Technical Review Board This is an internal working note of the LIGO Laboratory
Caltech - T - 030013
Plan for Hardware Signal Injections Before and During the S2 Run, P. Shawhan, Sz. MrkaLIGO-T030013-00-DLASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO -CALIFORNIAINSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGYDocument
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Management and Operation Plans/BudgetStan Whitcomb NSF Annual Review 8 November 2004 CaltechLIGO-G040482-00-MOverview Address remaining two items of charge Impact of management change (Gary Sanders) Evolution of LIGO managementCurrent pl
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Amsterdam, September 22, 2008Status of the LSCDave Reitze University of FloridaLIGO-G080454-00-ZLIGO Scientific Collaboration1NewsMany exciting things happening on lots of fronts AdvLIGO, GEO, Virgo+, Astrowatch, E-LIGO, S5 analysis resu
Caltech - PH - 3
B u reau International des Poids et Mesure sThe Intern a t i o n a l System of Units (SI)7th edition1998Organisation Intergouvernementale de la Convention du MtreNote on the use of the English text To make its work more widely accessible, t
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PRIMER ON DATA ANALYSIScDon Skelton 1984TABLE OF CONTENTS pageI. MEAN AND STANDARD DEVIATIONMean, m, of the Parent Population Standard Deviation Practical Considerations Sigma of the Mean Example 1 - Torsion Pendulum Example 2 - Weighted Aver
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)Analog Electronic Measurements: AC MeasurementAcademic Year 2007-2008 Copyright c Virgnio de Oliveira Sannibale, 2001Contents10 Al
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics LaboratoryInstrumentation: The CRT OscilloscopeCopyright c Virgnio de Oliveira Sannibale, 20012ContentsA The Cathode Ray Tube Oscilloscope A.1 The
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISION1Freshman Physics Laboratory (PH003)Classical Mechanics Measurements: The Maxwell TopAcademic Year 2007-2008 CopyrightVirgnio de Oliveira Sannibale, 2001Contents1 T
Caltech - PH - 3
g t 4y e { y \$y f g { g y e y q x w\$myTye h Thprf|y|h{C4wkphy Puyr{q~q g \$pT4 hyXyf lph0Ff prgh{wfg wp |h{~gy ywfdr X{h9gwk w y~hyg{ lfw~yd~gt h{uglfG~ p{\$xw ukf ymwpwhgxymkf df ~y g h{hlfdhyf Fpk mphw x|Goueffhgg j hyyF}k mp| fU
Caltech - PH - 3
CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)Basics on Semiconductors PhysicsCopyright c Virginio de Oliveira Sannibale, 2001Contents10 Semiconductors Conduction 10.1 Conducti
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From: physics.nist.gov/constantsFundamental Physical Constants Complete ListingQuantity Symbol Value UNIVERSAL speed of light in vacuum magnetic constant electric constant 1/0 c2 characteristic impedance of vacuum 0 / 0 = 0 c Newtonian constant
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LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGYDocument Type T040160-00 Aug 10, 2004New BSC Transfer Functions Model for E2E-SimLIGO (DRAFT)V. SannibaleDistrib
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONSophomore Physics Laboratory (PH005/105)Analog Electronics: The Operational AmplifierAcademic Year 2007-2008 Copyright c Virgnio de Oliveira Sannibale, 2003Contents4
Caltech - G - 000154
Performance of the LIGO Pre-stabilized Laser SystemRick SavageLIGO Hanford Observatory Ninth Marcel Grossmann Meeting on General Relativity Rome 2000LIGO-G000154-00-WPSL Design and Performance AssessmentDesign: l Peter King, Rich Abbott, Alex A
Caltech - G - 060113
Nd:YVO4 Amplifier SystemBastian Schulz, Maik Frede, Ralf Wilhelm, and Dietmar KrachtLaser Zentrum HannoverFrank Seifert, Patrick Kwee and Benno WillkeAEI LSC March 06 G060113-00-ZOutline Single Amplifier stage design Amplifier Setup with 2
Caltech - G - 080222
Power Stabilization of the 35W Reference SystemFrank Seifert, Patrick Kwee, Benno Willke, Karsten Danzmann Max-Planck-Institute for Gravitational Physics (Albert-Einstein-Institute) University of Hannover LSC Caltech, March 19th, 2008 LIGO-G08xxxx-x
Caltech - G - 050267
Passive seismic attenuation for the LIGO Output mode cleaner; HAM-SASR. DeSalvo, C. Galli, G. Gennaro, M. Mantovani, S. Marka, V. Sannibale, A. Takamori, C. Torrie , A. Bertolini23nd May 2005LIGO-G050267-00-RIntroduction A SAS configuration (HA
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LIGO Data Analysis System (LDAS)PAC 11 MeetingCalifornia Institute of Technology November 29, 2001James Kent Blackburn LIGO Laboratory, CaltechLIGO-G010404-00-EThree remaining modules under active developmentCurrent release of LDAS: LDAS-0.0
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Enhanced LIGO Laser SystemS. Wagner, B. Schulz, R. Wachter, C. Veltkamp, M. Janssen, P. Weels, M. Frede, D. KrachtOutline Overview eLIGO Laser development eLIGO Laser System Laser Head Diode Box Control BoxCharacterization NPRO Laser H
Caltech - T - 070102
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY - LIGO CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGYDocument TypeLIGO-T070102-00-Z2007/09/05Post-S5 Operating System for the LIGO Data GridPaul Armor, Carsten Aul
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GEO+ Online Detector Characterization System.LIGO-G020382-00-ZGEO+ working groupCardiff University: Stas Babak R. Balasubramanian David Churches B.S. Sathyaprakash Birmingham University Alberto Vecchio Richard Ingley AEI: Soumya MohantyGEO+: Ge
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONSophomore Physics Laboratory (PH005/105)Analog Electronics AppendixCopyright c Virgnio de Oliveira Sannibale, 2001 (Revision September 2006)DRAF TContentsA Fouri
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aFEATURES Enhanced Replacement for LF411 and TL081 AC PERFORMANCE Settles to 0.01% in 1.0 s 16 V/ s min Slew Rate (AD711J) 3 MHz min Unity Gain Bandwidth (AD711J) DC PERFORMANCE 0.25 mV max Offset Voltage: (AD711C) 3 V/ C max Drift: (AD711C) 200 V/m
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONSophomore Physics Laboratory Physics 5 and 105 CourseLaboratory NotesAcademic Year 2008-2009 (Partial Revision September 2007)CopyrightVirgnio de Oliveira Sannibale
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)VadeMecum for Data Analysis Beginners(October 3, 2007) Copyright c Virgnio de Oliveira Sannibale, June, 20012AcknowledgmentsI st
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)Classical Mechanics Measurements: The Inverted PendulumAcademic Year 2007-2008 CopyrightVirgnio de Oliveira Sannibale, 2001Contents
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)Classical Mechanics Measurements: A Mechanical OscillatorAcademic Year 2007-2008 Copyright c Virgnio de Oliveira Sannibale, 2001Con
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CALIFORNIA INSTITUTE OF TECHNOLOGY PHYSICS MATHEMATICS AND ASTRONOMY DIVISIONFreshman Physics Laboratory (PH003)Analog Electronic Measurements: DC MeasurementsAcademic Year 2007-2008 Copyright c Virgnio de Oliveira Sannibale, 2001Contents9 Di
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THz Low Loss Flexible Waveguide (Caltech/CAS)Program: NIH R21 with Cavour Yeh (California Advanced Systems-CAS) (ends in Sept. 2008)Intensity (dB)Calculated Signal Power Propagation Losses at 600 GHz and 2.5 THz for some competing guide configur
Caltech - PEOPLE - 2
THz Detection of BC &amp; SC Carcinoma (Caltech/USC)Program: NIH R21 (pending) with David Peng (USC dept. of Dermatology), Warren Grundfest (UCLA dept. of surgery), Scott Fraser Purpose: Develop THz imaging spectrometer for demarcation of Basal and Squ
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THz Effects on Cellular Systems (Caltech/HMRI)Cell Apoptosis after RF ExposureProgram: NIH K25 continuation with Victor Pikov (HMRI) and Jan Stake (Chalmers) (ends in Sept. 2008) Purpose: Examine low level RF effects on cellular systems for health
Caltech - PEOPLE - 2
THz Radar Imaging (Caltech/JPL)Program: Navy Explosive Ordinance Division Phase 1: (ends November 2008). Purpose: Develop THz imaging radar for remote undergarment screening at 4-20m Underlying Technology: Solid state broad band swept frequency THz
Caltech - PEOPLE - 2
THz Source and Sensor Development (JPL/Caltech)Program: Assorted NASA &amp; JPL internal tasks Utilizes approx. 15 people in SWAT group at JPL Purpose: Develop THz sensors and sources for space based instruments: Earth, planets, astrophysics Underlying
Caltech - PEOPLE - 2
THz Imaging for Biomedical Applications (Caltech/JPL)Program: NIH bioengineering cross training grant with Scott Fraser &amp; Warren Grundfest (UCLA) (ends in Sept. 2008) Purpose: Develop THz imaging techniques and instruments for biomedical applicatio
Caltech - ABSTRACTS - 2009
The Mark 5C VLBI Data System A. R. Whitney(1), J. D. Romney(2) and K. Owens(3) (1) MIT Haystack Observatory, Westford, MA, USA (2) National Radio Astronomy Observatory, Socorro, NM, USA (3) Conduant Corporation, Longmont, CO, USAThe rapid adoption
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Dr. Reed L. Riddle Close binaries, stellar interactions and novaeGuest lecture Astronomy 20 November 2, 2004Gravitational Tides Look at the forces acting on one body orbiting another - more pull on closer side Subtract center of mass force - o
Caltech - AY - 122
The Celestial Sphere Coordinate Systems, Time Systems, and AstrometryThink of it as an outward projection of the terrestrial long-lat coordinate system onto the sky! the Equatorial SystemThe Equatorial SystemThe coordinates are Right Ascension
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Ay 20 - Fall 2004 The Long-Lost Lecture 14:Planetary System Formation, Extrasolar Planets, Life in the Universe, and SETIPre-main Sequence Evolution10Disk/wind105 yrLstar Planet building1 109 yr 107 yr100 AU104 yrPlanetary systemMa
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Introduction to DatabasesMatthew J. Graham CACR Methods of Computational Science Caltech, 2009 January 27 Acknowledgements to Julian Bunn and Ed Upchurchmat!ew grahamwhat is a database?A structured collection of data residing on a computer syst
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Ay 20 - Lecture 3:Astronomical Instruments and Measurements What can be measured and how Magnitudes, fluxes, and photometric systems Imaging and photometry Spectroscopy Other stuff: time series, polarimetry .What Properties of Electromagnetic
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Ay 124 Midterm (Observational Part)Posted on Tuesday, Feb. 3 Due by 5 pm on Wednesday, Feb. 11 (directly to the TA) Note: You have up to 2 hours to do this part, and it counts for 40% of your midterm grade. Then you have up to 3 hours to do the th
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Ay 20 - Fall 2004 - Lecture 17Stellar Luminosity and Mass Functions * History and Formation of Our GalaxyStellar Luminosity and Mass Functions Basic statistical descriptors of stellar populations: probability distribution for stellar luminositie
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Astronomy 20:Basic Astronomy and the Galaxy Fall 2004 http:/ www.astro.caltech.edu/~george/ay20/Lecture 1: The class logistics A bit of history The nature of astronomy as a science Coordinates, times, and unitsThe Evolution of Astronomy Fro