Caltech - AERO - 1989

Caltech - AERO - 1987

Caltech - PUBS - 1987

Caltech - AERO - 1985

Caltech - CIT - 40

QuickTimeTM and a TIFF (Uncompressed) decompressor are needed to see this picture.Angular Noise in a Suspended Interferometer with DC ReadoutRoyal Reinecke Co-Mentors: Alan Weinstein and Rana AdhikariQuickTimeTM and a TIFF (Uncompressed) decompr

Caltech - G - 020413

Selected features of DB2 & metadatabase replicationIgor Yakushin 4/09/02LIGO-G020413-00-LContent^ ^ ^ ^^ ^ ^^ ^db2cc Administration server Transaction logging Returning a database to a consistent state after minor failures Backup and recov

Caltech - G - 080532

Virgo+ Commissioning StatusLIGO-G080532-00-ZMain upgrades and activities Laser system: from 10 25 watt output power at the IMC TCS: ring + Central Heating Electronics: ADCs and DSP replacement, Global Control Viewports replacement NE mirror

Caltech - MSC - 2008

Negative Differential Resistance at SAM of Oligo (Phenylene Ethynylene) on Au (111) SurfaceHyungjun Kim1, Seung Soon Jang2 and William A. Goddard III11Materials and Process Simulation Center (MC 139-74)California Institute of Technology, Pasad

Minnesota - CE - 3201

CE 3201 Introduction to Transportation EngineeringGeometric Design of Highways Vertical Curve Sight Distance (cont.)Chapter 3CE 3201 Introduction to Transportation EngineeringMinimum Stopping-Sight Distance Construction of a vertical curve is

Minnesota - CE - 3201

Name_ Class Solution _ CE 3201 - Recitation #1 Bicycle Race It has been estimated that Tour-de-France champion Lance Armstrong could generate a sustained 500 Watts of power over a 20-minute period, while a healthy young human male (HYHM) can generate

Minnesota - CE - 4211

Traffic Engineering Topic: Traffic Studies & Data CollectionHenry Liu CE 4211/5211 Traffic Engineering University of Minnesota email: henryliu@umn.eduShockwaves signalized intersectionsxqBAB D BA A D0 kCACtTraffic Studies

Minnesota - CE - 4211

Department of Civil Engineering CEE 4211/5211 Traffic EngineeringSpring 2009 Dr. Henry LiuLab 2: The Fundamental Diagram of TrafficLab Report Due: Monday February 23, 20091Department of Civil Engineering CEE 4211/5211 Traffic EngineeringSp

Caltech - G - 010120

Anatomy of an ldasJobLSC Meeting March 2001 Antony C. Searle ACIGA / ANULIGO-G010120-00-ZLDAS and E3!!E3 study by Philip Charlton (CIT) using LDAS datacondAPI. Correlations and PSDs produced in realtime.! !Continuous loop submitted batch

Minnesota - EE - 3940

EE 3940 Global Seminar: Engineering and Research in Taiwan and Hong Kong Prof. Jerry Sobelman May Intersession 2008 Goals and Objectives of the Course The purpose of this class is to obtain an understanding of a broad range of research and engineer

Minnesota - EE - 4363

Minnesota - EE - 4301

Lab #3 EE4301 ECE UMNSchematic Design Entry, Implementation, and SimulationSchematic Design Entry, Implementation, and Simulation-PURPOSE - This lab will present basically the same design steps learned during the first two laboratories. Howev

Minnesota - EE - 4301

Downloading to XC3S100EPURPOSE: This lab will present a brief overview of the XC3S100E FPGA Board (of Digilent) and how to download bitstream (the result of the implementation of a design) files to it. 1. Introduction to the XC3S100E FPGA and BASYS

Minnesota - ME - 2011

UNDERSTANDING DC MOTORS ACTIVITY GUIDETASK A: What Motors Can Do Split group into teams of two for simultaneous testing of multiple motors. Tie 6 ft. or so of thread to a motor shaft and wind a few turns around the shaft so that the thread does not

Caltech - MATH - 8

Please don't hate power series! Math 8 2008, Chris Lyons In light of that tangled proof, the continual mix-up between z's and 2's, and a number of other things, you may have gotten a distaste for power series after my lecture today. But don't let my

Caltech - PH - 1

FP21 Oil and Water Don't Mix

Caltech - CNS - 221

Introduction Bloodgood & Sabatini - Science 2005 Harris MCell questions?Diusion: dont neglect the random walkWill FordMay 22, 2006logoWill FordCNS 221: Diusion with a little ReactionIntroduction Bloodgood & Sabatini - Science 2005 Harris

Caltech - CNS - 286

Homework Solution 1: Set Theory and Conditional ProbabilityAssigned 3/30, due 4/10 100 pointsProblem 1:a)Show P (A|B) P (A) + P (B) - 1 P (B)See Figure 1.0 below. Let b = A B, a = A - b, and c = B - bNote that a + b + c 1, so a + b + c -

Caltech - G - 050404

h(t): are you experienced?():Michael LandryLIGO Hanford Observatoryon behalf of the CW search groupLIGO-G050404-00-Zh(t) and the CW group h(t) for S4: Xavier Siemens created one version of h(t) using V1 calibration and V4 DQ flags Minimum

Caltech - G - 070601

Photon Calibrator DRR & CDR: Response to Reviewers' ReportPhil Willems, Mike SmithLIGO-G070601-00-MConceptual DesignReviewers' comment: "Given our experience with the iLIGO photon calibrators, we don't think it is worthwhile to do any significa

Caltech - G - 060036

The Ins and Outs of Inspiral SearchesPeter ShawhanCaltech / LIGO For the LSC Inspiral Analysis GroupSyracuse University March 3, 2006LIGO-G060036-00-ZA Perfect Gravitational Wave SourceTo lowest order, gravitational wave emission is determine

Caltech - G - 060137

Why (else) is J0537-6910 interesting to us?Ben Owen Penn StateLIGO-G060137-00-Z2006 March 22LIGO Scientific Collaboration1The story Discovery paper in 1998: Middleditch & co. were looking for SN 1987A x-ray pulses (Same time as r-modes g

Caltech - G - 070105

New Glitches seen/studied in Block-NormalShantanu Desai Pennsylvania State University for Glitch Working Group and many others Detchar session March 2007 LSC meetingG070105-00-Z1Outline of Talk Block-Normal "glitches" indicates events in S5 w

Caltech - G - 070516

Eyes Wide Open:Searching for Gravitational Wave BurstsPeter Shawhan for the LSC-Virgo Burst Analysis Working GroupLSC-Virgo Meeting July 23, 2007LIGO-G070516-00-ZPhilosophyWere listening to the whole sky who knows whats out there?Models a

Caltech - G - 050252

Gravitational Waves: From Astrophysics to OpticsPeter R. Saulson Syracuse University Department of Physics Spokesperson, LIGO Scientific CollaborationLIGO-G050252-00-Z1Outline What are gravitational waves, and why are they interesting? How d

Caltech - G - 030263

Implementation of LIGO's Triggered Burst SearchRauha Rahkola (U of Oregon), representing the LIGO Scientific CollaborationThis material is based upon work supported in part by National Science Foundation Award PHY-0071058May 30-31, 2003,LIGO G0

Caltech - ETD - 02092007

Caltech - ETD - 05272005

Chapter 819F NMR Probing the Acidity of Frozen Electrolyte SolutionsC. Robinson, C. S. Boxe, M. I. Guzmn, A. J. Colussi,* and M. R. Hoffmann W. M. Keck Laboratories, California Institute of Technology, Pasadena, CA 91125AbstractThe marginal b

Caltech - ETD - 09202002

Caltech - ETD - 09062007

Caltech - ETD - 05232006

Chapter 2. A Brief Review of Electron Diffraction Theory8Chapter 2. A Brief Review of Electron Diffraction TheoryThe theory of gas phase electron diffraction is hardly a new topic. It is well established for decades and has been thoroughly desc

Caltech - ETD - 11112004

Caltech - ETD - 02122009

Caltech - ETD - 02072006

Caltech - SSC - 2008

Spitzer Reveals 'No Organics' Zone Around Pinwheel GalaxyFor Release: July 21, 2008The Pinwheel galaxy is gussied up in infrared light in a new picture from NASA's Spitzer Space Telescope. The fluffy-looking galaxy, officially named Messier 101, i

Caltech - SSC - 2009

Dead Stars Tell Story of Planet BirthFor Release: January 05, 2009Astronomers have turned to an unexpected place to study the evolution of planets - dead stars. Observations made with NASA's Spitzer Space Telescope reveal six dead "white dwarf" st

Caltech - SSC - 2007

Astronomers Say Moons Like Ours Are UncommonFor Release: November 20, 2007The next time you take a moonlit stroll, or admire a full, bright-white moon looming in the night sky, you might count yourself lucky. New observations from NASA's Spitzer S

Caltech - SSC - 2007

Embryonic Star Captured with Jets FlaringFor Release: November 29, 2007A developing star wrapped in a black cocoon of dust is seen sprouting giant jets in a new image from NASA's Spitzer Space Telescope. The stellar portrait, captured in infrared

Caltech - SSC - 2006

Galaxy on Fire! NASA's Spitzer Reveals Stellar SmokeFor Release: March 16, 2006Where there's smoke, there's fire even in outer space. A new infrared image from NASA's Spitzer Space Telescope shows a burning hot galaxy whose fiery stars appear to

Caltech - SSC - 2007

Office of University Communications FOR IMMEDIATE RELEASEUniversity Services Building Room 413 P.O. Box 210158 Tucson, AZ 85721-0158 (520) 621-1877 (520) 626-4121 FaxFor Release Monday, Jan. 8, 2007 Science Contact Information Ilaria Pascucci 52

Caltech - SSC - 2006

NASA's Spitzer Sees Day and Night on Exotic WorldFor Release: October 12, 2006NASA's Spitzer Space Telescope has made the first measurements of the day and night temperatures of a planet outside our solar system. The infrared observatory revealed

Caltech - ETD - 09202008

Caltech - ETD - 05242005

A-1Appendix A. Design and Fabrication of Cold SleeveA cold sleeve was designed and fabricated in order to conduct temperaturedependent studies on trapped ions in the ICR cell. Figure A.1 shows the machine diagrams for a custom-designed flange to b

Caltech - ETD - 05092003

Mirror Thermal Noise in Interferometric Gravitational Wave DetectorsThesis byShanti R. RaoIn Partial Fulfillment of the Requirements for the Degree of Doctor of PhilosophyCalifornia Institute of Technology Pasadena, California2003 (Defended

Caltech - ETD - 10292007

On A Capacitated Multivehicle Routing ProblemThesis byXiaojie GaoIn Partial Fulfillment of the Requirements for the Degree of Doctor of PhilosophyCalifornia Institute of Technology Pasadena, California2008 (Defended August 3, 2007)iic2

Caltech - ETD - 05092003

75Chapter 4The Thermal Noise Interferometer4.1 IntroductionThe purpose of the Thermal Noise Interferometer (TNI) project is to build a low-noise interferometer capable of determining the fundamental noise sources that would limit LIGOs sensiti

Caltech - ETD - 01102006

Caltech - ETD - 03262007

Caltech - ETD - 01302007

7Chapter 2 Apparatus The ultrafast electron crystallography (UEC) apparatus in our lab is built for the study of thin crystals and surfaces, based on experience of three generations of gas phase ultrafast electron diffraction (UED). It includes a

Caltech - ETD - 03072006

75Part IIIPsychophysics7677Chapter 7Measuring the Cost of Deploying Top-down Visual Attention7.1 IntroductionImagine walking into a crowded restaurant, looking for your friend whom you are supposed to meet. You will be looking around,

Caltech - PAPER - 19

submitted to ApJLUV observations of periodic annular intensity fluctuations propagating around sunspots 1A.A. Georgakilas Solar Astronomy, California Institute of Technology, Pasadena, CA 91125 ageorg@caltech.edu and K. Muglach Astrophysikalisches

Caltech - PH - 1

QP51 Ball on a String Wrapping Around a Nail

Caltech - CIT - 40

INSTITUTE OF PHYSICS PUBLISHING Class. Quantum Grav. 23 (2006) 56615666CLASSICAL AND QUANTUM GRAVITYdoi:10.1088/0264-9381/23/18/010Control sideband generation for dual-recycled laser interferometric gravitational wave detectorsB W Barr1, O Miy

Caltech - T - 050098

Advanced LIGOT050098-00LIGO Laboratory / LIGO Scientific CollaborationLIGO-T050098-00-DAdvanced LIGO11 June 2005Optics Table Hole Size and Spacing based on Suspension Attachment Frequencies (Advanced LIGO)Dennis Coyne Distribution of thi

Caltech - AMALDI - 5

Properties of seismic noise at VirgoIrene FioriINFN Firenze for the Virgo Collaboration5th Amaldi Conference on Gravitational Waves Tirrenia (Italy) 7-11 July 2003Seismic Monitoring NetworkNorth End b. 3km 3km Low Frequency Accelerometers Tri-

Caltech - ASPEN - 2004

Can we use atom interferometers in searching for gravitational waves? C.J. Bord, University of Paris N. G. Tino, University of Firenze F. Vetrano, University of UrbinoF.Vetrano - Aspen Winter Conference, FEB 2004Intuitive concept: ~ 1/low

Caltech - AMALDI - 5

LIGO laser intensity noise suppressionAmaldi 5July 2003G030320-00-CFlavio NoceraPSLThe Pre-Stabilized Laser (PSL) subsystem is the light source for the LIGO detector as shown in figure 1ETMYLIGO interferometer4 kmITMY12 mPSLBS