Caltech - ETD - 02222007

Caltech - ETD - 05312007

ULTRA-DENSE NANO- AND MOLECULAR-ELECTRONIC CIRCUITSThesis by Jonathan Earl GreenIn Partial Fulfillment of the Requirements for the Degree ofDoctor of PhilosophyCALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2007 (Defended May 18, 200

Caltech - ETD - 09222005

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Caltech - CH - 110

Caltech - CH - 110

Caltech - AE - 244

Mechanics of Nanomaterials (Ae 244)Nano-BioMechanics1Overview nano-biomechanics2Overview nano-biomechanics3Overview nano-biomechanicswww.balgrist.ch4Overview nano-biomechanics5M. Spector, Ph.D. and I.V. Yannas, Ph.D., MITRel

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 26Genes, Genomes, and the Genetic CodeGene: the basic functional unit of an organism's heredity, or isolated sequences of DNA bases represent the instructions for a variety of cell functions A single gene consists of

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 35Summary of Detection Methods(1) Direct methods (2) Astrometry position (3) Radial velocity motion (4) Transits brightness Effects of a planet on the parent star (5) Gravitational microlensing Effects of a planet

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 33 Transits of Mercury are a rare phenomenon due to the orbital plane of Mercury being slightly tilted (about 7 degrees) relative to the orbital plane of the Earth Orbital inclination plays a key role in the visibilit

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 22The Ice Crust Of EuropaTidal flexing is continually deforming the ice crust of Europa, until it cracks. Ridges may have formed when underlying material broke through.Europa : The Water World ?The center is the m

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 07Star FormationWhere planets also form Giant Molecular Clouds (GMCs) Raw material for star birth Gravitational Collapse & Fragmentation Proto-stars, proto-binaries, proto-clusters Rotation & Magnetic Fields Accret

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 11Sun spot and magnetic field activity in the sun may also affect evolution of lifePenumbraTypical temperature in the sun spot ~ 4200K, much colder than the rest part of the solar surface UmbraThe strong magnetic

Caltech - AS - 3012

AS3012: Exoplanetary ScienceStephen Kane srk1 Room 226Radial velocities Currently the most successful method used to detect exoplanets Method relies on the Doppler shift of starlight resulting from the star orbiting a common center of mass with

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 10The Temperature-Luminosity Diagram, also called Hertzsprung-Russell (HR) Diargam About 90% of stars are along a swath of the graph called the Main Sequence, stars with higher surface temperatures have much greater

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 05Common Character of Life Order Reproduction Growth and development Energy utilization Response to the environment Evolutionary adaptationEvolution as Biology's Unifying Theme, proposed by Charles Darwin in hi

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 18Method II: Listen at various radio wavelengths for signals Several pioneers of radio broadcasting, including Nikola Tesla (1856-1943) and Guglilmo Marconi (1874-1937), suggested the possibility of interplanetary rad

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 24IV. Life on Earth Biochemistry and Origins of Life on Earth Early Life and Evolution of Life on EarthBiochemistry of Living Organisms- Ingredients of Life: - Chemistry / biochemistry basics - Some functional b

Caltech - AS - 3012

AS3012: Exoplanetary ScienceStephen Kane srk1 Room 226Detection Methods Covered So Far(1) Direct methods (2) Astrometry position (3) Radial velocity motion (4) Transits brightness Effects of a planet on the parent starTransitsSimplest meth

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 13III. Life in the Solar System Overview and origin of the solar system Atmospheres & habitability of Venus and Earth Life on Mars? Mars missions Life on Europa? The giant planets and their moons3.1. Overview and

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 17Life on MarsFour chief ways to detect life on Mars Use powerful telescopes to search the planet for any large scale structures, or changes with time, that could be ascribed to the efforts of a technically advanced

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 28The formation of EarthAccretion: Era of bombardment Differentiation: higher-density material (iron, nickel) sank toward the center while lower-density material rose toward the surface Planetary Heating: Accretion /

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 15Frequency of Meteor Impacts on EarthImpact frequency depends on the size of the impactor, note that smaller impacts are much more frequent than larger onesComets and Asteroids may have contributed towards the inv

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 23Possibility of Life on Jupiter Hydrogen-rich environment (similar to the conditions on the primitive Earth), however, Jupiter, 318 times Earths mass, keeps hydrogen from escaping, i.e., Jupiter has a huge number of

Caltech - AS - 3012

AS3012: Exoplanetary ScienceStephen Kane srk1 Room 226AS3012: Exoplanetary Science Detection Techniques How can we discover extrasolar planets? Characteristics of the exoplanet population Planet formation Explaining the properties of exoplane

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 25Living cells are carbon-basedChemical composition of the human body by weight This composition is fairly typical of all living matter on Earth Most of the oxygen in living cells is actually part of water The mole

Caltech - AST - 2037

ASTRO 2037 Life in the UniverseStephen Kane392-2052 Ext. 250 skane@astro.ufl.edu 312 Bryant Space Science CenterAstro 2037 Spring 07, Lecture 01Astro 2037 outline Three lectures per week: Tuesday 9:35am 10:25am Thursday 9:35am 10:25am, 10:40

Caltech - AS - 3012

AS3012: Exoplanetary ScienceStephen Kane srk1 Room 226Detection Methods Covered So Far(1) Direct methods (2) Astrometry position (3) Radial velocity motion (4) Transits brightness Effects of a planet on the parent star (5) Gravitational lensi

Caltech - AST - 2037

Astro 2037 Spring 07, Lecture 03Habitability of Mars Public debate about Martian canals and cities end in 1965 NASA's Mariner 4 spacecraft sent to Mars and flew to within 6000 miles of the martian surface A few dozen television-quality images of

Caltech - BI - 145

Blood and Body DefensesJim Pierce Bi 145a Lecture 10, 2007-08BloodBlood is a connective tissueCells Extracellular MatrixBloodHematopoeisis in uteroHematopoeisis in uteroHematopoiesisBi 214 HematopoiesisGreat model of: A Developm

Caltech - G - 060597

MASSACHUSETTS INSTITUTE OF TECHNOLOGYSPECTROSCOPY LABORATORYApplication of LIGO Technology to Biomedical OpticsKeisuke Goda Quantum Measurement Group @ MIT, LIGO Collaboration with MIT Spectroscopy Lab and Massachusetts General HospitalLIGO Sem

Caltech - G - 060597

MASSACHUSETTS INSTITUTE OF TECHNOLOGYSPECTROSCOPY LABORATORYApplication of LIGO Technology to Biomedical OpticsKeisuke Goda Quantum Measurement Group @ MIT, LIGO Collaboration with MIT Spectroscopy Lab and Massachusetts General HospitalLIGO Sem

Caltech - LAW - 134

20 Biotechnology Law Report 678 Number 5 (October 2001) Mary Ann Liebert, Inc.Stem Cells: Ethics, Law and PoliticsALEXANDER MORGAN CAPRON*Over the past three years, human stem cells have moved from being something of esoteric interest for basi

Caltech - BI - 122

Organelles and prionsCentromeres ensure the proper segregation of genes during mitosis and meiosis. !Molecules that not linked to chromosomes bearing nuclear centromeres behave differently during mitosis and do not obey Mendel's rules.! !Organell

Caltech - APH - 150

APh150: Physics of Biological Structure and FunctionWinter 2003When: To be determined Who: You and me (Rob Phillips, x 3374, phillips@aero.caltech.edu, 221 Steele) Where: 104 Watson What: See below! How: Lecture twice a week and weekly homework. No

Caltech - BI - 145

Cardiovascular PhysiologyWhere Does the Flow Go?Jim Pierce Bi 145a Lecture 17, 2008-09Afterload: Getting Flow out of the Heart The Cardiac Output is the total flow out of the heart per time. Each time the heart pumps, it pumps out a stroke vol

Caltech - BI - 145

ProblemSet#5,Bi145a DueWednesday,November19,2008 Pleaseplaceeachproblemofthehomeworkonaseparatepage.Thatway, JimandtheTAscangradethehomeworkcontemporaneously. 1) Theoriginaldescriptionofnormallevelsofredbloodcellsin humanscamefromexaminationsofafewdo

Caltech - BI - 145

Syllabus Part 3This handout should contain my extra notes on general and specific cell physiology. These are only additional notes. Please refer to the required and recommended references for further detail on discussed topics. Required Reading: Ber

Caltech - BI - 145

Problem Set #2, Bi 145a Due Wednesday, October 15, 2008 Please place each problem of the homework on a separate page. That way, Jim and the TA's can grade the homework contemporaneously. 1) Cells are exposed to many forces. a) Give an example of

Minnesota - SOC - 0087

The Death of Till Death Us Do Part Pinsof 2002What is the main cause of ending a marriage?Death1974Divorce Marriage becomes an object of therapeutic intervention and scientific inquiryMarriage is defined as pair-bonding, potentially procr

Minnesota - PSY - 3061

Outline Cortex Efferent pathways Muscles When things go wrongLecture 11Motor System and Movement Keep in mind that the flow of information is opposite to sensory systemsIntro to Motor System Like sensory systems, hierarchical organization

Minnesota - PSY - 3061

Assignment 15Name _Know your drugs: Below are three classes of drugs. For each class, list one drug that is representative of that class, the neurotransmitter or receptor that is involved in its action, and one "typical" effect of that class. NOT

Minnesota - PSY - 3061

LeftRight1 2 3 4 5LGNLGNWeekly Assignment 7Name_See what you can see: On the previous page is a diagram of the primary visual pathway. At the top of the page is the visual field. The left half of the visual field is red, and the right h

Minnesota - PSY - 3061

Lecture 10Other SensesOutline Olfaction Gustation SomatosensationOlfaction Odorants are airborne chemicals Olfactory mucosa (epithelium) smelling slime in which olfactory receptor cells are embedded Each receptor cell contains many recept

Minnesota - PSY - 3135

Annu. Rev. Genet. 2001. 35:83101 Copyright c 2001 by Annual Reviews. All rights reservedSIR FRANCIS GALTON AND THE BIRTH OF EUGENICSNicholas W. GillhamAnnu. Rev. Genet. 2001.35:83-101. Downloaded from arjournals.annualreviews.org by University of

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Minnesota - AREND - 011

College Student Achievement and Persistence Resources for Professional Development2006 David R. Arendale, Ph.D., Asst Prof, College of Education & Human Development, Univ. of Minnesota; David@Arendale.orgAssociations and Organizations (Profit & No

Minnesota - CALV - 0016

0022-3565/03/3052-733739$7.00 THE JOURNAL OF PHARMACOLOGY AND EXPERIMENTAL THERAPEUTICS Copyright 2003 by The American Society for Pharmacology and Experimental Therapeutics JPET 305:733739, 2003Vol. 305, No. 2 47829/1060199 Printed in U.S.A.Kin

Minnesota - WANG - 0808

=Zhiyong Wang=1015 29th Ave SE, Apt.FMinneapolis, MN 55414Cell phone: (612) 387-0575Email: wang0808@umn.edu-OBJECTIVE-Research Chemist / Research Scientist / Materials Scientist in industry--QUALIFICATIONS-Ph.D. in Materials

Minnesota - ENT - 5241

Ecological Risk AssessmentEnt 5241/ WRS 5241 University of Minnesota Fall 2006, D. A. Andow Class 7. Exposure Characterization, Part I I. Analysis Phase A. Exposure Characterization B. Adverse Effects Characterization C. Leads to Risk Characterizati