'Dust particle' diaporamas de présentation

VCE PHYSICS

VCE PHYSICS. Unit 4 Topic 3 SOUND. UNIT OUTLINE. To achieve this outcome students should demonstrate the knowledge and skills to; explain sound as the transmission of energy via longitudinal pressure waves;

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Clicker Questions for Wave unit

Clicker Questions for Wave unit. I gave these clicker questions after the activity was completed except for the Wave interference demonstration day. Waves on a String. A. A. 1. If you advance the movie one frame, the knot at point A would be in the same place higher lower

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UFOs in the LHC

UFOs in the LHC. CERN MAC #4 Tobias Baer August, 12 th 2011.

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update on UFOs: 2012 Observations , Studies and Extrapolations

update on UFOs: 2012 Observations , Studies and Extrapolations. LBOC Tobias Baer July, 24 th 2012 .

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Catch the Wave

Catch the Wave. Welcome. Fact. or. Fiction. The distance light travels in a year is about 6,000,000,000,000 miles. Fact or Fiction. Light Travels 2. That is a fact . The distance from the Earth to the Sun is about 1,400,000,000 meters. Fact or Fiction. That is fiction.

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Discovering Computers 2011

Discovering Computers 2011. Chapter 6 Computer Storage Issues . Chapter Objectives. Next. Differentiate among CD-ROMs, recordable CDs, rewritable CDs, DVD-ROMs, BD-ROMs, HD DVD-ROMs, recordable DVDs, and rewritable DVDs. Differentiate between storage devices and storage media.

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Chapter 1. Concepts of Motion

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Effect of supra thermal electrons on particle charge in RF sheath

Effect of supra thermal electrons on particle charge in RF sheath. A.A.Samarian and S.V. Vladimirov School of Physics, University of Sydney, NSW 2006, Australia. Outlines. Charge vs Size dependence The experimental dependence of the dust charge as a function of its size

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Zdeslav Hrepic Dean A. Zollman N. Sanjay Rebello

Zdeslav Hrepic Dean A. Zollman N. Sanjay Rebello. Students' Mental Models of Sound Propagation. 125 th AAPT National Meeting Boise, Idaho. Kansas State University Physics Education Research Group. Supported by NSF ROLE Grant # REC-0087788. Research Questions.

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PHYS 101

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Damping of the dust particle oscillations at very low neutral pressure

Damping of the dust particle oscillations at very low neutral pressure. M. Pustylnik, N. Ohno, S.Takamura, R. Smirnov. Introduction. In the linear approximation the motion of a dust particle trapped in a sheath is described by the harmonic oscillator equation:.

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Warm Up

Warm Up. Scientific Notation. Algebra I Seminar. Do You Recognize These Numbers?. The Speed of light! The mass of a dust particle! The mass of a proton! The revolutions of a turntable! The volume of a raindrop!. 300,000,000 m/sec. 0.000 000 000 753 kg

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CHE 12 Bonding review

CHE 12 Bonding review. Particles in Chemistry. Particles in Chemistry. Atoms (very tiny: trillions of atoms in a speck of dust) Ions (also very tiny: approximately atomic-sized)

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Shelby Karis Amanda

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Dust-Beam interaction in the LHC vacuum chamber

Dust-Beam interaction in the LHC vacuum chamber. SUPERVISOR: FRANK ZIMMERMANN. Outline of the talk. Background Dust particle dynamics Beam lifetime Future work. Introduction.

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Sound

Sound. A dust particle is floating in front of a loud speaker. When the speaker is turned on, the particle will. Move up and down. Be pushed away from the speaker. Move side to side. Not move at all. Move in a circular path. None of these is correct.

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Introduction

Figure 1: (below) a T-Tauri star with an accretion disk. The accretion disk is the source of gas (and maybe dust) ejected to form Herbig-Haro objects Figure 2: (right) diagram of a Herbig-Haro object. a. b. c.

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