Fundamentals of Plasma Physics Basic concepts

Size: px
Start display at page:

Download "Fundamentals of Plasma Physics Basic concepts"

Transcription

1 Fundamentals of Plasma Physics Basic concepts APPLAuSE Instituto Superior Técnico Instituto de Plasmas e Fusão Nuclear Vasco Guerra

2 Since the dawn of Mankind men has tried to understand plasma physics...

3

4

5

6

7 Plasmas: The As basic perguntas o questions início fundamentais What is plasma? How is plasma created? Why is plasma interesting? What is plasma good for?

8 O What que As is é perguntas plasma? um plasma? fundamentais Ionized gas Quasi-neutral Exhibits collective behavior The potential energy of a typical particle is much smaller than its kinetic energy

9 Para que serve um plasma? Plasmas in nature 99% of the (visible) matter in the universe! Stars Nebulae Solar wind Ionosphere van Allen belts Lightning Aurora

10 The origin of the word plasma The word was introduced in 1928 by Irving Langmuir Langmuir, Oscillations in ionized gases, Proc. Nat. Acad. Sci. U.S. (1928) From the Greek πλάσμα (to mould), since the brightness of Crookes discharge tubes moulds to the shape of the tube Analogy with blood plasma... we have observed some phenomena of remarkable beauty which may prove to be of theoretical interest. Langmuir, Science (1924) 60 p 392

11 Como se forma um plasma? How is plasma created?

12 Quatro estados da matéria... e não Four As states... perguntas or four fundamentais elements??? quatro elementos!

13 Para que serve um plasma? How to produce a plasma? Increase the temperature Use non equilibrium to locally increase ne -photoionisation -electric discharges

14 Why is plasma interesting? Light electrons, tend to have high temperatures, while the ions, heavier, tend to have low temperatures (non equilibrium!) Reactions that normally can occur only at high temperatures can take place at low temperatures! Plasma emits UV and visible radiation Plasmas are useful for nearly everything!

15 Para What As que is perguntas plasma serve um good fundamentais plasma? for? For nearly everything!

16 Para que serve um plasma? Plasma applications Thermonuclear fusion Plasma propulsion Gas lasers Micro and nanoelectronics Depollution Biology and medicine Processing of materials Particle acceleration

17 Nuclear fusion Lawson s criterion: nτ>10 20 m -3 s

18 Magnetic confinement fusion

19 Inertial fusion

20 Fundamentals Debye shielding Plasma frequency Plasma parameter Ionization degree

21 Debye shielding Test charge: positive ion, infinite mass Attracts the electrons and repels the other positive ions The electron density in the vicinity increases A negative charge cloud forms - shielding - which tends to cancel the test charge

22 Debye shielding Electrostatic potential (r) = 1 Q T 4 0 r Debye potential ( adiabatic response ) (r) = 1 Q T 4 0 r exp rd

23 Debye shielding D = 0kT n 0 e 2 1/2 Quasi-neutrality does not hold inside a Debye sphere

24 Debye shielding The phenomenon is known as Debye shielding and is the first exemple of a plasma collective behavior The hypothesis of the typical particle s potential energy being much smaller than its kinetic energy is used in the linearization of Poisson s equation

25 Debye shielding Debye s potential due to a charge in a plasma decays much faster than in vacuum For r λd the shielding cancels qt and φ(r) 0 qt does not have to be a special particle: each charged particle in the plasma tends to establish its own shielding cloud Plasma condition: λd L (typical dimension of the system) quasi-neutral

26 Debye shielding Some typical values

27 Plasma parameter Distance between neighbouring particles ~ n 1/3 0 Potencial energy due to the closest neighbour ~ 1 4 " 0 e 2 r 1 " 0 n 1/3 0 e 2 Typical kinetic energy ~ 1 2 m v2 = 3 2 kt e Plasma condition: = n 0 3 D 1 Plasma: number of electrons in a Debye cube >>1

28 Ionization degree Plasma can coexist with another state In the ionosphere there are regions where 99% of the gas is neutral and only 1% is ionized We have then a partially ionized plasma The plasma parameter Λ is calculated only with the ionized component (and we have Λ>>1 and λd L) Usually there is a continuous exchange of charge between the particles of the neutral gas and the ones of the ionized plasm Medium is characterized by the ionization degree, ne/(ne+n0)

29 Plasma frequency E Oscillatory motion of angular frequency ωpe=

30 Plasma frequency It is one more example of collective behavior We can define a ionic plasma frequency and a total plasma frequency, ωp 2= ωpi 2 +ωpe 2 To have a plasma, the collective behavior must dominate over the individual collisions Plasma condition: ωpe νc (electron-neutral collision frequency), or ωpeτ 1

31 How to study plasmas? Single particle motion Kinetic equations Fluid equations

32 The wonderful world of plasmas!

33 Voyager I

34

Fundamentals of Plasma Physics Transport in weakly ionized plasmas

Fundamentals of Plasma Physics Transport in weakly ionized plasmas Fundamentals of Plasma Physics Transport in weakly ionized plasmas APPLAuSE Instituto Superior Técnico Instituto de Plasmas e Fusão Nuclear Luís L Alves (based on Vasco Guerra s original slides) 1 As perguntas

More information

Plasma Astrophysics Chapter 1: Basic Concepts of Plasma. Yosuke Mizuno Institute of Astronomy National Tsing-Hua University

Plasma Astrophysics Chapter 1: Basic Concepts of Plasma. Yosuke Mizuno Institute of Astronomy National Tsing-Hua University Plasma Astrophysics Chapter 1: Basic Concepts of Plasma Yosuke Mizuno Institute of Astronomy National Tsing-Hua University What is a Plasma? A plasma is a quasi-neutral gas consisting of positive and negative

More information

Introduction. Chapter Plasma: definitions

Introduction. Chapter Plasma: definitions Chapter 1 Introduction 1.1 Plasma: definitions A plasma is a quasi-neutral gas of charged and neutral particles which exhibits collective behaviour. An equivalent, alternative definition: A plasma is a

More information

Lecture 2. Introduction to plasma physics. Dr. Ashutosh Sharma

Lecture 2. Introduction to plasma physics. Dr. Ashutosh Sharma Preparation of the concerned sectors for educational and R&D activities related to the Hungarian ELI project Ion acceleration in plasmas Lecture 2. Introduction to plasma physics Dr. Ashutosh Sharma Zoltán

More information

Lecture Note 1. 99% of the matter in the universe is in the plasma state. Solid -> liquid -> Gas -> Plasma (The fourth state of matter)

Lecture Note 1. 99% of the matter in the universe is in the plasma state. Solid -> liquid -> Gas -> Plasma (The fourth state of matter) Lecture Note 1 1.1 Plasma 99% of the matter in the universe is in the plasma state. Solid -> liquid -> Gas -> Plasma (The fourth state of matter) Recall: Concept of Temperature A gas in thermal equilibrium

More information

The ideal Maxwellian plasma

The ideal Maxwellian plasma The ideal Maxwellian plasma Dr. L. Conde Departamento de Física Aplicada. E.T.S. Ingenieros Aeronáuticos Universidad Politécnica de Madrid Plasmas are,... The plasma state of matter may be defined as a

More information

xkcd.com It IS about physics. It ALL is.

xkcd.com It IS about physics. It ALL is. xkcd.com It IS about physics. It ALL is. Introduction to Space Plasmas! The Plasma State What is a plasma? Basic plasma properties: Qualitative & Quantitative Examples of plasmas! Single particle motion

More information

Figure 1.1: Ionization and Recombination

Figure 1.1: Ionization and Recombination Chapter 1 Introduction 1.1 What is a Plasma? 1.1.1 An ionized gas A plasma is a gas in which an important fraction of the atoms is ionized, so that the electrons and ions are separately free. When does

More information

Space Plasma Physics Thomas Wiegelmann, 2012

Space Plasma Physics Thomas Wiegelmann, 2012 Space Plasma Physics Thomas Wiegelmann, 2012 1. Basic Plasma Physics concepts 2. Overview about solar system plasmas Plasma Models 3. Single particle motion, Test particle model 4. Statistic description

More information

xkcd.com It IS about physics. It ALL is.

xkcd.com It IS about physics. It ALL is. xkcd.com It IS about physics. It ALL is. Introduction to Space Plasmas The Plasma State What is a plasma? Basic plasma properties: Qualitative & Quantitative Examples of plasmas Single particle motion

More information

PLASMA: WHAT IT IS, HOW TO MAKE IT AND HOW TO HOLD IT. Felix I. Parra Rudolf Peierls Centre for Theoretical Physics, University of Oxford

PLASMA: WHAT IT IS, HOW TO MAKE IT AND HOW TO HOLD IT. Felix I. Parra Rudolf Peierls Centre for Theoretical Physics, University of Oxford 1 PLASMA: WHAT IT IS, HOW TO MAKE IT AND HOW TO HOLD IT Felix I. Parra Rudolf Peierls Centre for Theoretical Physics, University of Oxford 2 Overview Why do we need plasmas? For fusion, among other things

More information

Fundamentals of Plasma Physics

Fundamentals of Plasma Physics Fundamentals of Plasma Physics Definition of Plasma: A gas with an ionized fraction (n i + + e ). Depending on density, E and B fields, there can be many regimes. Collisions and the Mean Free Path (mfp)

More information

Atomic and Nuclear Physics Review (& other related physics questions)

Atomic and Nuclear Physics Review (& other related physics questions) Atomic and Nuclear Physics Review (& other related physics questions) 1. The minimum electron speed necessary to ionize xenon atoms is A. 2.66 10 31 m/s B. 5.15 10 15 m/s C. 4.25 10 12 m/s D. 2.06 10 6

More information

Space Physics. An Introduction to Plasmas and Particles in the Heliosphere and Magnetospheres. May-Britt Kallenrode. Springer

Space Physics. An Introduction to Plasmas and Particles in the Heliosphere and Magnetospheres. May-Britt Kallenrode. Springer May-Britt Kallenrode Space Physics An Introduction to Plasmas and Particles in the Heliosphere and Magnetospheres With 170 Figures, 9 Tables, Numerous Exercises and Problems Springer Contents 1. Introduction

More information

Quasi-neutral limit for Euler-Poisson system in the presence of plasma sheaths

Quasi-neutral limit for Euler-Poisson system in the presence of plasma sheaths in the presence of plasma sheaths Department of Mathematical Sciences Ulsan National Institute of Science and Technology (UNIST) joint work with Masahiro Suzuki (Nagoya) and Chang-Yeol Jung (Ulsan) The

More information

Roman Marcarelli, Class of Physics and Math. Investigation of Laser Wakefield Acceleration in Plasmas

Roman Marcarelli, Class of Physics and Math. Investigation of Laser Wakefield Acceleration in Plasmas Roman Marcarelli, Class of 2019 Physics and Math Investigation of Laser Wakefield Acceleration in Plasmas Biographical Sketch My name is Roman Marcarelli, and I m a junior math and physics major in the

More information

Uppsala universitet Institutionen för astronomi och rymdfysik Anders Eriksson

Uppsala universitet Institutionen för astronomi och rymdfysik Anders Eriksson Tentamen för Rymdfysik I 2006-08-15 Uppsala universitet Institutionen för astronomi och rymdfysik Anders Eriksson Please write your name on all papers, and on the first page your address, e-mail and phone

More information

A note on the plasma sheath and the Bohm Criterion

A note on the plasma sheath and the Bohm Criterion A note on the plasma sheath and the Bohm Criterion G.D. Severn Dept. of Physics, University of San Diego, San Diego CA 92110 (Dated: April 6, 2006) PACS numbers: 52.27.Aj, 52.27.Cm The word sheath in connection

More information

Chapter 1 Nature of Plasma

Chapter 1 Nature of Plasma Chapter 1 Nature of Plasma Abstract Charge neutrality is one of fundamental property of plasma. Section 1.2 explains Debye length λ D in (1.2), a measure of shielding distance of electrostatic potential,

More information

Sensors Plasma Diagnostics

Sensors Plasma Diagnostics Sensors Plasma Diagnostics Ken Gentle Physics Department Kenneth Gentle RLM 12.330 k.gentle@mail.utexas.edu NRL Formulary MIT Formulary www.psfc.mit.edu/library1/catalog/ reports/2010/11rr/11rr013/11rr013_full.pdf

More information

Physics Important Terms and their Definitions

Physics Important Terms and their Definitions Physics Important Terms and their S.No Word Meaning 1 Acceleration The rate of change of velocity of an object with respect to time 2 Angular Momentum A measure of the momentum of a body in rotational

More information

The Sun Our Extraordinary Ordinary Star

The Sun Our Extraordinary Ordinary Star The Sun Our Extraordinary Ordinary Star 1 Guiding Questions 1. What is the source of the Sun s energy? 2. What is the internal structure of the Sun? 3. How can astronomers measure the properties of the

More information

An Overview of the Details

An Overview of the Details The Sun Our Extraordinary Ordinary Star 1 Guiding Questions 1. What is the source of the Sun s energy? 2. What is the internal structure of the Sun? 3. How can astronomers measure the properties of the

More information

Plasma & Fusion on Earth: merging age-old natural phenomena into your present and future

Plasma & Fusion on Earth: merging age-old natural phenomena into your present and future Plasma & Fusion on Earth: merging age-old natural phenomena into your present and future Presented by Rick Lee Chief Operator, DIII-D Operations Manager, Energy/Fusion Outreach Program General Atomics

More information

Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi. Lecture No. #01 Introduction to Plasmas

Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi. Lecture No. #01 Introduction to Plasmas Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi Lecture No. #01 Introduction to Plasmas Today, we begin a series of lectures on plasma physics. My first

More information

Introduction to Plasma Physics

Introduction to Plasma Physics Introduction to Plasma Physics Hartmut Zohm Max-Planck-Institut für Plasmaphysik 85748 Garching DPG Advanced Physics School The Physics of ITER Bad Honnef, 22.09.2014 A simplistic view on a Fusion Power

More information

Introduction to Plasma Physics. Emilia Kilpua and Hannu Koskinen

Introduction to Plasma Physics. Emilia Kilpua and Hannu Koskinen Introduction to Plasma Physics Emilia Kilpua and Hannu Koskinen HK, 11.12.2015 2 Contents 1 Introduction 3 1.1 General definition and occurrence....................... 3 1.2 Brief history of plasma physics........................

More information

An Overview of the Details

An Overview of the Details Guiding Questions The Sun Our Extraordinary Ordinary Star 1. What is the source of the Sun s energy? 2. What is the internal structure of the Sun? 3. How can astronomers measure the properties of the Sun

More information

Chapter IX: Nuclear fusion

Chapter IX: Nuclear fusion Chapter IX: Nuclear fusion 1 Summary 1. General remarks 2. Basic processes 3. Characteristics of fusion 4. Solar fusion 5. Controlled fusion 2 General remarks (1) Maximum of binding energy per nucleon

More information

PLASMA ASTROPHYSICS. ElisaBete M. de Gouveia Dal Pino IAG-USP. NOTES: (references therein)

PLASMA ASTROPHYSICS. ElisaBete M. de Gouveia Dal Pino IAG-USP. NOTES:  (references therein) PLASMA ASTROPHYSICS ElisaBete M. de Gouveia Dal Pino IAG-USP NOTES:http://www.astro.iag.usp.br/~dalpino (references therein) ICTP-SAIFR, October 7-18, 2013 Contents What is plasma? Why plasmas in astrophysics?

More information

PHYS 312. Basic Plasma Physics

PHYS 312. Basic Plasma Physics Physics 312 Basic Plasma Physics 1 PHYS 312. Basic Plasma Physics Time: 3:15-4:30, Tuesday, Thursday Place: SEQ Teaching Center room 101 Instructor: Alexander Kosovichev e-mail: sasha@quake.stanford.edu

More information

purposes is highly encouraged.

purposes is highly encouraged. The following slide show is a compilation of slides from many previous similar slide shows that have been produced by different members of the fusion and plasma physics education community. We realize

More information

Langmuir Probes as a Diagnostic to Study Plasma Parameter Dependancies, and Ion Acoustic Wave Propogation

Langmuir Probes as a Diagnostic to Study Plasma Parameter Dependancies, and Ion Acoustic Wave Propogation Langmuir Probes as a Diagnostic to Study Plasma Parameter Dependancies, and Ion Acoustic Wave Propogation Kent Lee, Dean Henze, Patrick Smith, and Janet Chao University of San Diego (Dated: May 1, 2013)

More information

Collisions and transport phenomena

Collisions and transport phenomena Collisions and transport phenomena Collisions in partly and fully ionized plasmas Typical collision parameters Conductivity and transport coefficients Conductivity tensor Formation of the ionosphere and

More information

Astronomy Chapter 12 Review

Astronomy Chapter 12 Review Astronomy Chapter 12 Review Approximately how massive is the Sun as compared to the Earth? A. 100 times B. 300 times C. 3000 times D. 300,000 times E. One million times Approximately how massive is the

More information

Application of Plasma Phenomena Lecture /3/21

Application of Plasma Phenomena Lecture /3/21 Application of Plasma Phenomena Lecture 3 2018/3/21 2018/3/21 updated 1 Reference Industrial plasma engineering, volume 1, by J. Reece Roth, Chapter 8-13. Plasma physics and engineering, by Alexander Fridman

More information

Introduction to Theoretical Plasma Physics

Introduction to Theoretical Plasma Physics Karl-Heinz Spatschek Introduction to Theoretical Plasma Physics October 14, 2008 Only for personal use! Chapter 1 Introduction A plasma is a many body system of a huge number of interacting (charged and

More information

Introductory Lecture on Plasmas EEG 783. Robert A. Schill, Jr. University of Nevada Las Vegas

Introductory Lecture on Plasmas EEG 783. Robert A. Schill, Jr. University of Nevada Las Vegas Introductory Lecture on Plasmas EEG 783 Robert A. Schill, Jr. University of Nevada Las Vegas States of Matter Four Naturally Occurring States of Matter Solids, Liquids, Gas, Plasmas Solids Condense matter

More information

Stellar evolution Part I of III Star formation

Stellar evolution Part I of III Star formation Stellar evolution Part I of III Star formation The interstellar medium (ISM) The space between the stars is not completely empty, but filled with very dilute gas and dust, producing some of the most beautiful

More information

Lectures on basic plasma physics: Introduction

Lectures on basic plasma physics: Introduction Lectures on basic plasma physics: Introduction Department of applied physics, Aalto University Compiled: January 13, 2016 Definition of a plasma Layout 1 Definition of a plasma 2 Basic plasma parameters

More information

Matti Laan Gas Discharge Laboratory University of Tartu ESTONIA

Matti Laan Gas Discharge Laboratory University of Tartu ESTONIA Matti Laan Gas Discharge Laboratory University of Tartu ESTONIA Outline 1. Ionisation 2. Plasma definition 3. Plasma properties 4. Plasma classification 5. Energy transfer in non-equilibrium plasma 6.

More information

ELECTROSTATICS. When two materials rub together the contact between their surfaces may cause: a) the surfaces to become hot and show wear and tear.

ELECTROSTATICS. When two materials rub together the contact between their surfaces may cause: a) the surfaces to become hot and show wear and tear. 1 ELECTROSTATICS Friction And Charge When two materials rub together the contact between their surfaces may cause: a) the surfaces to become hot and show wear and tear. b) the surfaces to become attracted

More information

The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star

The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star The Sun Closest star to Earth - only star that we can see details on surface - easily studied Assumption: The Sun is a typical star Why is the Sun hot and bright? Surface Temperature of the Sun: T =

More information

Optical Pumping of Rubidium

Optical Pumping of Rubidium Optical Pumping of Rubidium Janet Chao, Dean Henze, Patrick Smith, Kent Lee April 27, 2013 Abstract 1 INTRODUCTION Irving Langmuir coined the term plasma in a paper in 1928, ushering a whole new and exciting

More information

Waves and Instabilities in Dusty Plasmas

Waves and Instabilities in Dusty Plasmas 15 th Topical Conference on RF Power in Plasmas May 20 22, 2003 Jackson Hole, Wyoming Waves and Instabilities in Dusty Plasmas Bob Merlino University of Iowa Outline What is a dusty plasma? Where are dusty

More information

PHYS 780. Basic Plasma Physics

PHYS 780. Basic Plasma Physics Phys780: Plasma Physics Lecture 1: Basic concepts 1 PHYS 780. Basic Plasma Physics Time: 1:00 pm -2:25 pm, U.S. Eastern Time, Monday, Wednesday Location: GITC 1403, on-line via VYDEO (Students will receive

More information

Spectroscopy and Molecular Emission. Fundamental Probes of Cold Gas

Spectroscopy and Molecular Emission. Fundamental Probes of Cold Gas Spectroscopy and Molecular Emission Fundamental Probes of Cold Gas Atomic Lines Few atoms have fine structure transitions at low enough energy levels to emit at radiofrequencies Important exceptions HI

More information

Plasma Physics Prof. Vijayshri School of Sciences, IGNOU. Lecture No. # 38 Diffusion in Plasmas

Plasma Physics Prof. Vijayshri School of Sciences, IGNOU. Lecture No. # 38 Diffusion in Plasmas Plasma Physics Prof. Vijayshri School of Sciences, IGNOU Lecture No. # 38 Diffusion in Plasmas In today s lecture, we will be taking up the topic diffusion in plasmas. Diffusion, why do you need to study

More information

Plasma Spectroscopy Inferences from Line Emission

Plasma Spectroscopy Inferences from Line Emission Plasma Spectroscopy Inferences from Line Emission Ø From line λ, can determine element, ionization state, and energy levels involved Ø From line shape, can determine bulk and thermal velocity and often

More information

CHAPTER 29: STARS BELL RINGER:

CHAPTER 29: STARS BELL RINGER: CHAPTER 29: STARS BELL RINGER: Where does the energy of the Sun come from? Compare the size of the Sun to the size of Earth. 1 CHAPTER 29.1: THE SUN What are the properties of the Sun? What are the layers

More information

THE SUN AND THE SOLAR SYSTEM

THE SUN AND THE SOLAR SYSTEM Chapter 26 THE SUN AND THE SOLAR SYSTEM CHAPTER 26 SECTION 26.1: THE SUN S SIZE, HEAT, AND STRUCTURE Objectives: What is the Sun s structure and source of energy? Key Vocabulary: Fusion Photosphere Corona

More information

Notes on fusion reactions and power balance of a thermonuclear plasma!

Notes on fusion reactions and power balance of a thermonuclear plasma! SA, 3/2017 Chapter 5 Notes on fusion reactions and power balance of a thermonuclear plasma! Stefano Atzeni See S. Atzeni and J. Meyer-ter-Vehn, The Physics of Inertial Fusion, Oxford University Press (2004,

More information

FUNDAMENTALS OF PHYSICS - Vol. I Plasmas - Julio J. Martinell, Rafael Navarro-Gonzalez, and Alejandro C. Raga

FUNDAMENTALS OF PHYSICS - Vol. I Plasmas - Julio J. Martinell, Rafael Navarro-Gonzalez, and Alejandro C. Raga PLASMAS Julio J. Martinell, Rafael Navarro-Gonzalez, and Alejandro C. Raga Plasma Physics Department, ICN, UNAM, México D. F., Mexico Keywords: Ionized gas, interstellar medium, star formation, solar wind,

More information

Collision Processes. n n The solution is 0 exp x/ mfp

Collision Processes. n n The solution is 0 exp x/ mfp Collision Processes Collisions mediate the transfer of energy and momentum between various species in a plasma, and as we shall see later, allow a treatment of highly ionized plasma as a single conducting

More information

ELECTROHYDRODYNAMICS IN DUSTY AND DIRTY PLASMAS

ELECTROHYDRODYNAMICS IN DUSTY AND DIRTY PLASMAS ELECTROHYDRODYNAMICS IN DUSTY AND DIRTY PLASMAS Gravito-Electrodynamics and EHD by HIROSHI KIKUCHI Institute for Environmental Electromagnetics, Tokyo, Japan KLUWER ACADEMIC PUBLISHERS DORDRECHT / BOSTON

More information

The Sun sends the Earth:

The Sun sends the Earth: The Sun sends the Earth: Solar Radiation - peak wavelength.visible light - Travels at the speed of light..takes 8 minutes to reach Earth Solar Wind, Solar flares, and Coronal Mass Ejections of Plasma (ionized

More information

9-1 The Sun s energy is generated by thermonuclear reactions in its core The Sun s luminosity is the amount of energy emitted each second and is

9-1 The Sun s energy is generated by thermonuclear reactions in its core The Sun s luminosity is the amount of energy emitted each second and is 1 9-1 The Sun s energy is generated by thermonuclear reactions in its core The Sun s luminosity is the amount of energy emitted each second and is produced by the proton-proton chain in which four hydrogen

More information

Dispersive Media, Lecture 7 - Thomas Johnson 1. Waves in plasmas. T. Johnson

Dispersive Media, Lecture 7 - Thomas Johnson 1. Waves in plasmas. T. Johnson 2017-02-14 Dispersive Media, Lecture 7 - Thomas Johnson 1 Waves in plasmas T. Johnson Introduction to plasmas as a coupled system Magneto-Hydro Dynamics, MHD Plasmas without magnetic fields Cold plasmas

More information

1. What is the minimum energy required to excite a mercury atom initially in the ground state? ev ev ev

1. What is the minimum energy required to excite a mercury atom initially in the ground state? ev ev ev Page 1 of 10 modern bank Name 25-MAY-05 1. What is the minimum energy required to excite a mercury atom initially in the ground state? 1. 4.64 ev 3. 10.20 ev 2. 5.74 ev 4. 10.38 ev 2. The diagram represents

More information

MODERN PHYSICS OF PLASMAS (19 lectures)

MODERN PHYSICS OF PLASMAS (19 lectures) UNIT OF STUDY OUTLINE (PHYS 3021, 3921, 3024, 3924, 3025, 3925) MODERN PHYSICS OF PLASMAS (19 lectures) Course coordinator and principal lecturer: Dr Kostya (Ken) Ostrikov Lecturer (normal student stream,

More information

Discovered by German scientist Johann Hittorf in 1869 and in 1876 named by Eugen Goldstein.

Discovered by German scientist Johann Hittorf in 1869 and in 1876 named by Eugen Goldstein. DO PHYSICS ONLINE CATHODE RAYS CATHODE RAYS (electron beams) Streams of electrons (negatively charged particles) observed in vacuum tubes - evacuated glass tubes that are equipped with at least two metal

More information

MATHEMATICAL MODELS OF LIFE SUPPORT SYSTEMS - Vol. I - Mathematical Models of Plasma Physics - N.N.Kalitkin, D.P.Kostomarov

MATHEMATICAL MODELS OF LIFE SUPPORT SYSTEMS - Vol. I - Mathematical Models of Plasma Physics - N.N.Kalitkin, D.P.Kostomarov MATHEMATICAL MODELS OF PLASMA PHYSICS N.N.Kalitkin Institute for Mathematical Modeling of Russian Academy of Science, Moscow, Russia Lomonosov Moscow State University, Moscow, Russia Keywords: Plasma,

More information

Physique des plasmas radiofréquence Pascal Chabert

Physique des plasmas radiofréquence Pascal Chabert Physique des plasmas radiofréquence Pascal Chabert LPP, Ecole Polytechnique pascal.chabert@lpp.polytechnique.fr Planning trois cours : Lundi 30 Janvier: Rappels de physique des plasmas froids Lundi 6 Février:

More information

Measuring velocity of ion acoustic waves through plasma Hannah Saddler, Adam Egbert, and Warren Mardoum

Measuring velocity of ion acoustic waves through plasma Hannah Saddler, Adam Egbert, and Warren Mardoum Measuring velocity of ion acoustic waves through plasma Hannah Saddler, Adam Egbert, and Warren Mardoum (Dated: 11 December 2015) This experiment aimed to measure velocity of ion acoustic waves propagating

More information

Introduction to Theoretical and Applied Plasma Chemistry

Introduction to Theoretical and Applied Plasma Chemistry 1 Introduction to Theoretical and Applied Plasma Chemistry 1.1. PLASMA AS THE FOURTH STATE OF MATTER Although the term chemistry in the title of the book does not require a special introduction, the term

More information

ELECTROMAGNETIC WAVES

ELECTROMAGNETIC WAVES VISUAL PHYSICS ONLINE MODULE 7 NATURE OF LIGHT ELECTROMAGNETIC WAVES SPECTRA PRODUCED BY DISCHARGE TUBES CATHODE RAYS (electron beams) Streams of electrons (negatively charged particles) observed in vacuum

More information

Physical Processes in Astrophysics

Physical Processes in Astrophysics Physical Processes in Astrophysics Huirong Yan Uni Potsdam & Desy Email: hyan@mail.desy.de 1 Reference Books: Plasma Physics for Astrophysics, Russell M. Kulsrud (2005) The Physics of Astrophysics, Frank

More information

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e +

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e + β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Last Lecture: Radioactivity, Nuclear decay Radiation damage This lecture: nuclear physics in medicine and fusion and fission Final

More information

Experimental Investigations of Magnetic Reconnection. J Egedal. MIT, PSFC, Cambridge, MA

Experimental Investigations of Magnetic Reconnection. J Egedal. MIT, PSFC, Cambridge, MA Experimental Investigations of Magnetic Reconnection J Egedal MIT, PSFC, Cambridge, MA Coronal Mass Ejections Movie from NASA s Solar Dynamics Observatory (SDO) Space Weather The Solar Wind affects the

More information

Cosmic Rays - R. A. Mewaldt - California Institute of Technology

Cosmic Rays - R. A. Mewaldt - California Institute of Technology Cosmic Rays - R. A. Mewaldt - California Institute of Technology Cosmic rays are high energy charged particles, originating in outer space, that travel at nearly the speed of light and strike the Earth

More information

The Physics of Fluids and Plasmas

The Physics of Fluids and Plasmas The Physics of Fluids and Plasmas An Introduction for Astrophysicists ARNAB RAI CHOUDHURI CAMBRIDGE UNIVERSITY PRESS Preface Acknowledgements xiii xvii Introduction 1 1. 3 1.1 Fluids and plasmas in the

More information

Physics 11b Lecture #10

Physics 11b Lecture #10 Physics 11b Lecture #10 Magnetic Fields S&J Chapter 29 What We Did Last Time Electromotive forces (emfs) atteries are made of an emf and an internal resistance Resistor arithmetic R = R + R + R + + R series

More information

is the minimum stopping potential for which the current between the plates reduces to zero.

is the minimum stopping potential for which the current between the plates reduces to zero. Module 1 :Quantum Mechanics Chapter 2 : Introduction to Quantum ideas Introduction to Quantum ideas We will now consider some experiments and their implications, which introduce us to quantum ideas. The

More information

The Structure of the Sun. CESAR s Booklet

The Structure of the Sun. CESAR s Booklet How stars work In order to have a stable star, the energy it emits must be the same as it can produce. There must be an equilibrium. The main source of energy of a star it is nuclear fusion, especially

More information

Currently, the largest optical telescope mirrors have a diameter of A) 1 m. B) 2 m. C) 5 m. D) 10 m. E) 100 m.

Currently, the largest optical telescope mirrors have a diameter of A) 1 m. B) 2 m. C) 5 m. D) 10 m. E) 100 m. If a material is highly opaque, then it reflects most light. absorbs most light. transmits most light. scatters most light. emits most light. When light reflects off an object, what is the relation between

More information

The Sun Our Star. Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun

The Sun Our Star. Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun The Sun Our Star Properties Interior Atmosphere Photosphere Chromosphere Corona Magnetism Sunspots Solar Cycles Active Sun General Properties Not a large star, but larger than most Spectral type G2 It

More information

Our sun is the star in our solar system, which lies within a galaxy (Milky Way) within the universe. A star is a large glowing ball of gas that

Our sun is the star in our solar system, which lies within a galaxy (Milky Way) within the universe. A star is a large glowing ball of gas that Our sun is the star in our solar system, which lies within a galaxy (Milky Way) within the universe. A star is a large glowing ball of gas that generates energy through nuclear fusion in its core. The

More information

Structural Modifications of Cyclotron to Produce New Therapeutic & Diagnostic Particles

Structural Modifications of Cyclotron to Produce New Therapeutic & Diagnostic Particles Global Science and Technology Journal Vol. 5. No. 1. September 2017 Issue. Pp. 16-22 Structural Modifications of Cyclotron to Produce New Therapeutic & Diagnostic Particles BimanTanvir Ahmed *, Ramit Azad

More information

Kinetic modelling of the jet extraction mechanism in spherical IEC devices

Kinetic modelling of the jet extraction mechanism in spherical IEC devices Kinetic modelling of the jet extraction mechanism in spherical IEC devices Type of activity: Standard study 1 Background & Study Motivation 1.1 Introduction Inertial Electrostatic Confinement (IEC) devices

More information

Why study plasma astrophysics?

Why study plasma astrophysics? Why study plasma astrophysics? Nick Murphy and Xuening Bai Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics January 25, 2016 Today s plan Definition of a plasma Plasma astrophysics:

More information

How Do Stars Appear from Earth?

How Do Stars Appear from Earth? How Do Stars Appear from Earth? Magnitude: the brightness a star appears to have from Earth Apparent Magnitude depends on 2 things: (actual intrinsic brightness) The color of a star is related to its temperature:

More information

Ay Fall 2004 Lecture 6 (given by Tony Travouillon)

Ay Fall 2004 Lecture 6 (given by Tony Travouillon) Ay 122 - Fall 2004 Lecture 6 (given by Tony Travouillon) Stellar atmospheres, classification of stellar spectra (Many slides c/o Phil Armitage) Formation of spectral lines: 1.excitation Two key questions:

More information

2/8/16 Dispersive Media, Lecture 5 - Thomas Johnson 1. Waves in plasmas. T. Johnson

2/8/16 Dispersive Media, Lecture 5 - Thomas Johnson 1. Waves in plasmas. T. Johnson 2/8/16 Dispersive Media, Lecture 5 - Thomas Johnson 1 Waves in plasmas T. Johnson Introduction to plasma physics Magneto-Hydro Dynamics, MHD Plasmas without magnetic fields Cold plasmas Transverse waves

More information

CHAPTER 27. Continuum Emission Mechanisms

CHAPTER 27. Continuum Emission Mechanisms CHAPTER 27 Continuum Emission Mechanisms Continuum radiation is any radiation that forms a continuous spectrum and is not restricted to a narrow frequency range. In what follows we briefly describe five

More information

Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi

Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi Lecture No. # 03 DC Conductivity and Negative Differential Conductivity Well friends, in this lecture, I

More information

Our sole source of light and heat in the solar system. A very common star: a glowing g ball of gas held together by its own gravity and powered

Our sole source of light and heat in the solar system. A very common star: a glowing g ball of gas held together by its own gravity and powered The Sun Visible Image of the Sun Our sole source of light and heat in the solar system A very common star: a glowing g ball of gas held together by its own gravity and powered by nuclear fusion at its

More information

Low Temperature Plasma Technology Laboratory

Low Temperature Plasma Technology Laboratory Low Temperature Plasma Technology Laboratory CENTRAL PEAKING OF MAGNETIZED GAS DISCHARGES Francis F. Chen and Davide Curreli LTP-1210 Oct. 2012 Electrical Engineering Department Los Angeles, California

More information

Contents. 2. Fluids. 1. Introduction

Contents. 2. Fluids. 1. Introduction Contents 1. Introduction 2. Fluids 3. Physics of Microfluidic Systems 4. Microfabrication Technologies 5. Flow Control 6. Micropumps 7. Sensors 8. Ink-Jet Technology 9. Liquid Handling 10.Microarrays 11.Microreactors

More information

The Sun. How are these quantities measured? Properties of the Sun. Chapter 14

The Sun. How are these quantities measured? Properties of the Sun. Chapter 14 The Sun Chapter 14 The Role of the Sun in the Solar System > 99.9% of the mass Its mass is responsible for the orderly orbits of the planets Its heat is responsible for warming the planets It is the source

More information

MAE 5595: Space Environments and Spacecraft Interactions. Lesson 4: Introduction

MAE 5595: Space Environments and Spacecraft Interactions. Lesson 4: Introduction MAE 5595: Space Environments and Spacecraft Interactions Lesson 4: Introduction Ambient Environment Neutral Environment Low pressure environment (150km ~ 3x10-9 atm) Ambient neutral gas (LEO atomic oxygen)

More information

Plasma waves in the fluid picture I

Plasma waves in the fluid picture I Plasma waves in the fluid picture I Langmuir oscillations and waves Ion-acoustic waves Debye length Ordinary electromagnetic waves General wave equation General dispersion equation Dielectric response

More information

Unit 1: Space. Section 2- Stars

Unit 1: Space. Section 2- Stars Unit 1: Space Section 2- Stars Stars Recall: stars are celestial bodies of hot gas that give off heat and light Stars The milky way contains hundreds of billions of stars and is only one of hundreds of

More information

Neutron Stars. Neutron Stars and Black Holes. The Crab Pulsar. Discovery of Pulsars. The Crab Pulsar. Light curves of the Crab Pulsar.

Neutron Stars. Neutron Stars and Black Holes. The Crab Pulsar. Discovery of Pulsars. The Crab Pulsar. Light curves of the Crab Pulsar. Chapter 11: Neutron Stars and Black Holes A supernova explosion of an M > 8 M sun star blows away its outer layers. Neutron Stars The central core will collapse into a compact object of ~ a few M sun.

More information

4 Discuss and evaluate the 5th state of matter. 3 - Differentiate among the four states of matter in terms of energy,

4 Discuss and evaluate the 5th state of matter. 3 - Differentiate among the four states of matter in terms of energy, Goal: Differentiate among the four states of matter in terms of energy, particle motion, and phase transitions. 4 States of Mater Sections 3.1, 3.2 4 Discuss and evaluate the 5 th state of matter. 3 -

More information

AP PHYSICS 2 FRAMEWORKS

AP PHYSICS 2 FRAMEWORKS 1 AP PHYSICS 2 FRAMEWORKS Big Ideas Essential Knowledge Science Practices Enduring Knowledge Learning Objectives ELECTRIC FORCE, FIELD AND POTENTIAL Static Electricity; Electric Charge and its Conservation

More information

Pulsars. Table of Contents. Introduction

Pulsars. Table of Contents. Introduction Pulsars Table of Contents Introduction... 1 Discovery...2 Observation...2 Binary Pulsars...3 Pulsar Classes... 3 The Significance of Pulsars... 3 Sources...4 Introduction Pulsars are neutron stars which

More information

The Physics of Plasmas

The Physics of Plasmas The Physics of Plasmas T.J.M. BOYD University of Essex J.J. SANDERSON University of St Andrews PUBLISHED BY THE PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE The Pitt Building, Trumpington Street, Cambridge,

More information

The Sun. the main show in the solar system. 99.8% of the mass % of the energy. Homework due next time - will count best 5 of 6

The Sun. the main show in the solar system. 99.8% of the mass % of the energy. Homework due next time - will count best 5 of 6 The Sun the main show in the solar system 99.8% of the mass 99.9999...% of the energy 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Homework due next time - will count best 5 of 6 The

More information

IEPC M. Bodendorfer 1, K. Altwegg 2 and P. Wurz 3 University of Bern, 3012 Bern, Switzerland. and

IEPC M. Bodendorfer 1, K. Altwegg 2 and P. Wurz 3 University of Bern, 3012 Bern, Switzerland. and Future thruster application: combination of numerical simulation of ECR zone and plasma X-ray Bremsstrahlung measurement of the SWISSCASE ECR ion source IEPC-2009-234 Presented at the 31st International

More information

A Polywell p+11b Power Reactor Joel G. Rogers, Ph.D.

A Polywell p+11b Power Reactor Joel G. Rogers, Ph.D. A Polywell p+11b Power Reactor Joel G. Rogers, Ph.D. rogersjg@telus.net Aneutronic fusion is the holy grail of fusion power research. A new method of operating Polywell was developed which maintains a

More information