Space Physics and Space Weather Space: “empty” volume between bodies (solid bodies are excluded) Space physics: space within solar system (astrophysics.

Slides:



Advertisements
Similar presentations
The divergence of E If the charge fills a volume, with charge per unit volume . R Where d is an element of volume. For a volume charge:
Advertisements

Motion of a Charged Particle in a Magnetic Field
Physics of fusion power
Chapter 26: The Magnetic Field
Winter Quarter 2009 Vassilis Angelopoulos Robert Strangeway Date Topic [Instructor] 1/5 Organization and Introduction to Space Physics I [A&S] 1/7 Introduction.
The Beginning of Modern Astronomy
Chapter 29 Magnetic Fields.
PH0101 UNIT 2 LECTURE 2 Biot Savart law Ampere’s circuital law
AS 4002 Star Formation & Plasma Astrophysics BACKGROUND: Maxwell’s Equations (mks) H (the magnetic field) and D (the electric displacement) to eliminate.
EE3321 ELECTROMAGENTIC FIELD THEORY
The Movement of Charged Particles in a Magnetic Field
Single particle motion and trapped particles
ESS 7 Lecture 14 October 31, 2008 Magnetic Storms
Space Weather. Coronal loops Intense magnetic field lines trap plasma main_TRACE_loop_arcade_lg.jpg.
Physics of fusion power Lecture 6: Conserved quantities / Mirror device / tokamak.
Wednesday, Oct. 26, 2005PHYS , Fall 2005 Dr. Jaehoon Yu 1 PHYS 1444 – Section 003 Lecture #16 Wednesday, Oct. 26, 2005 Dr. Jaehoon Yu Charged Particle.
Electricity&… Magnetism Review of Coulomb`s Force,Magnetic Fields and Magnetic Force Lecture 22 Monday: 5 April 2004.
Reinisch_ Solar Terrestrial Relations (Cravens, Physics of Solar Systems Plasmas, Cambridge U.P.) Lecture 1- Space Environment –Matter in.
Magnetospheric Morphology Prepared by Prajwal Kulkarni and Naoshin Haque Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global.
Physics 121: Electricity & Magnetism – Lecture 9 Magnetic Fields Dale E. Gary Wenda Cao NJIT Physics Department.
Magnetism July 2, Magnets and Magnetic Fields  Magnets cause space to be modified in their vicinity, forming a “ magnetic field ”.  The magnetic.
K L University 1. 2 MAGNETOSTATICS 3 Introduction to Magneto statics – Magnetic field, Magnetic force, Magnetic flux Biot-Savat’s law -- Applications.
Certain objects and circuits produce magnetic fields Magnetic fields, like electric fields, are vector fields They have a magnitude and a direction Denoted.
Chapter 21 & 22 Electric Charge Coulomb’s Law This force of repulsion or attraction due to the charge properties of objects is called an electrostatic.
26. Magnetism: Force & Field. 2 Topics The Magnetic Field and Force The Hall Effect Motion of Charged Particles Origin of the Magnetic Field Laws for.
Chapter 28 Magnetic Fields Key contents Magnetic fields and the Lorentz force The Hall effect Magnetic force on current The magnetic dipole moment.
ESS 7 Lectures 10, 11 and 12 October 22, 24, and 27 The Magnetosphere.
Physics of fusion power Lecture 7: particle motion.
Tuija I. Pulkkinen Finnish Meteorological Institute Helsinki, Finland
Magnetism 1. 2 Magnetic fields can be caused in three different ways 1. A moving electrical charge such as a wire with current flowing in it 2. By electrons.
General electric flux definition
Chapter 19 Magnetism 1. Magnets 2. Earth’s Magnetic Field 3. Magnetic Force 4. Magnetic Torque 5. Motion of Charged Particles 6. Amperes Law 7. Parallel.
Van Allen Radiation Belts The Van Allen radiation belts consist of charged particles surrounding the Earth in doughnut-shaped regions. The particles are.
Space Physics and Space Weather Space: “empty” volume between bodies (solid bodies are excluded) Space physics: space within solar system (astrophysics.
Introduction to Space Weather
Science topics Magnetism Magnetism Sun spots Sun spots Solar flares Solar flares Corona mass ejections Corona mass ejections.
ASEN 5335 Aerospace Environments -- Radiation Belts1 The Radiation Belts A radiation belt is a population of energetic particles stably-trapped by the.
Magnetic Field A magnetic field is a region in which a body with magnetic properties experiences a force.
Magnetism B B B x x x x x x ® ® ® ® ® ­ ­ ­ ­ ­ ­ ­ ­ v v v ´ q q q F
Space Physics and Space Weather
Chapter 19 Magnetism. General Physics Review – Magnetic Fields ELECTRIC FIELDS From (+) to (–) charges Field lines (electric flux) Start / End at charges.
P212c28: 1 Chapter 28: Magnetic Field and Magnetic Forces Iron ore found near Magnesia Compass needles align N-S: magnetic Poles North (South) Poles attracted.
Chapter 29 Magnetic Fields 1.Introduction to magnetic field. 2.The forces on moving charges and currents inside a magnetic field. 3.The math that will.
Winter Quarter 2008 Christopher T. Russell Raymond J. Walker Date Topic 1/7 Organization and Introduction to Space Physics I 1/9 Introduction to Space.
Magnetic Forces. * Current-carrying wires have magnetic fields and… * Magnets exert forces on other magnets. Therefore… Magnets exert forces on current-carrying.
Radiation belt particle dynamics Prepared by Kevin Graf Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network.
Magnetic Forces. Forces in Magnetism The existence of magnetic fields is known because of their affects on moving charges. What is magnetic force (F B.
1 Chapter 19: Magnetism The nature of magnetism Iron ore found near Magnesia Compass needles align N-S: magnetic Poles North (South) Poles attracted to.
ESS 7 Lecture 2 September 29, 2008 A Little History.
Magnetism: Force and Field. General Characteristics Like poles repel Unlike poles attract You can never isolate a north pole from a south pole. N S N.
Magnetic Forces. The Force on a Moving Charge in a Magnetic Field Just as current-carrying wires (a stream of moving charges) experience a force in a.
ASEN 5335 Aerospace Environments -- Magnetospheres 1 As the magnetized solar wind flows past the Earth, the plasma interacts with Earth’s magnetic field.
Certain objects and circuits produce magnetic fields Magnetic fields, like electric fields, are vector fields They have a magnitude and a direction Denoted.
PHY 102: Lecture Magnetic Field 6.2 Magnetic Force on Moving Charges 6.3 Magnetic Force on Currents 6.4 Magnetic Field Produced by Current.
Physics Chapter 21: Magnetism. ☺Magnets ☺Caused by the Polarization of Iron Molecules ☺Material Containing Iron (Fe)
ELEN 340 Electromagnetics II Lecture 2: Introduction to Electromagnetic Fields; Maxwell’s Equations; Electromagnetic Fields in Materials; Phasor Concepts;
Introduction to Plasma Physics and Plasma-based Acceleration
Solar Magnetic Fields. Capacitors in Circuits Charge takes time to move through wire  V is felt at the speed of light, however Change in potential across.
Particle in uniform B-field
Electric Field & Magnetic Field
The Movement of Charged Particles in a Magnetic Field
Single particle motion and trapped particles
Chapter 3 Plasma as fluids
Space Physics and Space Weather
Introduction to Space Weather
General Physics (PHY 2140) Lecture 14 Electricity and Magnetism
Earth’s Ionosphere Lecture 13
Magnetic Fields Exert Forces on Moving Charges
LECTURE I: SINGLE-PARTICLE MOTIONS IN ELECTRIC AND MAGNETIC FIELDS
Magnetosphere: Structure and Properties
Presentation transcript:

Space Physics and Space Weather Space: “empty” volume between bodies (solid bodies are excluded) Space physics: space within solar system (astrophysics is not space physics) Solar-terrestrial relations: space physics focused on solar wind and terrestrial space Space plasma physics: application of plasma physics to space Space physics: Coriolis force and gravity not important (unless noted) Space weather: space physics applications. Space phenomena that endanger space assets and applications and human in space Space physics: electromagnetic field + charged particles Require significant math: –Working on but not solving partial differential equations in this class –Vector operations Require: electromagnetics (additional reading may help)

Regions in Space Solar wind (sun’s atmosphere, but not bonded by gravity): plasma (ions and electrons in equal number but not attached to each other) stream flows out continuously, but with variations, from the sun with extremely high speeds into the interplanetary space. Note: in space, all ions are positively charged. Formation of the magnetosphere: the solar wind disturbs geomagnetic field; geomagnetic field deflects solar wind. If there is no SW SW effect on the geomagnetic field

Regions in Space Magnetopause: the boundary separates the magnetosphere from the solar wind (crucial for any solar wind entry). Bow shock: standing upstream of the magnetopause, because the solar wind is highly supersonic. Magnetosheath: the region between the bow shock and the magneto- pause. Magnetotail: the mag- netosphere is stretched by the solar wind on the nightside.

Radiation belts: where most energetic particles are trapped, (major issue for space mission safety). Regions in Space

Plasmasphere: inner part of magnetosphere (1000km – 4 Earth radii) with higher plasma density of ionospheric origin. Ionosphere: (80 ~ 1000 km) regions of high density of charged particles of earth origin. Thermosphere: (> 90 km) neutral component of the same region as the ionosphere. The temperature can be greater than 1000 K. Regions in Space

Space Weather Phenomena Magnetic storms (hurricanes in space) Global-scale long-lasting geomagnetic disturbances Magnetic substorms (tornadoes in space) Impulsive geomagnetic disturbances Auroras (rains from space) Enhanced energetic particle precipitations associated with storms/substorms Ionospheric plasma density disturbances (fog?) Destruction of the layered structure of the ionosphere.

Evidence for Space Processes Aurora: emissions caused by high energy charged particle precipitation into the upper atmosphere from space. Geomagnetic field: caused by electric currents below the earth’s surface. Geomagnetic storm/substorm: period of large geomagnetic disturbances. Periodicity of magnetic storms: ~ 27 days. Rotation of the Sun: 26 ~ 27 days.

Space physics started with observations of the aurora. –Old Testament references to auroras. –Greek literature speaks of “moving accumulations of burning clouds” –Chinese literature has references to auroras prior to 2000BC

–Galileo theorized that aurora is caused by air rising out of the Earth’s shadow to where it could be illuminated by sunlight. (Note he also coined the name aurora borealis meaning “northern dawn”.) –Descartes thought they are reflections from ice crystals. –Halley suggested that auroral phenomena are ordered by the Earth’s magnetic field. –In 1731 the French philosopher de Mairan suggested they are connected to the solar atmosphere.

By the 11th century the Chinese had learned that a magnetic needle points north-south. By the 12th century the European records mention the compass. That there was a difference between true north and the direction of the compass needle (declination) was known by the 16th century. William Gilbert (1600) realized that the field was dipolar. In 1698 Edmund Halley organized the first scientific expedition to map the field in the Atlantic Ocean.

Plasma A plasma is an electrically neutral ionized gas. –The Sun is a plasma –Interplanetary medium: the space between the Sun and the Earth is “filled” with a plasma. –The Earth is surrounded by plasmas: magnetosphere, ionosphere. –Planetary magnetospheres, ionospheres –A stroke of lightning forms plasma –Over 99% of the Universe is plasma. Although neutral a plasma is composed of charged particles- electric and magnetic forces are critical to understand plasmas. Plasma physics: three descriptions –Single particle theory –Fluid theory –Kinetic theory

Forces on charged particles (single particle theory) –Electric force F E = qE –Magnetic force F B = qv x B –Lorentz force F = qE + qv x B –Neutral forcesF g =mg,

Negative Charge Positive Charge Use right hand rule to find the direction of F. F=q v x B

Single Particle Motion SI Units –mass (m) - kg –length (l) - m –time (t) - s –electric field (E) - V/m –magnetic field (B) - T –velocity (v) - m/s –F g stands for non-electromagnetic forces (e.g. gravity) - usually ignorable.

–If q is positive particle gyrates in left handed sense –If q is negative particle gyrates in a right handed sense

Gyro motion –The gyro radius is a function of energy. –Energy of charged particles is usually given in electron volts (eV) –Energy that a particle with the charge of an electron gets in falling through a potential drop of 1 Volt- 1 eV = 1.6X Joules (J). Energies in space plasmas go from electron Volts to kiloelectron Volts (1 keV = 10 3 eV) to millions of electron Volts (1 meV = 10 6 eV) Cosmic energies go to gigaelectron Volts ( 1 geV = 10 9 eV). The circular motion does no work on a particle Only the electric field can energize particles!

Electric Field Added to a Plasma (B=0) E external

Homework 2.13, 2.15 (no (d) for under), 2.16, 2.18, 2.4* Errors in the book. –2.4, gamma => 1/gamma –2.13, page 32, line 2 above the figure, delB=-3B/r –2.15, alpha is a constant, not pitch angle. –2.18, 10^6 km, not used. –2.18: assume parallel for curvature drift and perpendicular for gradient drift –2.18, Hint: radius of curvature: calculus.

Lecture II

Pitch angle and magnetic moment

Single particle theory: guiding center drift The electric field can modify the particles motion. –Assume but still uniform and F g =0. –Frequently in space physics it is ok to set Only can accelerate particles along Positive particles go along and negative particles go along Eventually charge separation wipes out – has a major effect on motion. As particle gyrates it moves along and gains energy Later in the circle it losses energy. This causes different parts of the “circle” to have different radii - it doesn’t close on itself. Drift velocity is perpendicular to and No charge dependence, (electrons and ions move in the direction and speed) therefore no currents

Drift Motion: General Form Any force capable of accelerating and decelerating charged particles can cause them to drift. –If the force is charge independent the drift motion will depend on the sign of the charge and can form perpendicular currents.

Electric and Magnetic Fields: Simple situations Single electric charge (monopole): –Positive charge –Negative charge –Net charge –E field (intensity): + => - Electric dipole No magnetic monopole. Magnetic field (magnetic dipole) –Magnet: N and S (pointing to), geomagnetic poles: located oppositely, –B (mag flux density, including magnetization): N=>S –(H: mag field intensity) –current loop E and B are chosen in plasma physics because of the Lorentz force.

Maxwell’s Equations Maxwell’s equations –Poisson’s Equation (originally from Coulomb's law) E is the electric field  is the electric charge density  0 is the electric permittivity (8.85 X Farad/m) Positive charge starts electric field line Negative charge ends the line. –Gauss Law (absence of magnetic monopoles) B is the magnetic field Magnetic field line has neither beginning nor end.

Maxwell’s Equations (II) –Faraday’s Law –Ampere’s Law c is the speed of light.  0 is the permeability of free space, H/m J is the current density  0  0 = 1/c 2

Integral Form of Maxwell’s Equations Maxwell’s equations in integral form –A is the area, dA is the differential element of area –n is a unit normal vector to dA pointing outward. –V is the volume, dV is the differential volume element –n’ is a unit normal vector to the surface element dF in the direction given by the right hand rule for integration around C, and is magnetic flux through the surface. –ds is the differential element around C. Gauss’ integral theorem

Nonuniform B Field: Gradient B drift

Centrifugal Force: Curvature drift

Adiabatic Invariants

Magnetic mirrors The two components are related as required by the divergence-free of the magnetic field

The force is along B and away from the direction of increasing B. If and kinetic energy must be conserved a decrease in must yield an increase in Particles will turn around when

Magnetic bottle bounce period

In general, the second adiabatic invariant –The integral of the parallel momentum over one complete bounce between mirrors is constant (as long as B doesn’t change much in a bounce). –Using conservation of energy and the first adiabatic invariant –If the field is a dipole their trajectories will take them around the planet and close on themselves.

The third adiabatic invariant –As particles bounce they will drift because of gradient and curvature drift motion. –As long as the magnetic field doesn’t change much in the time required to drift around a planet the magnetic flux inside the orbit must be constant.

Limitations on the invariants –  is constant when there is little change in the field’s strength over a cyclotron path. –All invariants require that the magnetic field not change much in the time required to one cycle of motion where  is the orbit period.

The Concept of the Guiding Center –Separates the motion (v) of a particle into motion perpendicular (v  ) and parallel ( v || ) to the magnetic field. –To a good approximation the perpendicular motion can consist of a drift (u D ) and the gyromotion ( v  c ) –Over long times the gyromotion is averaged out and the particle motion can be described by the guiding center motion consisting of the parallel motion and drift.