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Opening Remarks Why the details? Not everything I said is included in the slides. Please pay attention to the lectures and catch the most essential points. Form your own opinions and thoughts. Should ask questions. Try to attend classes as much as you can.

Opening Remarks

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Opening Remarks. Why the details? Not everything I said is included in the slides. Please pay attention to the lectures and catch the most essential points. Form your own opinions and thoughts. Should ask questions. Try to attend classes as much as you can. Let us make a deal. - PowerPoint PPT Presentation

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Page 1: Opening Remarks

Opening Remarks

• Why the details?• Not everything I said is

included in the slides.• Please pay attention to the

lectures and catch the most essential points.

• Form your own opinions and thoughts.

• Should ask questions.• Try to attend classes as

much as you can.

Page 2: Opening Remarks

Let us make a deal.

• Turn off your cell phone during the class.• Do not conduct private conversation.• If you have questions, you may directly

ask me.• If you have urgent need to leave the

room, you are excused. Otherwise do not leave the classroom frequently.

• After several classes we should have a review session. Druing the meeting let us exchange ideas about the teaching.

Page 3: Opening Remarks

Let me reiterate:

• Most of the stuff I discuss during the class may not be found in standard textbooks.

• The Universiy gives me this teaching task and responsibility. Personally I take it seriously.

• I sincerely wish that you can learn something new from this course. Let us work ogether and optimize the result.

Page 4: Opening Remarks

Graduate Courses

• Normal and regular courses

Designed for basic education and training.

• Special topic courses

Expectations are very different. My responsibility is to introduce some new and special stuff. My duty is to promote kinetic theory and space plasma physics.

Page 5: Opening Remarks

About the title of the course

• “Nonlinear processes in space plasmas”

• “Space plasma physics and kinetic instabilities”

Page 6: Opening Remarks

Planning & Rationale

• Basic and general theory• Theories of plasma instabilities• Discussion of several important

phenomena in space physics

Page 7: Opening Remarks

Introducing Plasma Physics

Page 8: Opening Remarks

Space Plasma Physics & Plasma Astrophysics

• Plasma physics was initially advanced for controlled thermonuclear fusion research.

• There are special processes that mainly occur in space plasmas. Space plasma physics is a field basically developed for understnading space ans astrophysical plasmas.

Page 9: Opening Remarks

The birth of plasma physics

• Plasma is an ionized gas.• Charged particles can be affected by

electric and magnetic fields.• It was thought that plasma may be

studied in a similar way as we dealt with a neutral gas which is generally treated as a fluid.

• Since a neutral gas may be studied with hydrodynamics, plasma may be considered as a conducting fluid.

Page 10: Opening Remarks

• As a result, magnetohydrodynamics was born.

• MHD theory was unsuccessful in fusion experiments in mid 1950s.

• Kinetic theory began to attract attention.• Discovery of numerous new instabilities

that pushes the birh of modern plasma

physics.

Page 11: Opening Remarks

Why ?

Scientists gradually realize that the basic physical property of plasmas is critically different from that of a neutral gas.

Page 12: Opening Remarks

How ?

• In a neutral gas inter-particle collisions dominate but in a plasma wave-particle interactions prevail.

• There exist many instabilities in plasmas while very few instabilities occur in gases.

• Plasma turbulence can greatly modify the physics of a plasma. As a result, many new physical processes can take place in plasmas that are not possible in gases.

Page 13: Opening Remarks

• In plasmas there are many wave modes.• Instabilities imply that these wave modes

can be amplified. The enhanced waves can result in nonlinear processes that can change the fundamental property.

• Particle-particle interactions are much less important than the interactions of waves with particles.

• There are many other reasons.

Consequently we must recognize plasma physics is a new branch of physics, and in general plasmas should not be treated as a gas.

Page 14: Opening Remarks

A Landmark Work

• A paper by L. D. Landau was published in 1946.

• In this paper Landau showed that Langmuir wave may be damped while there are no collisions.

• Later on this paper led to the realization of wave-particle resonance.

• It also led to the discovery of kinetic instabilities in plasmas.

Page 15: Opening Remarks

Why plasma physics is important to space physics and

astrophysics?

The reason is simple:

In stellar and solar atmosphere, in interstellar or interplanetary space plasma is everywhere. How can one understand the physics in these regions without the knowledge of plasma physics?

Page 16: Opening Remarks

Three approaches to study plasmas

• Single particle dynamics

• MHD and fluid theories

• Kinetic theory

Page 17: Opening Remarks

Why kinetic theory is important?

• Many physical processes in plasmas depend on microscopic particle motion.

• However, fluid dynamics considers only averaged particle motion.

• And single particle dynamics cannot represent an ensemble of particles.

• Kinetic theory seems to be the best tool available to study plasma physics.

Page 18: Opening Remarks

Force Fields

• Gravitational field• Electric and magnetic fields• Ambient or background field• Fields associated with waves• Self-consistent fields

Page 19: Opening Remarks

In fluid dynamics theory

• Density, velocity and pressure are all functions of coordinates space that is dimensional.

• All physical quantities and the force fields are statistically averaged.

• As a result, the theory does not and cannot describe microscopic particle motion.

Page 20: Opening Remarks

Commonly use terms in kinetic theory

• Phase space• Distribution function • Probability density • Kinetic equation• Fokker-Planck equation• Lenard-Balescu equation• Vlasov equation

Page 21: Opening Remarks

Conclusion

• Fluid theory may be useful if we only want to study dynamic issues.

• However, if we want to explain some important phenomena and understand the underlying physics, fluid dynamics theory is not sufficient.

• Remember: plasma is very different from an ordinary gas.

Page 22: Opening Remarks

Density and Fields

• In real space particles move randomly. • Microscopic fields and density fluctuate

in time and space.• Concept of phase space is important.• Only statistical averaged quantities are

of interest.• Kinetic theory is developed for this goal.

Page 23: Opening Remarks

Microscopic Picture

• In a real plasma fields and particle density are random microscopic quantities.

• All particles are moving stochastically. • However, each particle is governed by the

equation of motion which is controlled by microscopic fields are .

• Each particle moves continuously in phase space.

Page 24: Opening Remarks

Intermission

Page 25: Opening Remarks

Phase-Space Orbit

( , , )tr p

'( '), '( '), 't t tr p

Page 26: Opening Remarks

Continuity Equation