Phys222 Classical Physics II
Spring 2008


<a href=http://www.hq.nasa.gov/hpcc/insights/vol5/helio.htm >Magnetic field of the Sun</a>

NASA:  Magnetic field lines (white) and magnetic field strength (low = blue to high = red) due to Coronal Mass Ejections (CME's) from the Sun.
CME's are gigantic bubbles of ionized hydrogen and electrons.

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Syllabus
Thermodynamics and Statistical Physics
 
Ch 19  Thermal Physics
Ch 20  Heat and the First Law of Thermodynamics
Ch 21  The Kinetic Theory of Gases
Ch 22
  Heat Engines, Entropy, and the Second Law of Thermodynamics

 

Electricity and Magnetism
 
         Homework Assignment
Ch 23  Electric Fields
Ch 24  Gauss's Law
Ch 25  Electric Potential
Ch 26  Capacitance and Dielectrics
Ch 27  Current and Resistance
Ch 28  Direct Current Circuits
Ch 29  Magnetic Fields
 

 
 

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