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       WebAssign key: csub 4947 6222

Practice Exam 1

Practice Exam 2

Practice Exam 3 with Key

Lab 1: "Coffee" cooling

Lab 2: Specific Heat of Metals

Lab 3: Latent Heat of Fusion

Lab 4: Voltage, Current, and Resistance in a DC Circuit

Lab 5: Resistances in Series and Parallel

Lab 6: Voltage vs Time across an Unknown Capacitor

Lab 7: Force on a Current-Carrying Conductor in a Magnetic Field

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

 

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

Ch 30  Sources of the Magnetic Field

Ch 31  Faraday's Law