Spring 2011
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.
Files are password required.
SyllabusLab 1: "Coffee" cooling Lab 2: Latent Heat of Fusion Lab 3: Voltage vs Time across an Unknown Capacitor
Sample materials Quiz 1: Grades Quiz 1: KeysExam 1: Grades Exam 1: Keys Quiz 2: Grades Quiz 2: Keys Exam 2: Grades Exam 2: Keys Final Exam: Grades Final Exam: Keys Final Grades
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 Ch 30 Sources of the Magnetic Field Ch 31 Faraday's Law