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.
Syllabus
WebAssign key: csub 3738 9223 and csub 0374 5533 for the Updated Technology edition
Practice Exam 1
Quiz 1: Scores
Exam 1: Scores
Exam 1: Key
Practice Exam 2
Quiz 2: Scores
Quiz 2: Key
Exam 2: Scores
Exam 2: Key
Practice Exam 3 with Key
Quiz 3_1 Monday Scores
Quiz 3_1 Monday Key
Quiz 3_2 Rest of Week Scores
Quiz 3_2 Rest of Week Key
Exam 3: Scores
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 CurrentCarrying 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
