Ph110B-15
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| <<fl(W)>>elcome to the 2nd part of Classical Electrodynamics! Many of you are familiar to me from my past teaching, but some of you are new to me. I am glad to see ''everyone''! I extend my best wishes for your effective efforts in this course, and I hope that you will have fun while learning by challening yourself. | * Here is <<ln(https://gweon.com/forum/questions/?from_all=true&tags=final-exam,"the link")>> to all final exam related questions on the forum.—~-''<<DateTime(2015-06-05T13:17:21-0700)>>''-~ |
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| * The syllabus has been updated with the correct office hour information. However, there is no office hour today (Mar 31), as I have a dentist appointment.—~-''<<DateTime(2015-03-31T12:12:16-0700)>>''-~ | * The final exam is [[Homework+|here]]. Good luck!—~-''<<DateTime(2015-06-05T10:02:14-0700)>>''-~ |
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| <<h(<div style="margin-top: -1.0em; text-align: right;">)>>~-[[OldNews|Archived news items can be found here]].-~<<h(</div>)>> |
Welcome to Phys 110B, 2015!
Here is <<ln: execution failed [Cannot have arguments without name following named arguments] (see also the log)>> to all final exam related questions on the forum.—1:17PM, Jun 05, 2015
The final exam is here. Good luck!—10:02AM, Jun 05, 2015
What is this course about?
Classical electrodynamics is all about the light. And electrons and other charged particles... In this course, we will start with Maxwell's equations—something of a monument in the history of physics—and study some conclusions that we can draw from them. By doing so, we will learn about the light, or the electronmagnetic field, and its interaction with charged particles within the realm of “classical” physics. We will learn conservation principles, waves, radiation, and end with the special relativistic view of light.