Ph110B-15
| Differences between revisions 44 and 51 (spanning 7 versions) | Back to page |
|
Size: 1444
Comment:
|
Size: 1134
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 5: | Line 5: |
| * In solutions to homework 6, there may be some helpful general thing to read, in addition to finding solutions to problems. This is regarding the general notion of an angular profile diagram. Please read pages 11-12 of the solutions to homework 6 for (hopefully helpful) discussion on this.—~-''<<DateTime(2015-05-21T14:50:01-0700)>>''-~ * Please note a small but important [[Homework+#Homework|correction to homework 6]].—~-''<<DateTime(2015-05-18T15:57:06-0700)>>''-~ |
* 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)>>''-~ |
| Line 9: | Line 7: |
| * The midterm exam and its solutions are [[Homework+|posted here]].—~-''<<DateTime(2015-05-12T13:50:57-0700)>>''-~ | * The final exam is [[Homework+|here]]. Good luck!—~-''<<DateTime(2015-06-05T10:02:14-0700)>>''-~ |
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.