Here's a partial list of the resources out there in your quest to become a better teacher.
Never forget this! Your peers, Head GSI, course head, and random older graduate students all have teaching experience. You can bounce ideas off them, discuss an issue you're having, or solicit them for tried-and-true techniques. There's no substitute for experience!
We can't emphasize enough the usefulness of the EBRB! It's a collection of numerous worksheets, activities, demonstrations, handouts, and homework assignments developed by past GSIs, all stored on this wiki. Most things in it are well-vetted and effective. It's a great place to pull out a good worksheet for a topic you're covering or to find inspiration for your section.
As you may suspect, the EBRB was preceded by a physical Big Red Binder, which lives in the 7th Floor Library in Campbell Hall. Feel free to page through it if you wish - the “PBRB” contains worksheets that haven't yet been scanned in to the EBRB. If you happen to find something really useful that doesn't seem to be on the EBRB, it'd be great if you could upload it.
Everything listed below should be in the cabinet in 264 Evans (or possibly scattered around the room if people have been lazy and not put stuff away). Always check to make sure you have everything you need for a demo well before section begins!
Descriptions of more demos can be found in the EBRB.
Contact demos@physics
to reserve a demonstration at least one day before class. Only demos that can fit in a standard printer-paper box can be taken out of LeConte. The larger demos can be set up in a LeConte lecture room, if one is available. Go to http://physics.berkeley.edu/index.php?option=com_content&task=view&id=54&Itemid=95 to view descriptions of the available demos. Demos most relevant to astronomy are listed below (the Demo Codes are used by the Physics people to catalog their stuff):
Title | Demo Code | Fits in a Box ? |
---|---|---|
How a Rainbow Works (reflection and refraction) | E+60+10 | no |
Radiation Pressure | C+65+15 | yes |
No Sound in a Vacuum | B+45+15 | yes |
Wave Interference (beats for two sound sources) | B+35+25 | yes |
EM Wave Model | D+5+32 | yes |
Doppler Effect for Sound | B+65+0 | yes |
Inverse Square Law for Light | E+55+0 | probably |
Gas Temperature and Particle Motion | C+55+0 | yes |
Blackbody Spectra and Wien's Law | E+65+25 | no |
Model of the Eye | E+30+65 | no |
Diffraction Limit | E+10+45 | yes |
Airy Disk | E+10+10 | no |
Acceleration due to Gravity (feather and rock fall in vacuum) | A+0+0 | probably |
Conservation of Angular Momentum (rotating chair with bicycle wheel) | A+30+15 | no |
Convection | C+20+0 | yes |
Earth's Magnetic Field | D+30+4 | yes |
Center of Mass | A+50+37 | yes |
These demos require only simple household items to perform.
They have tons of info and are great for directing you to various parts of the University and giving general teaching information. There website is http://gsi.berkeley.edu/.
There are lots of sites out there with great info on teaching introductory astronomy. Some of them are:
awest@astro
) with questionsjcaspers@berkeley
)JSilverman@astro
) with questions When planning questions and lectures, you may find it helpful to look at http://www.physics.umaine.edu/ncomins/miscon.htm, which contains information on more than 1700 common astronomy misconceptions. It's compiled by Neal F. Comins of the University of Maine and the content is taken from his book “Heavenly Errors: Misconceptions about the real nature of the Universe.”
Great for giving students what they want (pretty astronomy!). Contact Attila Kabai, akabai@astro.berkeley.edu
. Also, make sure that you can actually operate the telescope and that you have a list of objects that you want to observe before actually running a star party. Talk to your AY 300 instructor and/or Head GSI for more info. Also check out the Star Party page in the EBRB.
Has information about various technology services available on campus and can get you keys to A/V cabinets in lecture rooms. Visit http://ets.berkeley.edu/ or go to the basement of Dwinelle Hall for more info. To quickly view a room's A/V attributes, go to http://students.berkeley.edu/rooms/attributes.asp.
Great for showing pretty pictures and online demos when the room you're using doesn't have a built-in projector. Make a reservation well in advance by going to http://astro.berkeley.edu/resources/campbell/reservations/video.html and contact central@astro
if you run into reservation problems.
They'll have info (and probably pictures) for most, if not all, of your students. Also, to make it clear that you're not playing favorites or anything like that, rather than “friending” your students online you might want to just create an online group for each of your sections that any of the students in the section can join.
Useful to take pictures of students/classes to help with name memorization. Contact central@astro
to reserve the camera well in advance.
Online directory of students in a given course or section, great for memorizing student names. GSI names must be assigned by a department administrator (Dexter) to specific sections before this system works. Their homepage is at http://courseweb.pitt.edu/.
An audience response system is good for keeping student attention and diagnosing student understanding during lecture. The department currently has a set of 36 clickers (transmitters) and one receiver stored by Dexter. The software is available for download at http://www.gtcocalcomp.com/prs_software.php. Contact Andrea Monter at GTCO CalComp (800-344-4723, ext 203; AMonter@gtcocalcomp.com
) to order more clickers. Sometimes, you can get free clickers when you purchase the textbooks for your class - ask Amy Teeling (Amy.Teeling@aw.com
, 510-547-2211) if you'd like to hear more about this option.
Good for putting books on reserve so that students running on a tight budget do not have to buy the book. Contact Heather Pena (hpena@library
) for more info.
Good for coordinating book ordering or clicker ordering. Call (510) 642-9000.