Astronomy 150 | Spring 2012

Computer Lab 2: Solar Rotation

Purpose: To introduce students to the techniques that astronomers use to measure the rotation rate of the sun using images of sunspots. To introduce some of the difficulties of using two-dimensional images to derive three-dimensional properties of celestial objects.

Goals:

Lab Description: This exercise enables students to measure the rate of rotation of the sun at various latitudes using an archive of 368 images of the sun obtained over a four month span in 2002 obtained by the Global Oscillation Network Group (GONG) project . Because of the high spatial and temporal resolution of the sample, these are the best images to date from which students can determine the solar rotation rate. Software provided enables student to access the GONG images, display them as still images or animations, measure and record the positions of sunspots, plot its heliocentric coordinates versus time, and thus determine the apparent rotation period of the spot.

Lab Software: The program we will use (THE PERIOD OF ROTATION OF THE SUN) can be downloaded to your computer, or you can go to any of the ICS computer labs (running Windows). The software is available under "Class Software > ASTR150" on the "Win_Apps" menu.

If you want to install on your own machine, there is a link below to download the program (note - download is quite large ~400 MB, due to the size of the image database).

Lab Groups: You may work on this lab in groups of up to 3 people. A single lab report can be turned in for the group (with all group member names and NetIDs, of course).

Due Date: The completed Lab Worksheet below is due in class Friday, April 20.

Help Sessions: Help sessions will be conducted on April 19 from 5-7pm in the Oregon ICS Lab.

Downloads:


Brian Fields
Last modified: Fri Apr 6 09:54:08 CDT 2012