Students will individually weigh a random sample of pennies. The data will be graphed to look for patterns, then explanations will be sought to explain these patterns. Some of the key ideas are using graphical representations of data to help identify patterns. This is a key concept in all sciences, including in the IceCube Neutrino Observatory - data
PolarConnect event with Heidi Roop who is working with an Ice Core Drilling team on the West Antarctic Ice Sheet in Antarctica. A PDF of the slides is not available for this event.
This PolarConnect event was held on 16 December 2010 with Heidi Roop who is working with an ice core drilling team on the West Antarctic Ice Sheet. This live event was broadcast and had a live component at the AGU 2010 Fall Meeting.
Live from IPY! event with researcher Heidi Roop and other members of the ice coring team at WAIS Divide Camp, Antarctica. The presentation focused on project and the mechanics and science of ice coring.
This was a real-time event with PolarTREC teacher Casey O'Hara being broadcast from the South Pole Station, Antarctica. Casey presented on the IceCube telescope project and covered a bit about life at the South Pole station.
This article from the San Francisco Chronicle is about Casey O'Hara's upcoming expedition to Antarctica. It also includes some great photos from a pre-expedition icecream making lab. You can visit the article online here.
This data plotting lesson compares different stratospheric ozone data collected at the South Pole in September 1969, September 1998, September 2008, January 1999, and January 2008. This ozone comparison activity allows students to make conclusions about the annual and seasonal ozone hole as well as overall ozone concentration changes over Antarctica. Students use authentic data collected at the
This data plotting lesson is about temperature changes throughout the atmosphere. The data was collected together with the ozone data in January 2008.
The temperature vs. altitude profile allows students to make conclusions about annual and seasonal temperature changes in the atmosphere up to about 35 kilometers in the stratosphere. The best part of this lesson is using