Students will learn about the difference between the methods of neutrino detection – optical versus radio. This will then allow them to understand why the relative size of the detectors is so different. Students will also engage in a hands-on activity to understand scale through creating models of the two detectors.
This lesson is intended to help students make connections to polar science while discovering how and why sea ice drives deep ocean currents. Students will also learn key terminology related to sea ice and using actual salinity content charts, will graph a typical sea ice core’s salinity as it relates to depth.