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.
Kate Miller is joined by IceCube undergraduate researcher, Samantha Pedek, in presenting at the Arlington Public Schools' Superintendent's Seminar.
Superintendent’s Seminar is a summer enrichment program for rising 11th and 12th graders who have demonstrated a desire for an academic experience. Approximately 30 students from across the district spend a week participating in activities focusing on this year's theme of
In this lesson, students will be introduced to the Standard Model, learning key vocabulary such as Fermions, Hadrons, Mesons, Baryons, Quarks, Leptons, particles, and anti-particles. In particular, students will come to understand what a neutrino is and why it is such a unique particle. This understanding connects to the IceCube Neutrino Observatory’s search for neutrinos in an effort to
In this lesson students will learn how to use photography to support scientific research by documenting collected measurement information through observational photography. This lesson was written for a Photography course, to be taught in a lab with access to either a darkroom or computers/printers. Alternatively this lesson could be modified to work in a non-photography class, by removing the photography
1) Why is it important to collect large quantities of research data?
2) How can photographing a subject be similar to scientific observation?
3) How can one plot photographic data on a map?
Introduction:
This lesson was written for a Photography I course, to be taught in a lab with access to either a darkroom or computers/printers. The
This website is an overview of the TAMSEIS project addressing the questions of the Transantarctic Mountain origins and the structure of the East Antarctic craton.