Lesley Anderson was connected with local California radio station KSON before and during her trip to South Pole, Antarctica as part of the PolarTREC program.
1. KSON Radio Station hosts a live interview with Lesley Anderson at the food fund in Bonita, CA.:
http://www.kson.com/media/audio-channel/john-and-tammys-food-fund-friday-bonita
2. Article in John & Tammy Blog (see downloadable article).
3. Facebook post during her stay
The Star News, a Chula Vista newspaper interviews Lesley Anderson about her experience studying neutrinos at the South Pole and her plans to bring the research back into her classroom.
2017 Antarctica Day celebration with PolarTREC teacher Lesley Anderson speaking from the South Pole, and researcher Dr. Jim Madsen discussing the IceCube Neutrino Observatory and the Askaryan Radio Array. This event was held on 4 December 2017.
My experience at McMurdo Station involved the study of neutrons caused by cosmic radiation from the sun. The sun can be very active. Changes in the sun's active surface can result in the ejection of high energy particles (from solar flares, coronal mass ejections, or related phenomena). Some of these particles can get sent toward the earth
Presentation prepared for the Rochester Community Schools Board of Education related to the PolarTREC 2017 Neutron Monitors for Solar Study expedition.
Students will examine sunspots and track them at different latitudes on the Sun.
This activity is adapted from the Tracking Sunspots activity on NASA’s Solar and Heliocentric Observatory (SOHO) website (2009): https://soho.nascom.nasa.gov/classroom/for_students.html.
Objectives:
Students begin to familiarize themselves with solar activity by tracking sunspots at different latitudes on the Sun.
This activity is designed to get students thinking about
This is a suite of labs created by Michigan State University and the Joint Institute for Nuclear Astrophysics (JINA). It provides a number of lessons and activities in nuclear physics. It can be used to demonstrate the types of reactions typical in cosmic ray interactions and the interactions that the CosRay neutron monitors depend on.