How do we know what kind of phytoplankton are in the water? The Imaging FlowCytobot (IFCB) is a robot that scientists use to image phytoplankton in the water. One IFCB can take up to 30,000 pictures per hour! The IFCB can be used in the field to detect plankton blooms in real time. In this activity, students will practice
From July 19, 2022, to August 15, 2022, I participated in the Harmful Algal Blooms in Arctic Waters research cruise on the R/V Norseman II. The Chief Scientist was Dr. Robert Pickart from Woods Hole Oceanographic Institution (WHOI), and the research team included scientists from WHOI, Oregon State University, the Florida Fish and Wildlife Conservation
This event with teacher Rebecca Siegel was broadcast live on 4 August 2022 from the Norseman II in Arctic waters. Rebecca is joined by team members from Woods Hole Oceanographic Institute working on Harmful Algal Blooms in Arctic Waters.
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
When radioactive elements decay they emit high-speed particles. These can be detected by use of a cloud chamber. The cloud chamber was invented by Charles Thomson Rees Wilson in 1911. The chamber works by saturating the air inside with alcohol vapor. Cooling the chamber with dry ice supersaturates the air. The energetic particles produced by the radioactive decay ionize
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.