URI Physics Colloquium

The URI Physics department hosts an ongoing speaker series each academic year, which features physics experts from URI and other universities, as well as scientific organizations.

During the fall and spring semesters, colloquia are held in East Hall, Room 112. Refreshments are served before each talk at 3:30 pm in the East Hall Library or Room 112.

All are welcome, and there is no fee to attend.

Schedule for Spring 2025 

Date Speaker Title (click on the link for abstract) Host Location
January 31, 2025 Jennifer Borsavage  
Robert Coyne
East Hall 112
February 7, 2025 Mark Semco  
Vanita Srinivasa
East Hall 112
February 13, 2025 Ning Bao   Department of Physics East Hall 112
February 21, 2025     Department of Physics East Hall 112
February 28, 2025     URI East Hall 112
March 14, 2025    

Wenchao Ge

East Hall 112
March 21, 2025      Department of Physics East Hall 112
March 28, 2025        
April 4, 2025        
April 11, 2025        
         
         
         
         
         

 

Abstracts:

Exploring Earth’s Outer Atmosphere Through Soft X-Ray Emissions

This presentation will focus on the study of soft X-ray emissions from Earth’s magnetosphere. When highly charged solar wind particles interact with neutral atoms in Earth’s outer atmosphere, a process called charge exchange occurs, leading to the emission of X-ray photons. These emissions offer a unique method for imaging the interaction between the solar wind and Earth’s magnetic field. By capturing X-ray images from satellites, it becomes possible to quickly map the distribution of solar wind plasma and track the movement of the dayside magnetopause, the boundary that separates Earth’s magnetosphere from the solar wind. This movement provides valuable insight into how energy from the Sun interacts with Earth’s space environment.

To further investigate these interactions, the exosphere, Earth’s outermost atmospheric layer, is modeled to study the distribution of neutral particles. The objective is to quantify the neutral density within the exosphere by simulating particle motion influenced by gravitational forces. These simulations, when compared with atmospheric models, improve our understanding of the exosphere’s structure and its role in solar wind interactions.