Faculty mentor: Dmitri Ivanov
As part of the sFLASH collaboration, I found the constant of proportionality known as Fluorescence Yield linking the amount of fluorescence light produced by high energy cosmic rays in the atmosphere to the primary particle energy of the cosmic rays. I used a FLUKA simulation and past experimental data to reach my result.
Watch my research presentation below.
Questions or comments? Contact me at: email@example.com