Radio Frequency Research during COVID-19

The purpose of this experiment is to study the effects of the sudden change in electromagnetic radiation from multiple sources, including solar radiation, the magnetosphere, and the aurora borealis on the D-region of the ionosphere. VLF was chosen for measurement because naturally occurring waves propagate through the Earth-ionosphere waveguide, which can be used to remotely observe the ionosphere. The D-region reduces the energy in propagating waves due to absorption. This means that any fluctuations in the D-region are inversely correlated to the strength of VLF waves being received. In addition, Auroral emissions such as hiss, roar, and burst will be measured using an HF receiver. Currently, there is a good understanding of space climate, but not space weather. Therefore, this project aims to also build a HF receiver that will be launched simultaneously with VLF to measure the correlation between both frequencies. Furthermore, the team prospects to gather data that will contribute with the ham radio community to better understand space weather. While still having limited access to the lab due to COVID-19, the research team has been facing challenges by not being able to personally interact, plan, brainstorm, and to continue the hands-on part of building the experiments. Although this new form of researching and communicating has been an adaptation process on how the work continues to be conducted, this team has been able to turn this possible disadvantage to an advantage. Utilizing online platforms such as Zoom and Microsoft Teams for visual interactions, Slack and emails for messaging and further contact within the group,outside individuals, and organizations, this team has been able to successfully collaborate with different professors and experts in the field to improve the project and further develop our research.