GRBAlpha is a new cube sat that was launched in March 2021 with the main objective of characterizing the background and degradation of the gamma ray detectors. The secondary objective was to attempt to detect gamma ray bursts (GRB). This secondary objective can be a challenge if we do not understand the particle background experienced by the onboard instruments sufficiently well enough, as a small burst might be interpreted as noise or misinterpreted as another feature of the radiation environment during its low earth polar orbit. Using the same data used by the Heliophysics and Space Weather group at NASA, we seek to explore the effects of Space Weather on the local earth environment, specifically with focus on how these particular events effect the background of the particle detector instruments onboard the satellite. We hope to improve the background model that we are currently using, to adjust for any potential events in the future, so that we can increase the sensitivity and significance of GRB detection.