A recent study conducted by Khagendra Katuwal, an astronomy graduate student, and R.T. James McAteer, Deputy Provost and Professor of Astrophysics at New Mexico State University (NMSU), focuses on the relationship between coronal holes and solar wind. Published in *The Astrophysical Journal*, the research analyzed 70 coronal holes using data from NASA's Solar Dynamics Observatory (SDO). The study revealed that approximately 88% of these coronal holes exhibited significant magnetic field imbalances, which are crucial for generating high-speed solar wind streams. Katuwal, inspired by his studies in heliophysics, aims to improve space weather forecasting models by understanding how these magnetic structures influence solar wind. The research highlights the importance of connecting fundamental solar physics to real-world impacts, particularly on technology affected by solar activity. Looking ahead, Katuwal plans to leverage data from the Daniel K. Inouye Solar Telescope in Hawaii to further investigate the dynamics of coronal holes and their magnetic properties.