Development of Experimental Setup and Enhanced Analytical Methodologies to Study Cosmic \(\gamma \) -Ray Flux Variations During Total Solar Eclipses
摘要
Over the past 25 years, attempts to detect an inverted Gaussian-shaped decrease in \(\gamma \) -ray flux during total solar eclipses have produced inconsistent results. This study introduces an optimized setup using four large-volume NaI(Tl) scintillation detectors to measure \(\gamma \) -ray flux during the 22 July 2009 eclipse from two locations: Indore and Siliguri. Elevated detectors minimized terrestrial interference, but rain-induced radon daughters complicated analysis. A RooFit-based method combining exponential and Gaussian functions was developed to unify energy spectra and address rain effects. A novel technique isolated true background, reducing rain-affected \(\gamma \) -ray flux by over half. This improved setup and analysis provide a foundational approach for future eclipse experiments.