The Impact of Solar Flares and Cosmic Rays on Atmospheric Decay

Aims: The objective of this paper is to introduce a Relativistic Stochastic Process that calculates the number of cosmic ray and high energy solar flare particles that enter the atmosphere.
Study Design: The Relativistic Stochastic Process is tested against the Arley model.
Place and Duration of Study: Department of research and development, at Economics Traffic Clinic in Paris, between January 2013 and March 2013.
Methodology: The Relativistic Stochastic Process is a derivative of the Arley's probabilistic model. Although Arley's simplified model gives satisfactory results, it does not adequately address the phenomenon of cosmic ray and high energy solar flare particle showers.
Results: The simulation with the Relativistic Stochastic Process gives better results compared to the Arley model.
Conclusion: Relativistic Stochastic Process is more realistic and thus accurate and reliable.