INTRODUCTION TO COSMIC RAYS (SOLAR ENERGY SYSTEM) | PHYSICS MSc PROJECT WORK



Introduction
                Cosmic rays are high energy sub-atomic particles from outside of the solar system which contains mostly protons and alpha particles (Usoskin et al, 2004). Cosmic rays are associated with electromagnetic radiations and can travel at nearly the speed of light with enormous energy in the range 0.1-15Gev (Devendraa and Singh, 2010). Most cosmic rays are thought to originate outside the solar system, with many coming from within our Milky Way galaxy, and a few arriving from other galaxies. Cosmic ray causes ionization in the atmosphere.
When cosmic rays enter the earth’s atmosphere, they collide with ambient atmospheric gas molecules thereby ionizing them.  In this process the may produce secondary particles which can be sufficiently energetic to contribute themselves to further ionization of the neutral gases. This leads to the development of an ionization cascade (or shower). The intensity and penetration dept of the cascade depends on the energy of the primary cosmic particles. Cascade of particles with several hundred MeV of kinetic energy may reach the ground. However, due to their charge cosmic ray particles are additionally deflected by the geomagnetic field. Almost all particles can penetrate into the polar region, where the magnetic field lines are perpendicular to the ground, where as only the rare most highly energetic particles with energy above 15Gev are able to penetrate the lower atmosphere near the equator.
            It is interesting to note that solar energy flux reaching the earth’s orbit Fs = 1.36 x 103wm-2   whereas the cosmic energy flux (particles with energy > 0.1Gev) FCR = 10-5Wm-2(Frohlich and Learn, 1997). Thus, energy input by cosmic rays in the Earth’s atmosphere is about 10-9 times that of solar energy and hence it is unlikely that cosmic rays could influence the atmosphere processes (Devendraa and Learn, 2010). However, cosmic rays are the only source of ion production in the lower atmosphere (Devendraa and Learn, 2010), which is confirmed from the measurements of Ermakov and Komotskov (Ermakov et al, 1992). Therefore, the processes, depending on the electrical properties of the atmosphere such as atmospheric electric current, lightening production, cloud and thunder cloud formation etc, can be affected by cosmic rays. For studying cosmic ray ground based observatories covering large areas are needed because the flux of cosmic rays gaze too low at these energies for direct measurement by balloons or satellite based experiment (Apel and Arteage, 2011).
    In this project work, we have reviewed the run-away breakdown mechanism in the atmosphere. In particular Gurevich et al 1992 shall be our case study.

Aims and Objectives
       Cosmic rays that penetrate the atmosphere undergo shower and reaches the earth surface.
1.      We aimed at studying the mechanisms of electron breakdown in the atmosphere
2.      To have a mathematical investigation into the electron breakdown.

Scope of the Study
We have to investigate acceleration and frictional drag on electrons in the earth atmosphere with respect to the Earth surface

Methodology
We have to approach the study in non relativistic and relativistic view mathematically.
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