Influence of the Magnetic and Electric Fields on the (SEPs) at Solar Corona Region


The objective of this research investigates the influence of the electric and magnetic fields at the corona region of the sun on the solar energetic particles. The result show that the azimuthal magnetic field component has higher values for the slow than the fast solar wind for the same distance and angles, besides that the azimuthal Bφ at constant distance 5×Rʘ is higher at the equator than the pole region and the values of slow solar wind higher than the fast solar wind. Similarly the colatitude electric field Eθ will have higher values at the equator than the pole region. It is seen that the equator region will be more advantage and effect on the movement of the solar energetic particles that contribute to the solar wind.