Grad B Drifts of Heavy Ions Solar Energetic Particles at Solar Corona Region

Abstract

     The objective of this research study the Grad B drifts velocity of the heavy ion of the solar wind (C⁺⁴, C⁺⁵ (at corona region with distance (1 to 15) * 6.69*10⁸m for two varied angles (Ɵ= 90ᵒ, 180ᵒ). It has been studied, that grad B drifts velocity, in the model of Parker spiral. within single particle dynamics model, in a spherical coordinate system (local coordinate system with an axis aligned with the magnetic field). This work result shown that, azimuthal grad B drift velocity, V_{∇Bφ`</sub> takes maximum value at polar zone for (C<sup>+4</sup>, C<sup>+5</sup>) for both velocities of solar wind. Also, there is no azimuthal grad B drifts V<sub>∇Bφ`} at equators zone. And as for colatitude grad B drift velocity, V_∇Bθ` takes high value at most of regions and the highest value at polar zone for fast and slow solar winds. And noting that the slow solar winds have higher values than fast solar wind at the equator region.