Simulation of Solar Coronal Magnetic Field UsingPotential Field Model

Authors

  • Loay Abood Department of Computer Science, College of Science, University of Baghdad, Baghdad, Iraq
  • Kamal Abood Department of Astronomy and Space Science, College of Science, University of Baghdad, Baghdad, Iraq

DOI:

https://doi.org/10.24996/ijs.2015.56.4c.%25g

Keywords:

solar coronal , magnetic field, potential field, magnetogram

Abstract

In this paper, 3D simulation of the global coronal magnetic field, which use observed line of sight component of the photosphere magnetic field from (MDI/SOHO) was carried out using potential field model. The obtained results, improved the theoretical models of the coronal magnetic field, which represent a suitable lower boundary conditions (Bx , By , Bz) at the base of the linear force-free and nonlinear force free models, provides a less computationally expensive method than other models. Generally, very high speed computer and special configuration is needed to solve such problem as well as the problem of viewing the streamline of the magnetic field. For high accuracy special mathematical treatment was adopted to solve the computation complexity.

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Published

2025-03-07

Issue

Section

Computer Science

How to Cite

Simulation of Solar Coronal Magnetic Field UsingPotential Field Model. (2025). Iraqi Journal of Science, 56(4c), 3569-3577. https://doi.org/10.24996/ijs.2015.56.4c.%g

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