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The Visual Computer

, Volume 26, Issue 5, pp 385–395 | Cite as

A new technique for the calculation and 3D visualisation of magnetic complexities on solar satellite images

  • O. W. AhmedEmail author
  • R. Qahwaji
  • T. Colak
  • T. Dudok De Wit
  • S. Ipson
Original Article

Abstract

In this paper, we introduce two novel models for processing real-life satellite images to quantify and then visualise their magnetic structures in 3D. We believe this multidisciplinary work is a real convergence between image processing, 3D visualisation and solar physics. The first model aims to calculate the value of the magnetic complexity in active regions and the solar disk. A series of experiments are carried out using this model and a relationship has been indentified between the calculated magnetic complexity values and solar flare events. The second model aims to visualise the calculated magnetic complexities in 3D colour maps in order to identify the locations of eruptive regions on the Sun. Both models demonstrate promising results and they can be potentially used in the fields of solar imaging, space weather and solar flare prediction and forecasting.

Keywords

Active regions Solar disk Solar flares Magnetic complexity Energy Satellite images 3D Sun 

Abbreviations

MDI

Michelson Doppler Imager

SOHO

Solar and Heliospheric Observatory

ESA

European Space Agency

NASA

National Aeronautics and Space Administration

NGDC

National Geophysical Data Center

GIF

Graphic Interchange Format

NOAA

National Oceanic and Atmospheric Administration

OpenGL

Open Graphics Library

ASAP

Automated Solar Activity Prediction

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Copyright information

© Springer-Verlag 2010

Authors and Affiliations

  • O. W. Ahmed
    • 1
    Email author
  • R. Qahwaji
    • 1
  • T. Colak
    • 1
  • T. Dudok De Wit
    • 2
  • S. Ipson
    • 1
  1. 1.School of Computing, Informatics and MediaUniversity of BradfordBradfordUK
  2. 2.LPC2EUniversity of OrléansOrleans Cedex 2France

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