Computer Science
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..541p&link_type=abstract
In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun
Computer Science
2
Solar Flares, Coronal Mass Ejections, Transient Phenomena
Scientific paper
The sun exhibits transient, large scale, energetic phenomena, namely solar flares, coronal mass ejections etc, directly affecting the space environment and the earth. The location and rate of appearance of these phenomena follow the general solar cycle, however there is a significant random component in their emergence. Also, the evolution and interactions between close magnetic structures of the sun is complicated and not a well understood process. We study the spatial and temporal distributions of transient energetic phenomena of the sun, investigating possible correlations and organization over wide range of scales. We also address the evolution of the distributions of energetic solar phenomena throughout the solar cycle.
Hillaris Alexander
Moussas Xenophon
Nikolopoulou A.
Polygiannakis J. M.
Preka-Papadema Panagiota
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