Spatial & Temporal Characteristics of Ha flares during the period 1975-2002 (comparison with SXR flares)

Details Spatial & Temporal Characteristics of Ha flares during the period 1975-2002 (comparison with SXR flares) Spatial & Temporal Characteristics of Ha flares during the period 1975-2002 (comparison with SXR flares)

2010-09-22

arxiv.org/abs/1009.4320v1

2006AIPC..848..194G

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conferen

Scientific paper

10.1063/1.2347977

Although the energetic phenomena of the Sun (flares, coronal mass injections etc.) exhibit intermittent stochastic behavior in their rate of occurrence, they are well correlated to the variations of the solar cycle. In this work we study the spatial and temporal characteristics of transient solar activity in an attempt to statistically interpret the evolution of these phenomena through the solar cycle, in terms of the self-organized criticality theory.

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