Statistical analysis of solar bright points observed with the SOHO spacecraft.

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Solar Corona: Bright Points, Solar Corona: Heating, Solar Atmosphere: Magnetic Reconnection, Solar Atmosphere: Uv Radiation

Scientific paper

Bright points, small and short lifetime structures, appear permanently in the atmosphere and could be associated with magnetic reconnections, potential sources of coronal heating. Such structures have been observed with the coronal instruments on-board SOHO and a statistical analysis was carried out in order to find the signature of very small scale structures.

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