Possible Presence of Lateral Influx of the Photospheric Radiation Within Sunspots

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The reduced profiles of C2 5150.56, CN 3864.32, MgH 5150.20 and Fe I 5150.84 lines, representing the penumbra, the penumbra-umbra boundary and the umbra of SPO 6403 have been analyzed by comparing them with the synthetic profiles computed from a set of umbral and penumbral models. The results are presented and discussed. It is suggested that there may be a significant lateral flow of photospheric radiation into the umbral and penumbral regions of the sunspots.

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