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Signature of collision of magnetic flux tubes in the quiet solar photosphere

Published online by Cambridge University Press:  26 August 2011

Aleksandra Andic
Aleksandra Andic*
Affiliation:
BBSO, 40386 N. Shore Ln.Big Bear City, CA-92314, USA email: aandic@bbso.njit.edu
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Abstract

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Collision of the magnetic flux tubes in the Quiet Sun was proposed as one of the possible sources for the heating of the solar atmosphere (Furusawa and Sakai, 2000). The solar photosphere was observed using the New Solar Telescope ad Big Bear Solar Observatory. In TiO spectral line at 705.68 nm we approached resolution of 0.1″. The horizontal plasma wave was observed spreading from the larger bright point. Shorty after this wave an increase in the oscillatory power appeared at the same location as the observed bright point. This behavior matches some of the results from the simulation of the collision of the two flux tubes with a weak current.

Keywords

Bright pointsoscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 399 - 402
Copyright
Copyright © International Astronomical Union 2011

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