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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*
Affiliation:
BBSO, 40386 N. Shore Ln.Big Bear City, CA-92314, USA email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Andic, A., Goode, P. R., Chae, J., Cao, W., Ahn, K., Yurchyshyn, V., & Abramenko, V. 2010, Astrophys. J., 717L, 79Google Scholar
Chae, J. & Sakurai, T. 2008, Astrophys. J., 689, 593Google Scholar
Furusawa, K. & Sakai, J. 2000, Astrophys. J., 540, 1156CrossRefGoogle Scholar
Goode, P. R., Yurchyshyn, V., Cao, W., Abramenko, V., Andic, A., Ahn, K., & Chae, J. 2010, Astrophys. J., 714, L31Google Scholar
Lites, B. W., Socas-Navarro, H., Berger, T., Frank, Z., Shine, R. A., Tarbell, T. D., Title, A. M., Ichimoto, K., Katsukawa, Y., Tsuneta, S., Suematsu, Y., Shimizu, T., & Nagata, S. 2008, Astrophys. J., 672, 1237CrossRefGoogle Scholar
von der Lühe, O. 1993 Astron. Astrophys, 268, 347Google Scholar
Orozco Suárez, D., Bellot Rubio, L. R., del Toro Iniesta, J. C., Tsuneta, S., Lites, B. W., Ichimoto, K., Katsukawa, Y., Nagata, S., Shimizu, T., Shine, R. A., Suematsu, Y., Tarbell, T. D., & Title, A. M. 2007, Astrophys. J., 670, L61Google Scholar
Schüssler, M. & Vögler, A. 2008, Astron. Astrophys, 481, L5Google Scholar
Steiner, O., Rezaei, R., & Schaffenberger, W., Wedemeyer-Böhm, 2008, Astrophys. J., 680, L85Google Scholar
Torrence, C. & Compo, G. P. 1998, Bull. Amer. Meteor. Soc. 79, 61Google Scholar
Wöger, F., von der Lühe, O., & Reardon, K. 2008, Astron. Astrophys, 488, 375CrossRefGoogle Scholar