Moving magnetic features around a pore

Spectropolarimetric observations from SUNRISE/IMaX, obtained in 2013 June, are used for a statistical analysis to determine the physical properties of moving magnetic features (MMFs) observed near a pore. MMFs of the same and opposite polarity, with respect to the pore, are found to stream from its border at an average speed of 1.3 km s(-1) and 1.2 km s(-1), respectively, with mainly same-polarity MMFs found further away from the pore. MMFs of both polarities are found to harbor rather weak, inclined magnetic fields. Opposite-polarity MMFs are blueshifted, whereas same-polarity MMFs do not show any preference for up-or downflows. Most of the MMFs are found to be of sub-arcsecond size and carry a mean flux of similar to 1.2 x 10(17) Mx.

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Author Kaithakkal, A. J.
Riethmüller, T. L.
Solanki, S. K.
Lagg, A.
Barthol, P.
Gandorfer, A.
Gizon, L.
Hirzberger, J.
vanNoort, M.
Rodríguez, J. Blanco
Iniesta, J. C. Del Toro
Suárez, D. Orozco
Schmidt, W.
Pillet, V. Martínez
Knölker, Michael
Publisher UCAR/NCAR - Library
Publication Date 2017-03-24T00:00:00
Digital Object Identifier (DOI) Not Assigned
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Topic Category geoscientificInformation
Progress N/A
Metadata Date 2023-08-18T19:12:28.571705
Metadata Record Identifier edu.ucar.opensky::articles:19666
Metadata Language eng; USA
Suggested Citation Kaithakkal, A. J., Riethmüller, T. L., Solanki, S. K., Lagg, A., Barthol, P., Gandorfer, A., Gizon, L., Hirzberger, J., vanNoort, M., Rodríguez, J. Blanco, Iniesta, J. C. Del Toro, Suárez, D. Orozco, Schmidt, W., Pillet, V. Martínez, Knölker, Michael. (2017). Moving magnetic features around a pore. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7668g0w. Accessed 25 July 2025.

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