TY - JOUR
T1 - Moving Magnetic Features Around a Pore
AU - Kaithakkal, A. J.
AU - Riethmüller, T. L.
AU - Solanki, S. K.
AU - Lagg, A.
AU - Barthol, P.
AU - Gandorfer, A.
AU - Gizon, L.
AU - Hirzberger, J.
AU - Vannoort, M.
AU - Rodríguez, J. Blanco
AU - Iniesta, J. C.Del Toro
AU - Suárez, D. Orozco
AU - Schmidt, W.
AU - Pillet, V. Martínez
AU - Knölker, M.
N1 - Funding Information:
This work was partly supported by the BK21 plus program through the National Research Foundation (NRF) funded by the Ministry of Education of Korea.
Publisher Copyright:
© 2017. The American Astronomical Society. All rights reserved..
PY - 2017/3
Y1 - 2017/3
N2 - 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 ∼1.2 × 1017 Mx.
AB - 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 ∼1.2 × 1017 Mx.
KW - Sun: magnetic fields
KW - Sun: photosphere
UR - http://www.scopus.com/inward/record.url?scp=85016147360&partnerID=8YFLogxK
U2 - 10.3847/1538-4365/229/1/13
DO - 10.3847/1538-4365/229/1/13
M3 - Article
AN - SCOPUS:85016147360
SN - 0067-0049
VL - 229
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
M1 - 13
ER -