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On the Polarimetric Signature of Emerging Magnetic Loops in the Quiet Sun

  • Authors: B. Viticchié

Viticchié 2012 The Astrophysical Journal Letters 747 L36.

  • Provider: AAS Journals

Caption: Figure 2.

Example of an Ω loop emergence event extracted from the analyzed time sequences. Upper row: sub-sequence of Stokes I continuum sub-fields centered around the location of the emergence event. The contours mark the positions of the positive circular polarization signature (red contours), the negative circular polarization signature (blue contours), and the linear polarization signature (green contours). These allow one to point out the emergence event according to the criteria used in Martínez González & Bellot Rubio (2009). The contour regions have areas larger than 4 pixels of Hinode SOT/SP and max(| Q|, | U|) > 8 × 10 −3 and max(| V|) > 6 × 10 −3 (see Section 3). Lower row: Stokes V profiles with |δ a| > 0.3 from the pixels in the locations of the two circular polarization signatures marked by the blue and red contours in the upper row. The colors encode the polarimetric signature from which the profiles were picked.

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