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Table 2.

Orbital motions of umbral flux fragments relative to previously-emerged umbrae and the observed active region chiralities.

NOAA Start Time End Time Total Orbit Avg. Orbit Emerging Coronal Estimated FR
AR (UT) (UT) (°) (° day−1) Flux Field Height (Mm)
11429 04 Mar 12 18:00 (a) 06 Mar 12 18:00 −74 −37 LH LH 56 ± 5
07 Mar 12 00:00 (a) 08 Mar 12 06:00 −36 −29
08 Mar 12 12:00 (a) 14 Mar 12 12:00 −19 −3
08 Mar 12 12:00 (b) 14 Mar 12 12:00 −180 −30

11504 09 Jun 12 18:00 10 Jun 12 18:00 +2 +2 RH RH 173 ± 26
11 Jun 12 06:00 12 Jun 12 12:00 +60 +48 89 ± 30
12 Jun 12 18:00 15 Jun 12 18:00 +186 +62

11585 03 Oct 12 06:00 06 Oct 12 00:00 −111 −40 LH LH 98 ± 25
06 Oct 12 12:00 08 Oct 12 00:00 −41 −27
08 Oct 12 12:00 09 Oct 12 00:00 −7 −14

12665 08 Jul 17 00:00 10 Jul 17 00:00 −92 −46 LH LH 71 ± 20
10 Jul 17 06:00 14 Jul 17 00:00 −47 −12.5
14 Jul 17 00:00 15 Jul 17 00:00 −43 −43

Notes. Start Time and End Time delineate periods that orbiting motions of magnetic flux fragments were tracked over. In the total and averaged (avg.) daily orbital motions, positive angles are clockwise and negative angles are anticlockwise. Emerging flux and coronal field is determined as left-handed (LH) or right-handed (RH) as outlined in Sect. 3.3. Estimated heights of the flux ropes that formed in each active region are produced by the method described in Sect. 3.2.

(a)

In the case of March 2012, the first three rows represent the orbiting given by the fragment-tracking method. Observations suggest that the full extent of the orbiting from 8 to 14 March is not detected.

(b)

The fourth row for March 2012 contains orbit angles estimated by-eye.

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