The area asymmetry in bipolar magnetic fields | Astronomy & Astrophysics (A&A)

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Table 2

Temporal evolutions of A in the recurrent regions.

No.	1st rotation		2nd rotation		#^a	#^b
	yyyy-mm-dd	A	yyyy-mm-dd	A

1	1996-11-26	0.056	1996-12-23	0.028	2	1
2	1996-12-10	−0.093	1997-01-07	0.032	1	2
3	1997-09-08	−0.018	1997-10-06	0.061	3	1
4	1997-09-13	0.215	1997-10-11	0.003	1	1
5	1997-11-02	−0.060	1997-11-29	−0.062	2	2
6	1999-07-01^c	0.067	1999-07-27^c	−0.058	3	1
7	1999-12-19	−0.083	2000-01-15	−0.149	3	3
8	2000-02-27	0.127	2000-03-27	0.128	2	1
9	2000-06-30	0.146	2000-07-28	0.138	2	2
10	2000-09-21	0.138	2000-10-18	−0.008	1	1
11	2001-01-02	0.217	2001-01-29	−0.060	1	1

Notes.

^(a)

1: A comes closer to zero; 2: A is almost retained; 3: A becomes further from zero.

^(b)

1: Magnetic fluxes decrease; 2: Magnetic fluxes increase; 3: Magnetic fluxes do not change.

^(c)

2 nd and 3 rd rotations.

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