group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
48.43 | 317.96 | 24.97 | 164.25 | -7.17 | 139.23 | 8.20 | 210.58 | 0.2831 | 864.6 | 397.4 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 0.90 | 0.00 | 0.48 | -9.06 | 143.80 | 12.77 | 218.67 | 0.3509 | 714.0 | 518.2 | |
0.00 | 1.89 | 0.00 | 0.98 | -7.24 | 141.12 | 10.10 | 215.58 | 0.3002 | -774.0 | -474.8 | |
0.00 | 1.17 | 0.00 | 0.61 | -9.40 | 140.93 | 9.90 | 211.24 | 0.3285 | 704.0 | 611.8 | |
0.00 | 1.71 | 0.00 | 0.88 | -4.71 | 140.74 | 9.71 | 220.02 | 0.2626 | -1034.0 | -836.2 | |
0.00 | 0.90 | 0.00 | 0.46 | -4.89 | 140.74 | 9.71 | 219.57 | 0.2651 | -881.0 | -688.7 | |
48.43 | 294.92 | 24.97 | 152.01 | -6.76 | 139.35 | 8.32 | 211.38 | 0.2773 | 1440.4 | 443.8 | |
0.00 | 1.98 | 0.00 | 1.05 | -12.10 | 139.26 | 8.23 | 203.29 | 0.3554 | -841.0 | -669.0 | |
0.00 | 2.52 | 0.00 | 1.35 | -14.20 | 137.43 | 6.41 | 196.72 | 0.3775 | -831.0 | -597.5 | |
0.00 | 0.45 | 0.00 | 0.24 | -14.98 | 137.46 | 6.43 | 196.18 | 0.3897 | -701.0 | -566.4 | |
0.00 | 2.52 | 0.00 | 1.34 | -13.71 | 137.36 | 6.33 | 196.92 | 0.3695 | -876.0 | -723.5 | |
0.00 | 2.34 | 0.00 | 1.20 | -7.59 | 136.78 | 5.75 | 201.63 | 0.2706 | 860.0 | 773.4 | |
0.00 | 2.25 | 0.00 | 1.25 | -19.79 | 136.16 | 5.14 | 190.62 | 0.4591 | 687.0 | 622.5 | |
0.00 | 1.35 | 0.00 | 0.75 | -19.65 | 135.84 | 4.81 | 190.01 | 0.4561 | 737.0 | 609.5 | |
0.00 | 2.16 | 0.00 | 1.19 | -18.58 | 133.60 | 2.57 | 185.63 | 0.4347 | 746.0 | 512.9 | |
0.00 | 0.90 | 0.00 | 0.46 | -6.08 | 130.68 | -0.34 | 178.49 | 0.2265 | -784.0 | -657.1 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |