SOHO MDI 2000-09-30 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 120 | 826 | 81 | 562 | -8.10 | 321.19 | -40.97 | 109.44 | 0.6886 | -844.5 | -248.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -7.63 | 326.13 | -36.03 | 111.18 | 0.6275 | -551.0 | -419.2 | |
| 41 | 549 | 26 | 359 | -8.00 | 324.37 | -37.79 | 110.75 | 0.6512 | -1789.9 | -561.9 | |
| -2 | -2 | -2 | -2 | -7.48 | 324.37 | -37.79 | 110.00 | 0.6488 | 999999 | 999999 | |
| 18 | -2 | 12 | -2 | -8.00 | 323.87 | -38.29 | 110.49 | 0.6574 | -1525.3 | 999999 | |
| 6 | -2 | 4 | -2 | -7.62 | 323.56 | -38.60 | 109.79 | 0.6595 | -1075.4 | 999999 | |
| 16 | -2 | 10 | -2 | -8.28 | 323.28 | -38.88 | 110.59 | 0.6658 | -1007.1 | 999999 | |
| 7 | -2 | 5 | -2 | -7.88 | 323.27 | -38.88 | 110.02 | 0.6641 | -958.2 | 999999 | |
| 0 | 4 | 0 | 2 | -6.70 | 322.54 | -39.62 | 107.98 | 0.6682 | 353.0 | 268.2 | |
| 0 | 6 | 0 | 4 | -9.94 | 321.67 | -40.49 | 112.06 | 0.6924 | -605.0 | -427.1 | |
| 0 | 7 | 0 | 5 | -5.81 | 322.16 | -40.00 | 106.54 | 0.6694 | 317.0 | 576.3 | |
| 0 | 5 | 0 | 3 | -7.99 | 321.36 | -40.79 | 109.25 | 0.6876 | -391.0 | -344.4 | |
| 0 | 4 | 0 | 3 | -9.77 | 320.27 | -41.88 | 111.14 | 0.7078 | -305.0 | -358.5 | |
| 0 | 6 | 0 | 4 | -11.15 | 319.77 | -42.38 | 112.72 | 0.7193 | -219.0 | -187.6 | |
| 0 | 13 | 0 | 9 | -7.72 | 320.24 | -41.92 | 108.37 | 0.6999 | -484.0 | -245.3 | |
| 0 | 5 | 0 | 3 | -11.43 | 318.74 | -43.42 | 112.59 | 0.7320 | 203.0 | 250.7 | |
| 11 | 21 | 7 | 15 | -6.84 | 319.28 | -42.88 | 106.76 | 0.7079 | -709.8 | -369.5 | |
| 0 | 15 | 0 | 11 | -8.76 | 318.81 | -43.34 | 109.14 | 0.7204 | -834.0 | -379.2 | |
| 0 | 7 | 0 | 5 | -8.31 | 318.39 | -43.77 | 108.37 | 0.7236 | -464.0 | -348.2 | |
| 0 | 4 | 0 | 3 | -9.42 | 318.17 | -43.99 | 109.72 | 0.7302 | -295.0 | -245.2 | |
| 0 | 6 | 0 | 4 | -9.22 | 317.65 | -44.51 | 109.24 | 0.7353 | -410.0 | -268.3 | |
| 0 | 6 | 0 | 4 | -8.24 | 317.35 | -44.81 | 107.85 | 0.7351 | 722.0 | 528.1 | |
| 0 | 4 | 0 | 3 | -10.28 | 315.59 | -46.57 | 109.75 | 0.7615 | 620.0 | 563.3 | |
| 0 | 5 | 0 | 4 | -9.67 | 315.24 | -46.92 | 108.84 | 0.7631 | 664.0 | 602.9 | |
| 0 | 9 | 0 | 7 | -10.20 | 314.67 | -47.48 | 109.29 | 0.7709 | 736.0 | 728.4 | |
| 6 | 46 | 5 | 35 | -8.57 | 314.91 | -47.25 | 107.34 | 0.7630 | 988.5 | 803.7 | |
| 4 | 40 | 3 | 30 | -7.24 | 315.05 | -47.10 | 105.70 | 0.7572 | 1032.0 | 581.2 | |
| 0 | 4 | 0 | 3 | -7.86 | 314.79 | -47.37 | 106.39 | 0.7620 | 351.0 | 348.8 | |
| 0 | 9 | 0 | 7 | -9.88 | 314.20 | -47.95 | 108.71 | 0.7747 | 757.0 | 762.7 | |
| 3 | -26 | 2 | -26 | -7.32 | 314.58 | -47.58 | 105.63 | 0.7627 | 748.0 | 999999 | |
| 4 | -25 | 3 | -25 | -8.34 | 314.36 | -47.79 | 106.85 | 0.7681 | 987.1 | 999999 | |
| 0 | 6 | 0 | 4 | -10.63 | 313.93 | -48.22 | 109.53 | 0.7800 | 655.0 | 552.7 | |
| 0 | 5 | 0 | 4 | -8.87 | 314.21 | -47.94 | 107.46 | 0.7713 | 451.0 | 489.5 | |
| 4 | 13 | 4 | 10 | -9.55 | 313.01 | -49.15 | 107.86 | 0.7859 | 748.0 | 576.2 | |
| 0 | 3 | 0 | 2 | -7.43 | 312.90 | -49.26 | 105.21 | 0.7809 | 638.0 | 546.4 | |
| 0 | 4 | 0 | 4 | -7.82 | 312.53 | -49.63 | 105.58 | 0.7858 | 449.0 | 426.7 | |
| 0 | 4 | 0 | 3 | -9.38 | 312.19 | -49.97 | 107.36 | 0.7938 | 299.0 | 160.6 | |
| 0 | 9 | 0 | 7 | -8.84 | 311.92 | -50.23 | 106.62 | 0.7949 | 421.0 | 295.4 | |
| 0 | 2 | 0 | 2 | -8.29 | 311.84 | -50.32 | 105.92 | 0.7942 | 369.0 | 275.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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 | |
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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. | |