SOHO MDI 2000-09-28 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93 | 573 | 94 | 560 | -8.22 | 320.21 | -57.78 | 103.76 | 0.8619 | -331.2 | -120.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 378 | 12 | 340 | -7.65 | 323.59 | -54.40 | 103.96 | 0.8325 | -1221.2 | -355.0 | |
| 36 | -1 | 32 | -1 | -8.20 | 323.28 | -54.71 | 104.52 | 0.8367 | -927.8 | 999999 | |
| 6 | -1 | 6 | -1 | -8.17 | 322.38 | -55.60 | 104.23 | 0.8448 | -233.3 | 999999 | |
| 5 | 15 | 5 | 15 | -10.23 | 320.36 | -57.63 | 106.01 | 0.8668 | -380.0 | -257.6 | |
| 1 | 9 | 1 | 9 | -7.99 | 320.26 | -57.73 | 103.46 | 0.8630 | -379.5 | -227.1 | |
| 0 | 1 | 0 | 1 | -6.66 | 319.94 | -58.05 | 101.88 | 0.8632 | -396.0 | -329.7 | |
| 0 | 2 | 0 | 2 | -11.37 | 317.90 | -60.08 | 106.61 | 0.8887 | 316.0 | 351.5 | |
| 0 | 3 | 0 | 3 | -10.85 | 317.44 | -60.55 | 105.93 | 0.8912 | 246.0 | 230.1 | |
| 2 | 24 | 2 | 26 | -9.19 | 317.15 | -60.83 | 104.03 | 0.8904 | -350.0 | -148.3 | |
| 7 | 16 | 7 | 16 | -6.61 | 317.71 | -60.27 | 101.31 | 0.8817 | -459.4 | -273.6 | |
| 0 | 2 | 0 | 2 | -8.81 | 316.61 | -61.38 | 103.48 | 0.8939 | 625.0 | 513.9 | |
| 0 | 6 | 0 | 7 | -6.92 | 316.68 | -61.31 | 101.42 | 0.8904 | -191.0 | -85.7 | |
| 0 | 4 | 0 | 4 | -8.81 | 315.42 | -62.57 | 103.21 | 0.9028 | 260.0 | 322.5 | |
| 0 | 10 | 0 | 12 | -10.10 | 314.64 | -63.35 | 104.43 | 0.9103 | 632.0 | 574.8 | |
| 0 | 11 | 0 | 13 | -7.85 | 315.09 | -62.90 | 102.09 | 0.9037 | 773.0 | 576.5 | |
| 9 | 43 | 11 | 50 | -7.22 | 314.64 | -63.35 | 101.31 | 0.9060 | 820.7 | 546.9 | |
| 2 | -16 | 3 | -16 | -7.06 | 314.24 | -63.75 | 101.06 | 0.9087 | 507.1 | 999999 | |
| 12 | 47 | 15 | 58 | -9.12 | 312.98 | -65.01 | 103.00 | 0.9202 | 608.6 | 383.4 | |
| 0 | 2 | 0 | 2 | -7.05 | 312.86 | -65.13 | 100.77 | 0.9182 | 376.0 | 346.6 | |
| 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. | |