SOHO MDI 2000-10-29 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66 | 477 | 70 | 520 | 9.23 | 267.59 | -63.43 | 81.93 | 0.8934 | 484.7 | 30.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 2 | 9.68 | 270.16 | -60.87 | 81.43 | 0.8728 | 288.0 | 359.5 | |
| 0 | 4 | 0 | 4 | 8.87 | 269.74 | -61.28 | 82.36 | 0.8763 | 353.0 | 372.0 | |
| 3 | 401 | 3 | 434 | 8.33 | 269.24 | -61.79 | 82.97 | 0.8805 | 342.5 | 81.0 | |
| 24 | -3 | 25 | -3 | 9.69 | 268.57 | -62.45 | 81.42 | 0.8858 | 1068.2 | 999999 | |
| 3 | -3 | 3 | -3 | 8.84 | 268.67 | -62.36 | 82.39 | 0.8851 | 487.9 | 999999 | |
| 7 | -3 | 7 | -3 | 9.96 | 267.96 | -63.06 | 81.12 | 0.8907 | 813.7 | 999999 | |
| 0 | 6 | 0 | 6 | 6.56 | 268.92 | -62.10 | 84.97 | 0.8834 | -377.0 | -343.1 | |
| 12 | -3 | 13 | -3 | 9.58 | 267.57 | -63.46 | 81.54 | 0.8937 | 338.6 | 999999 | |
| 12 | -3 | 13 | -3 | 8.75 | 267.40 | -63.63 | 82.47 | 0.8951 | -415.2 | 999999 | |
| 0 | 6 | 0 | 6 | 7.23 | 267.39 | -63.64 | 84.17 | 0.8954 | -396.0 | -438.9 | |
| 5 | -3 | 6 | -3 | 9.65 | 266.28 | -64.75 | 81.46 | 0.9035 | 270.5 | 999999 | |
| 0 | 5 | 0 | 5 | 6.51 | 267.03 | -63.99 | 84.97 | 0.8983 | -367.0 | -435.0 | |
| 0 | 4 | 0 | 5 | 10.40 | 264.74 | -66.29 | 80.62 | 0.9145 | 42.0 | -26.6 | |
| 0 | 8 | 0 | 9 | 8.98 | 265.19 | -65.83 | 82.18 | 0.9114 | 82.0 | -9.4 | |
| 0 | 5 | 0 | 6 | 7.08 | 265.79 | -65.24 | 84.29 | 0.9074 | -219.0 | -238.8 | |
| 0 | 11 | 0 | 13 | 11.26 | 264.16 | -66.87 | 79.68 | 0.9185 | -598.0 | -434.8 | |
| 0 | 11 | 0 | 13 | 10.76 | 264.29 | -66.74 | 80.23 | 0.9176 | -228.0 | -217.8 | |
| 0 | 3 | 0 | 4 | 7.36 | 265.33 | -65.69 | 83.97 | 0.9107 | -293.0 | -313.3 | |
| 0 | 11 | 0 | 13 | 3.76 | 265.54 | -65.49 | 87.93 | 0.9103 | -408.0 | -246.2 | |
| 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. | |