SOHO MDI 2000-09-29 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 110 | 912 | 161 | 1322 | 9.66 | 80.88 | 70.81 | 277.87 | 0.9404 | 425.8 | 270.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15 | 805 | 27 | 1193 | 9.28 | 84.88 | 74.81 | 277.76 | 0.9624 | 33.9 | 308.2 | |
| 20 | -1 | 31 | -1 | 9.85 | 82.64 | 72.56 | 278.18 | 0.9510 | 139.0 | 999999 | |
| 5 | -1 | 8 | -1 | 9.91 | 81.75 | 71.68 | 278.18 | 0.9462 | 489.5 | 999999 | |
| 0 | 5 | 0 | 7 | 11.70 | 82.43 | 72.36 | 280.12 | 0.9493 | -196.0 | -61.2 | |
| 0 | 11 | 0 | 17 | 12.25 | 82.53 | 72.46 | 280.70 | 0.9497 | -66.0 | -62.6 | |
| 22 | -1 | 31 | -1 | 8.70 | 80.55 | 70.48 | 276.81 | 0.9398 | 573.3 | 999999 | |
| -6 | -1 | -6 | -1 | 9.10 | 80.49 | 70.42 | 277.24 | 0.9393 | 999999 | 999999 | |
| 19 | -1 | 26 | -1 | 9.63 | 80.02 | 69.95 | 277.76 | 0.9363 | 697.3 | 999999 | |
| 17 | -1 | 23 | -1 | 10.38 | 80.04 | 69.97 | 278.57 | 0.9361 | 676.8 | 999999 | |
| 12 | -1 | 15 | -1 | 9.01 | 78.09 | 68.01 | 276.97 | 0.9243 | 621.5 | 999999 | |
| 0 | 21 | 0 | 27 | 8.03 | 77.62 | 67.55 | 275.88 | 0.9217 | 355.0 | 243.4 | |
| 0 | 15 | 0 | 17 | 10.71 | 75.83 | 65.76 | 278.70 | 0.9082 | 57.0 | 127.1 | |
| 0 | 15 | 0 | 16 | 8.91 | 73.85 | 63.78 | 276.59 | 0.8941 | -398.0 | -257.1 | |
| 0 | 5 | 0 | 6 | 11.88 | 74.90 | 64.83 | 279.96 | 0.9011 | -234.0 | -152.3 | |
| 0 | 8 | 0 | 9 | 13.78 | 75.76 | 65.68 | 282.09 | 0.9069 | -473.0 | -331.4 | |
| 0 | 5 | 0 | 6 | 13.07 | 74.99 | 64.92 | 281.28 | 0.9015 | -319.0 | -330.8 | |
| 0 | 10 | 0 | 12 | 12.74 | 74.65 | 64.57 | 280.91 | 0.8990 | -449.0 | -410.4 | |
| 0 | 3 | 0 | 3 | 8.41 | 72.56 | 62.49 | 275.95 | 0.8841 | -449.0 | -342.6 | |
| 0 | 9 | 0 | 9 | 12.22 | 71.24 | 61.17 | 280.25 | 0.8721 | -51.0 | -94.2 | |
| 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. | |