SOHO MDI 2000-11-03 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 460 | 41 | 239 | -10.07 | 277.60 | 8.07 | 209.45 | 0.2904 | -1120.4 | -442.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 294 | 23 | 152 | -9.34 | 279.99 | 10.45 | 217.86 | 0.2930 | -2036.6 | -665.0 | |
| 5 | -1 | 3 | -1 | -9.73 | 279.52 | 9.99 | 215.81 | 0.2936 | -1362.4 | 999999 | |
| 12 | 54 | 6 | 28 | -9.83 | 278.50 | 8.96 | 212.71 | 0.2854 | -1436.3 | -758.4 | |
| 0 | 15 | 0 | 8 | -7.89 | 277.27 | 7.74 | 212.90 | 0.2466 | -969.0 | -799.3 | |
| 0 | 7 | 0 | 4 | -8.67 | 276.89 | 7.36 | 209.98 | 0.2546 | -555.0 | -620.1 | |
| 0 | 7 | 0 | 3 | -14.29 | 275.24 | 5.71 | 197.06 | 0.3302 | -595.0 | -658.4 | |
| 0 | 5 | 0 | 3 | -10.71 | 274.06 | 4.53 | 196.97 | 0.2672 | -629.0 | -462.7 | |
| 0 | 5 | 0 | 3 | -13.82 | 270.31 | 0.78 | 182.46 | 0.3085 | -553.0 | -498.7 | |
| 0 | 1 | 0 | 1 | -11.81 | 270.03 | 0.50 | 181.78 | 0.2746 | 669.0 | 686.5 | |
| 0 | 4 | 0 | 2 | -16.43 | 269.88 | 0.35 | 180.95 | 0.3514 | -853.0 | -722.5 | |
| 6 | 28 | 3 | 15 | -11.73 | 269.68 | 0.14 | 180.51 | 0.2732 | 1251.7 | 963.3 | |
| 0 | 8 | 0 | 4 | -13.46 | 269.60 | 0.06 | 180.21 | 0.3022 | 980.0 | 720.3 | |
| 5 | -11 | 3 | -11 | -11.65 | 269.28 | -0.25 | 179.09 | 0.2718 | 1383.2 | 999999 | |
| 0 | 4 | 0 | 2 | -13.34 | 269.16 | -0.37 | 178.79 | 0.3002 | 585.0 | 597.8 | |
| 0 | 5 | 0 | 2 | -14.55 | 268.17 | -1.37 | 175.86 | 0.3212 | 904.0 | 788.8 | |
| 6 | 23 | 3 | 12 | -13.46 | 267.46 | -2.07 | 173.33 | 0.3042 | 1222.5 | 915.6 | |
| 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. | |