SOHO MDI 2000-11-10 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54 | 383 | 28 | 200 | -12.70 | 176.88 | 7.49 | 204.76 | 0.3040 | 1498.9 | 551.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 17 | 0 | 9 | -12.90 | 179.10 | 9.70 | 210.70 | 0.3232 | -934.0 | -443.8 | |
| 0 | 5 | 0 | 3 | -12.58 | 178.69 | 9.29 | 210.15 | 0.3152 | -219.0 | -169.8 | |
| 12 | 312 | 6 | 162 | -13.25 | 177.63 | 8.24 | 206.26 | 0.3167 | 1288.2 | 765.9 | |
| 13 | -3 | 7 | -3 | -12.21 | 177.44 | 8.05 | 207.28 | 0.2998 | 2000.2 | 999999 | |
| 13 | -3 | 7 | -3 | -12.84 | 177.18 | 7.79 | 205.57 | 0.3074 | 1548.6 | 999999 | |
| 16 | -3 | 8 | -3 | -12.72 | 176.78 | 7.39 | 204.59 | 0.3027 | 1730.0 | 999999 | |
| 0 | 4 | 0 | 2 | -19.07 | 176.73 | 7.34 | 197.68 | 0.3992 | -491.0 | -673.3 | |
| 0 | 3 | 0 | 2 | -13.48 | 176.33 | 6.93 | 202.26 | 0.3112 | 534.0 | 451.8 | |
| 0 | 3 | 0 | 2 | -12.63 | 175.83 | 6.43 | 201.85 | 0.2951 | 683.0 | 578.3 | |
| 0 | 4 | 0 | 2 | -13.35 | 175.69 | 6.29 | 200.53 | 0.3054 | 664.0 | 652.9 | |
| 0 | 6 | 0 | 3 | -8.59 | 174.73 | 5.33 | 204.22 | 0.2250 | -821.0 | -755.8 | |
| 0 | 6 | 0 | 3 | -9.57 | 173.88 | 4.49 | 199.24 | 0.2352 | -760.0 | -632.1 | |
| 0 | 4 | 0 | 2 | -14.18 | 173.32 | 3.93 | 192.53 | 0.3075 | -706.0 | -594.4 | |
| 0 | 5 | 0 | 3 | -13.30 | 172.87 | 3.48 | 191.74 | 0.2915 | -716.0 | -609.4 | |
| 0 | 5 | 0 | 3 | -12.49 | 171.80 | 2.40 | 188.60 | 0.2750 | -698.0 | -622.4 | |
| 0 | 9 | 0 | 4 | -11.62 | 170.34 | 0.94 | 183.61 | 0.2576 | -764.0 | -567.9 | |
| 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. | |