SOHO MDI 2000-11-04 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64 | 508 | 35 | 274 | 2.42 | 272.01 | 23.56 | 267.18 | 0.4013 | 1615.8 | 698.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 442 | 18 | 240 | 2.06 | 273.17 | 24.72 | 266.52 | 0.4205 | 1700.4 | 770.7 | |
| 5 | -1 | 3 | -1 | 3.19 | 272.60 | 24.15 | 269.16 | 0.4103 | 1041.9 | 999999 | |
| 0 | 13 | 0 | 7 | 3.93 | 272.50 | 24.05 | 270.96 | 0.4083 | 1090.0 | 873.3 | |
| 4 | -1 | 2 | -1 | 2.20 | 272.41 | 23.96 | 266.70 | 0.4083 | 1578.5 | 999999 | |
| 22 | -1 | 12 | -1 | 2.70 | 272.25 | 23.80 | 267.91 | 0.4052 | 1941.3 | 999999 | |
| 0 | 7 | 0 | 4 | 1.45 | 271.65 | 23.20 | 264.65 | 0.3972 | 1085.0 | 870.3 | |
| 0 | 5 | 0 | 2 | -0.08 | 271.35 | 22.89 | 260.70 | 0.3959 | 575.0 | 502.9 | |
| 0 | 6 | 0 | 3 | 2.59 | 265.91 | 17.46 | 266.30 | 0.3017 | 772.0 | 644.0 | |
| 0 | 4 | 0 | 2 | 1.11 | 264.53 | 16.08 | 260.65 | 0.2819 | 591.0 | 474.7 | |
| 0 | 4 | 0 | 2 | 5.01 | 263.83 | 15.37 | 274.81 | 0.2663 | -739.0 | -679.9 | |
| 0 | 4 | 0 | 2 | 0.36 | 263.57 | 15.12 | 257.25 | 0.2686 | 624.0 | 537.3 | |
| 0 | 3 | 0 | 2 | 4.60 | 263.02 | 14.57 | 273.39 | 0.2523 | -712.0 | -577.8 | |
| 0 | 5 | 0 | 2 | 2.49 | 262.55 | 14.10 | 264.82 | 0.2454 | -978.0 | -820.7 | |
| 0 | 4 | 0 | 2 | 0.88 | 262.49 | 14.04 | 258.30 | 0.2489 | 667.0 | 559.6 | |
| 0 | 5 | 0 | 3 | 2.92 | 262.39 | 13.94 | 266.51 | 0.2422 | -810.0 | -809.7 | |
| 0 | 6 | 0 | 3 | 4.43 | 261.62 | 13.17 | 272.89 | 0.2285 | -937.0 | -890.7 | |
| 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. | |