SOHO MDI 2000-11-05 08:04:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73 | 501 | 42 | 281 | 2.36 | 272.12 | 28.11 | 267.79 | 0.4727 | 1505.2 | 645.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 436 | 10 | 246 | 2.23 | 273.50 | 29.49 | 267.74 | 0.4942 | 1325.7 | 712.3 | |
| 15 | -1 | 9 | -1 | 2.05 | 273.10 | 29.08 | 267.32 | 0.4883 | 1669.4 | 999999 | |
| 5 | -1 | 3 | -1 | 1.83 | 272.74 | 28.73 | 266.81 | 0.4832 | 1547.0 | 999999 | |
| 5 | -1 | 3 | -1 | 3.22 | 272.69 | 28.67 | 269.69 | 0.4811 | 983.9 | 999999 | |
| 0 | 5 | 0 | 3 | 3.87 | 272.71 | 28.70 | 271.05 | 0.4811 | 870.0 | 711.8 | |
| 7 | -1 | 4 | -1 | 2.18 | 272.53 | 28.51 | 267.51 | 0.4795 | 1438.3 | 999999 | |
| 23 | -1 | 13 | -1 | 2.69 | 272.32 | 28.31 | 268.55 | 0.4758 | 1844.9 | 999999 | |
| 0 | 5 | 0 | 3 | 1.56 | 271.60 | 27.59 | 266.02 | 0.4660 | 890.0 | 687.2 | |
| 0 | 6 | 0 | 3 | 3.56 | 271.56 | 27.55 | 270.34 | 0.4635 | 973.0 | 852.5 | |
| 0 | 3 | 0 | 2 | -0.01 | 271.29 | 27.27 | 262.58 | 0.4640 | 549.0 | 482.6 | |
| 0 | 9 | 0 | 5 | 0.95 | 269.95 | 25.94 | 264.31 | 0.4414 | 638.0 | 744.8 | |
| 0 | 5 | 0 | 3 | 3.95 | 266.04 | 22.03 | 271.04 | 0.3759 | 705.0 | 526.8 | |
| 0 | 6 | 0 | 3 | 2.04 | 265.42 | 21.41 | 265.80 | 0.3674 | 548.0 | 619.0 | |
| 0 | 5 | 0 | 2 | 2.41 | 262.72 | 18.71 | 266.18 | 0.3227 | -850.0 | -693.0 | |
| 0 | 13 | 0 | 7 | 1.95 | 262.60 | 18.58 | 264.71 | 0.3213 | -469.0 | -672.7 | |
| 0 | 8 | 0 | 4 | 2.80 | 262.20 | 18.19 | 267.30 | 0.3135 | -767.0 | -625.5 | |
| 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. | |