SOHO MDI 2000-11-24 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 407 | 100 | 665 | -22.65 | 65.45 | 69.95 | 245.41 | 0.9515 | -291.6 | 22.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20 | 137 | 42 | 284 | -21.13 | 70.01 | 74.51 | 247.76 | 0.9722 | -257.1 | 20.7 | |
| 0 | 11 | 0 | 22 | -22.47 | 68.86 | 73.37 | 246.25 | 0.9685 | -226.0 | -237.3 | |
| 7 | 28 | 12 | 45 | -21.47 | 65.85 | 70.36 | 246.85 | 0.9546 | -513.1 | -269.1 | |
| 5 | 130 | 8 | 196 | -22.84 | 64.37 | 68.87 | 245.18 | 0.9485 | 272.9 | 23.4 | |
| 23 | -4 | 34 | -4 | -23.41 | 63.61 | 68.11 | 244.46 | 0.9452 | -520.6 | 999999 | |
| 0 | 6 | 0 | 8 | -24.21 | 61.93 | 66.44 | 243.31 | 0.9373 | -295.0 | -316.5 | |
| 0 | 2 | 0 | 2 | -23.49 | 60.50 | 65.01 | 243.77 | 0.9283 | -468.0 | -456.7 | |
| 0 | 4 | 0 | 5 | -25.16 | 59.53 | 64.04 | 241.80 | 0.9250 | -122.0 | -107.9 | |
| 0 | 3 | 0 | 3 | -25.04 | 58.08 | 62.59 | 241.60 | 0.9161 | 56.0 | 25.9 | |
| 0 | 6 | 0 | 8 | -25.38 | 57.93 | 62.43 | 241.20 | 0.9157 | 363.0 | 294.3 | |
| 0 | 2 | 0 | 3 | -25.76 | 57.82 | 62.32 | 240.77 | 0.9157 | 286.0 | 173.1 | |
| 2 | 54 | 2 | 64 | -26.25 | 56.81 | 61.32 | 240.00 | 0.9104 | 549.6 | 173.2 | |
| 0 | 2 | 0 | 2 | -25.61 | 55.37 | 59.88 | 240.30 | 0.8999 | 29.0 | 109.4 | |
| 0 | 3 | 0 | 3 | -24.91 | 53.42 | 57.93 | 240.50 | 0.8850 | 212.0 | 239.0 | |
| 0 | 5 | 0 | 6 | -26.93 | 53.22 | 57.73 | 238.26 | 0.8883 | 201.0 | 264.5 | |
| 2 | 14 | 2 | 14 | -24.81 | 51.09 | 55.60 | 239.91 | 0.8677 | 813.6 | 669.0 | |
| 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. | |