SOHO MDI 2000-01-26 05:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 124 | 708 | 78 | 443 | 5.13 | 71.71 | 35.85 | 286.09 | 0.6089 | -273.1 | -70.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22 | 291 | 14 | 189 | 3.72 | 75.12 | 39.27 | 282.39 | 0.6490 | 1466.7 | 559.5 | |
| 23 | -1 | 15 | -1 | 4.46 | 75.12 | 39.26 | 283.50 | 0.6512 | 1320.5 | 999999 | |
| -2 | -1 | -2 | -1 | 4.07 | 75.04 | 39.19 | 282.93 | 0.6490 | 999999 | 999999 | |
| 6 | -1 | 4 | -1 | 4.93 | 73.91 | 38.06 | 284.67 | 0.6372 | 879.0 | 999999 | |
| 0 | 7 | 0 | 4 | 4.53 | 73.06 | 37.20 | 284.40 | 0.6247 | 546.0 | 588.0 | |
| 0 | 5 | 0 | 3 | 4.78 | 72.69 | 36.83 | 284.94 | 0.6207 | 693.0 | 726.2 | |
| 3 | 9 | 2 | 6 | 3.53 | 72.52 | 36.67 | 283.04 | 0.6142 | 1042.6 | 789.3 | |
| 0 | 11 | 0 | 7 | 4.90 | 72.07 | 36.22 | 285.40 | 0.6129 | 814.0 | 748.7 | |
| 0 | 4 | 0 | 3 | 5.73 | 70.94 | 35.09 | 287.24 | 0.6012 | 413.0 | 395.7 | |
| 0 | 7 | 0 | 5 | 6.82 | 70.18 | 34.33 | 289.37 | 0.5958 | -758.0 | -624.8 | |
| 0 | 2 | 0 | 1 | 6.76 | 69.80 | 33.95 | 289.49 | 0.5905 | -608.0 | -543.6 | |
| 33 | 372 | 20 | 225 | 5.40 | 69.15 | 33.29 | 287.61 | 0.5756 | -1688.8 | -662.8 | |
| 29 | -12 | 18 | -12 | 6.61 | 69.09 | 33.24 | 289.63 | 0.5803 | -1423.1 | 999999 | |
| 5 | -12 | 3 | -12 | 5.93 | 68.91 | 33.05 | 288.63 | 0.5747 | -1548.4 | 999999 | |
| 3 | -12 | 2 | -12 | 6.31 | 68.66 | 32.80 | 289.39 | 0.5731 | -1877.2 | 999999 | |
| -13 | -12 | -13 | -12 | 6.65 | 68.50 | 32.64 | 290.05 | 0.5726 | 999999 | 999999 | |
| 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. | |