SOHO MDI 2000-09-27 09:55:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 199 | 32 | 160 | -12.23 | 348.75 | -48.41 | 111.55 | 0.7868 | 152.5 | 155.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 12 | 4 | 9 | -11.91 | 356.60 | -40.55 | 114.77 | 0.7029 | -914.1 | -730.0 | |
| 7 | 15 | 5 | 11 | -11.53 | 356.14 | -41.01 | 114.03 | 0.7063 | -841.2 | -662.6 | |
| 0 | 9 | 0 | 6 | -11.46 | 352.63 | -44.53 | 112.21 | 0.7447 | -566.0 | -551.5 | |
| 0 | 5 | 0 | 4 | -12.52 | 351.72 | -45.43 | 113.12 | 0.7586 | -290.0 | -173.7 | |
| 0 | 7 | 0 | 5 | -11.58 | 350.31 | -46.84 | 111.35 | 0.7695 | 493.0 | 330.7 | |
| 0 | 6 | 0 | 5 | -13.34 | 349.48 | -47.68 | 113.12 | 0.7845 | -515.0 | -317.4 | |
| 2 | 9 | 2 | 7 | -13.60 | 348.93 | -48.23 | 113.20 | 0.7909 | -560.1 | -358.1 | |
| 0 | 2 | 0 | 1 | -13.00 | 348.30 | -48.85 | 112.22 | 0.7949 | 496.0 | 449.7 | |
| 0 | 3 | 0 | 2 | -10.54 | 348.83 | -48.33 | 109.47 | 0.7812 | 478.0 | 486.4 | |
| 7 | 27 | 5 | 22 | -10.96 | 347.76 | -49.39 | 109.57 | 0.7933 | 643.7 | 711.1 | |
| 0 | 3 | 0 | 3 | -12.28 | 347.26 | -49.90 | 110.95 | 0.8026 | 516.0 | 441.4 | |
| 7 | 57 | 6 | 48 | -13.64 | 346.75 | -50.40 | 112.35 | 0.8119 | 685.4 | 393.6 | |
| 0 | 2 | 0 | 2 | -11.34 | 347.18 | -49.97 | 109.81 | 0.8003 | 560.0 | 424.2 | |
| 11 | 35 | 9 | 29 | -11.43 | 346.66 | -50.50 | 109.73 | 0.8057 | 670.6 | 152.6 | |
| 2 | 7 | 1 | 6 | -10.60 | 346.42 | -50.74 | 108.65 | 0.8055 | 505.0 | 423.3 | |
| 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. | |