SOHO MDI 2000-07-11 03:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 356 | 40 | 361 | -18.47 | 49.40 | 57.26 | 246.15 | 0.8735 | -291.9 | -105.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10 | 145 | 11 | 159 | -17.88 | 52.40 | 60.26 | 247.67 | 0.8952 | -391.9 | -153.1 | |
| 5 | -1 | 6 | -1 | -17.89 | 51.81 | 59.68 | 247.51 | 0.8910 | -684.1 | 999999 | |
| 1 | 14 | 1 | 14 | -17.16 | 50.29 | 58.16 | 247.89 | 0.8780 | -553.0 | -390.2 | |
| 0 | 4 | 0 | 4 | -17.12 | 48.27 | 56.14 | 247.35 | 0.8619 | -375.0 | -405.1 | |
| 11 | 27 | 11 | 28 | -20.14 | 49.61 | 57.48 | 244.42 | 0.8796 | -579.6 | -310.1 | |
| 0 | 20 | 0 | 20 | -17.57 | 47.96 | 55.82 | 246.76 | 0.8604 | -518.0 | -287.5 | |
| 0 | 5 | 0 | 5 | -18.91 | 47.64 | 55.51 | 245.17 | 0.8612 | -266.0 | -84.5 | |
| 2 | 17 | 1 | 16 | -19.41 | 47.45 | 55.31 | 244.55 | 0.8610 | -35.3 | -84.9 | |
| 0 | 9 | 0 | 9 | -20.16 | 47.77 | 55.63 | 243.82 | 0.8655 | -553.0 | -521.9 | |
| 2 | 38 | 1 | 35 | -17.35 | 46.40 | 54.26 | 246.52 | 0.8468 | 600.7 | 137.6 | |
| 3 | 16 | 3 | 15 | -20.06 | 46.82 | 54.69 | 243.62 | 0.8577 | -476.1 | -294.2 | |
| 0 | 6 | 0 | 6 | -17.51 | 45.62 | 53.48 | 246.08 | 0.8406 | 600.0 | 604.2 | |
| 0 | 13 | 0 | 12 | -18.81 | 46.06 | 53.93 | 244.75 | 0.8480 | 367.0 | 457.0 | |
| 0 | 4 | 0 | 3 | -21.13 | 46.00 | 53.87 | 242.14 | 0.8542 | 109.0 | 61.5 | |
| 0 | 1 | 0 | 1 | -18.26 | 44.55 | 52.41 | 244.86 | 0.8334 | 550.0 | 499.0 | |
| 7 | 37 | 6 | 34 | -20.33 | 44.88 | 52.75 | 242.63 | 0.8426 | 679.9 | 118.0 | |
| 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. | |