SOHO MDI 2000-09-22 19:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98 | 409 | 52 | 215 | -5.74 | 81.75 | -16.07 | 128.54 | 0.3525 | -194.4 | -89.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 84 | 4 | 44 | -5.63 | 85.13 | -12.68 | 134.65 | 0.3086 | -1722.4 | -862.0 | |
| 4 | -1 | 2 | -1 | -5.19 | 85.02 | -12.80 | 133.38 | 0.3048 | -1129.1 | 999999 | |
| 8 | -1 | 4 | -1 | -5.87 | 84.89 | -12.93 | 134.66 | 0.3144 | -1317.1 | 999999 | |
| 6 | -1 | 3 | -1 | -5.52 | 84.81 | -13.00 | 133.68 | 0.3110 | -1578.4 | 999999 | |
| 17 | 66 | 9 | 34 | -5.82 | 84.12 | -13.70 | 132.87 | 0.3228 | -1440.7 | -687.7 | |
| 8 | 15 | 4 | 8 | -6.07 | 83.47 | -14.35 | 132.10 | 0.3336 | -1023.1 | -829.1 | |
| 6 | 46 | 3 | 24 | -6.42 | 82.77 | -15.05 | 131.49 | 0.3459 | -913.3 | -719.5 | |
| 0 | 6 | 0 | 3 | -4.99 | 82.48 | -15.33 | 127.71 | 0.3345 | -687.0 | -598.7 | |
| 0 | 4 | 0 | 2 | -5.12 | 82.16 | -15.66 | 127.41 | 0.3400 | -547.0 | -469.0 | |
| 0 | 5 | 0 | 3 | -5.99 | 81.32 | -16.50 | 127.91 | 0.3596 | 158.0 | 185.9 | |
| 3 | 12 | 2 | 6 | -6.27 | 80.28 | -17.54 | 126.80 | 0.3757 | 1007.0 | 759.9 | |
| 7 | 23 | 4 | 12 | -4.12 | 80.10 | -17.72 | 121.67 | 0.3583 | 1202.3 | 833.2 | |
| 3 | 33 | 1 | 18 | -7.04 | 79.92 | -17.90 | 127.85 | 0.3879 | 860.2 | 839.8 | |
| 9 | -13 | 5 | -13 | -6.73 | 79.64 | -18.17 | 126.78 | 0.3884 | 1217.1 | 999999 | |
| 0 | 12 | 0 | 6 | -5.98 | 79.47 | -18.35 | 124.92 | 0.3836 | 939.0 | 685.6 | |
| 0 | 4 | 0 | 2 | -4.66 | 79.51 | -18.31 | 122.07 | 0.3711 | 445.0 | 385.9 | |
| 0 | 9 | 0 | 5 | -4.93 | 78.71 | -19.10 | 121.56 | 0.3843 | 889.0 | 633.7 | |
| 9 | 90 | 5 | 48 | -5.46 | 78.49 | -19.33 | 122.40 | 0.3919 | 1443.6 | 633.4 | |
| 11 | -18 | 6 | -18 | -5.55 | 78.24 | -19.58 | 122.25 | 0.3961 | 1230.6 | 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. | |