SOHO MDI 2000-07-04 07:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26 | 172 | 21 | 139 | 19.12 | 30.57 | -51.60 | 68.37 | 0.7982 | 561.3 | 44.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11 | 46 | 9 | 36 | 19.61 | 33.90 | -48.27 | 66.97 | 0.7662 | 843.8 | 430.4 | |
| 3 | -1 | 2 | -1 | 19.88 | 33.47 | -48.70 | 66.74 | 0.7713 | 716.7 | 999999 | |
| 0 | 4 | 0 | 3 | 20.12 | 32.19 | -49.97 | 66.77 | 0.7847 | 352.0 | 311.8 | |
| 0 | 4 | 0 | 3 | 20.96 | 31.34 | -50.82 | 65.95 | 0.7950 | 402.0 | 347.6 | |
| 0 | 3 | 0 | 2 | 20.29 | 31.25 | -50.91 | 66.80 | 0.7943 | 277.0 | 283.1 | |
| 0 | 9 | 0 | 7 | 18.64 | 31.50 | -50.66 | 68.79 | 0.7883 | -570.0 | -626.2 | |
| 0 | 13 | 0 | 10 | 19.60 | 30.75 | -51.41 | 67.77 | 0.7977 | -355.0 | -284.7 | |
| 0 | 3 | 0 | 2 | 18.21 | 31.22 | -50.95 | 69.39 | 0.7904 | -487.0 | -403.6 | |
| 4 | 13 | 3 | 11 | 18.72 | 30.53 | -51.63 | 68.91 | 0.7981 | -678.3 | -529.4 | |
| 0 | 4 | 0 | 3 | 19.01 | 29.51 | -52.65 | 68.77 | 0.8086 | 55.0 | 113.3 | |
| 0 | 10 | 0 | 9 | 18.24 | 28.95 | -53.21 | 69.82 | 0.8126 | -778.0 | -434.1 | |
| 8 | 53 | 7 | 45 | 19.00 | 28.46 | -53.70 | 68.99 | 0.8185 | 910.9 | 211.8 | |
| 0 | 6 | 0 | 5 | 17.76 | 27.67 | -54.49 | 70.62 | 0.8240 | -521.0 | -475.6 | |
| 0 | 4 | 0 | 3 | 17.32 | 27.87 | -54.30 | 71.13 | 0.8214 | -667.0 | -536.0 | |
| 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. | |