SOHO MDI 2002-08-01 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 164 | 22 | 87 | -8.54 | 144.98 | -10.36 | 144.68 | 0.3065 | 162.1 | 182.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 9 | 1 | 4 | -8.85 | 150.15 | -5.18 | 160.55 | 0.2693 | -1045.6 | -887.5 | |
| 0 | 4 | 0 | 2 | -8.73 | 149.59 | -5.74 | 158.47 | 0.2707 | -850.0 | -631.5 | |
| 0 | 5 | 0 | 3 | -7.93 | 148.24 | -7.10 | 152.68 | 0.2679 | 867.0 | 792.7 | |
| 0 | 5 | 0 | 3 | -7.16 | 148.25 | -7.08 | 151.33 | 0.2562 | 932.0 | 850.9 | |
| 0 | 5 | 0 | 3 | -7.52 | 148.04 | -7.29 | 151.32 | 0.2634 | 978.0 | 868.5 | |
| 7 | 34 | 4 | 18 | -8.20 | 146.18 | -9.16 | 146.83 | 0.2893 | -1318.1 | -413.2 | |
| 3 | -6 | 2 | -6 | -8.53 | 146.17 | -9.17 | 147.42 | 0.2939 | -941.1 | 999999 | |
| 0 | 5 | 0 | 3 | -8.00 | 145.90 | -9.44 | 145.65 | 0.2891 | -714.0 | -658.6 | |
| 0 | 4 | 0 | 2 | -8.46 | 145.64 | -9.69 | 145.81 | 0.2977 | -732.0 | -512.3 | |
| 5 | 12 | 3 | 6 | -8.75 | 145.51 | -9.82 | 146.00 | 0.3029 | -970.9 | -553.1 | |
| 0 | 3 | 0 | 2 | -8.88 | 145.06 | -10.27 | 145.05 | 0.3090 | -259.0 | -354.5 | |
| 0 | 3 | 0 | 2 | -8.23 | 144.59 | -10.74 | 142.57 | 0.3049 | 605.0 | 487.8 | |
| 0 | 11 | 0 | 6 | -8.33 | 144.02 | -11.32 | 141.31 | 0.3120 | -305.0 | -71.4 | |
| 0 | 9 | 0 | 4 | -8.54 | 143.52 | -11.81 | 140.54 | 0.3199 | 664.0 | 320.5 | |
| 0 | 3 | 0 | 2 | -8.87 | 143.31 | -12.03 | 140.68 | 0.3264 | 604.0 | 540.9 | |
| 0 | 3 | 0 | 1 | -8.35 | 143.04 | -12.30 | 139.00 | 0.3227 | 845.0 | 790.1 | |
| 4 | 35 | 2 | 19 | -9.34 | 142.64 | -12.70 | 140.05 | 0.3394 | 1248.4 | 923.5 | |
| 4 | -17 | 2 | -17 | -9.01 | 142.44 | -12.89 | 139.00 | 0.3374 | 1363.8 | 999999 | |
| 8 | 14 | 4 | 7 | -8.57 | 142.25 | -13.08 | 137.69 | 0.3340 | 1213.8 | 906.5 | |
| 8 | -17 | 4 | -17 | -9.19 | 142.07 | -13.27 | 138.51 | 0.3436 | 1115.2 | 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. | |