SOHO MDI 2002-04-07 15:59:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 158 | 17 | 81 | -2.12 | 260.86 | 14.73 | 285.13 | 0.2642 | -313.1 | -137.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 74 | 2 | 38 | -2.04 | 262.76 | 16.62 | 283.40 | 0.2952 | -1375.7 | -925.9 | |
| 9 | -1 | 5 | -1 | -1.90 | 262.51 | 16.38 | 284.11 | 0.2919 | -1686.1 | 999999 | |
| 5 | -1 | 3 | -1 | -2.44 | 262.48 | 16.34 | 282.31 | 0.2890 | -1324.0 | 999999 | |
| 0 | 3 | 0 | 2 | -2.12 | 261.71 | 15.57 | 284.11 | 0.2778 | -692.0 | -641.3 | |
| 0 | 5 | 0 | 3 | -2.32 | 261.47 | 15.33 | 283.63 | 0.2730 | -1250.0 | -872.3 | |
| 0 | 5 | 0 | 3 | -2.01 | 261.22 | 15.08 | 284.95 | 0.2704 | -641.0 | -600.9 | |
| 0 | 10 | 0 | 5 | -2.21 | 259.82 | 13.68 | 285.77 | 0.2467 | 490.0 | 473.5 | |
| 2 | 27 | 1 | 14 | -2.14 | 259.18 | 13.04 | 286.81 | 0.2366 | 1100.4 | 973.4 | |
| 2 | -8 | 1 | -8 | -1.99 | 258.93 | 12.80 | 287.74 | 0.2335 | 1441.4 | 999999 | |
| 0 | 3 | 0 | 1 | -2.58 | 258.82 | 12.68 | 285.45 | 0.2286 | 682.0 | 697.8 | |
| 4 | 10 | 2 | 5 | -1.93 | 258.50 | 12.36 | 288.65 | 0.2268 | 1234.4 | 839.9 | |
| 7 | 17 | 3 | 8 | -2.47 | 258.46 | 12.32 | 286.38 | 0.2233 | 1523.2 | 930.4 | |
| 0 | 4 | 0 | 2 | -1.58 | 258.37 | 12.24 | 290.28 | 0.2269 | 789.0 | 721.0 | |
| 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. | |