SOHO MDI 2000-07-17 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82 | 578 | 45 | 322 | 19.19 | 289.07 | 22.55 | 305.48 | 0.4463 | 281.8 | 157.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | 22.28 | 293.24 | 26.72 | 306.75 | 0.5214 | 439.0 | 349.0 | |
| 18 | 340 | 10 | 190 | 19.42 | 290.84 | 24.32 | 303.97 | 0.4703 | 1429.1 | 673.1 | |
| 28 | -2 | 16 | -2 | 18.53 | 290.52 | 24.00 | 302.59 | 0.4596 | 1808.9 | 999999 | |
| 0 | 6 | 0 | 4 | 23.35 | 291.17 | 24.65 | 310.52 | 0.5058 | 913.0 | 681.4 | |
| -3 | -2 | -3 | -2 | 18.83 | 290.29 | 23.77 | 303.38 | 0.4588 | 999999 | 999999 | |
| 0 | 6 | 0 | 4 | 19.90 | 288.72 | 22.20 | 307.09 | 0.4473 | 560.0 | 447.9 | |
| 0 | 4 | 0 | 2 | 19.34 | 288.37 | 21.85 | 306.40 | 0.4381 | -639.0 | -432.6 | |
| 0 | 3 | 0 | 2 | 19.10 | 288.06 | 21.54 | 306.29 | 0.4323 | -417.0 | -442.4 | |
| 8 | 175 | 4 | 95 | 18.63 | 287.24 | 20.72 | 306.32 | 0.4179 | -963.9 | -704.0 | |
| 0 | 5 | 0 | 3 | 21.31 | 287.02 | 20.50 | 311.76 | 0.4393 | -426.0 | -459.2 | |
| 28 | -9 | 15 | -9 | 18.90 | 286.52 | 20.00 | 307.77 | 0.4110 | -1721.5 | 999999 | |
| 0 | 22 | 0 | 12 | 21.15 | 286.68 | 20.16 | 311.92 | 0.4338 | -806.0 | -776.1 | |
| 0 | 7 | 0 | 4 | 21.81 | 285.47 | 18.95 | 314.76 | 0.4263 | -714.0 | -410.0 | |
| 0 | 5 | 0 | 3 | 21.49 | 281.03 | 14.51 | 321.40 | 0.3753 | -734.0 | -584.7 | |
| 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. | |