SOHO MDI 2000-07-16 12:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25 | 141 | 14 | 73 | 20.55 | 288.40 | 7.76 | 335.97 | 0.3071 | 559.1 | 216.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 27.68 | 297.16 | 16.52 | 327.53 | 0.4709 | -497.0 | -393.0 | |
| 0 | 13 | 0 | 7 | 21.26 | 293.42 | 12.78 | 324.52 | 0.3568 | 880.0 | 708.6 | |
| 0 | 5 | 0 | 3 | 24.82 | 292.97 | 12.33 | 330.89 | 0.4000 | 953.0 | 750.6 | |
| 3 | 24 | 2 | 13 | 19.96 | 289.29 | 8.65 | 332.07 | 0.3030 | 1202.3 | 707.1 | |
| 9 | 29 | 5 | 15 | 19.10 | 289.20 | 8.56 | 330.84 | 0.2899 | 1323.8 | 862.8 | |
| 2 | -5 | 1 | -5 | 18.82 | 289.06 | 8.42 | 330.73 | 0.2846 | 1098.8 | 999999 | |
| 5 | -4 | 3 | -4 | 20.17 | 289.00 | 8.36 | 333.18 | 0.3038 | 829.9 | 999999 | |
| 0 | 4 | 0 | 2 | 19.08 | 286.96 | 6.32 | 337.51 | 0.2732 | -552.0 | -413.1 | |
| 0 | 10 | 0 | 5 | 19.13 | 286.37 | 5.73 | 339.47 | 0.2703 | 802.0 | 522.3 | |
| 0 | 10 | 0 | 5 | 21.31 | 286.20 | 5.56 | 342.64 | 0.3037 | -1169.0 | -864.6 | |
| 0 | 5 | 0 | 2 | 19.13 | 286.00 | 5.35 | 340.72 | 0.2682 | 616.0 | 569.0 | |
| 6 | 16 | 3 | 8 | 21.27 | 285.60 | 4.96 | 344.37 | 0.3003 | -1129.5 | -803.9 | |
| 0 | 7 | 0 | 4 | 20.20 | 285.44 | 4.80 | 343.79 | 0.2824 | -607.0 | -511.9 | |
| 0 | 5 | 0 | 2 | 20.86 | 285.08 | 4.44 | 345.57 | 0.2914 | -677.0 | -616.2 | |
| 0 | 4 | 0 | 2 | 19.75 | 285.00 | 4.36 | 344.74 | 0.2732 | 369.0 | 291.6 | |
| 0 | 6 | 0 | 3 | 21.15 | 284.75 | 4.11 | 346.85 | 0.2948 | -951.0 | -747.4 | |
| 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. | |