SOHO MDI 2000-09-05 18:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49 | 195 | 25 | 99 | 9.61 | 340.58 | 17.97 | 279.67 | 0.3118 | -767.1 | -238.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | 2.93 | 348.39 | 25.79 | 261.77 | 0.4408 | 662.0 | 447.6 | |
| 0 | 6 | 0 | 3 | 6.68 | 345.81 | 23.20 | 270.01 | 0.3930 | -890.0 | -723.3 | |
| 0 | 6 | 0 | 3 | 6.95 | 344.24 | 21.63 | 270.55 | 0.3676 | -904.0 | -774.1 | |
| 0 | 3 | 0 | 2 | 6.97 | 343.90 | 21.29 | 270.56 | 0.3621 | -886.0 | -757.1 | |
| 0 | 10 | 0 | 5 | 9.23 | 343.35 | 20.74 | 276.93 | 0.3536 | 883.0 | 701.9 | |
| 0 | 9 | 0 | 5 | 4.12 | 342.53 | 19.93 | 262.11 | 0.3447 | -473.0 | -584.8 | |
| 0 | 5 | 0 | 2 | 3.77 | 342.44 | 19.83 | 261.06 | 0.3442 | -877.0 | -767.2 | |
| 0 | 2 | 0 | 1 | 10.74 | 342.04 | 19.44 | 281.72 | 0.3354 | 558.0 | 457.1 | |
| 2 | 29 | 1 | 15 | 9.61 | 341.72 | 19.11 | 278.45 | 0.3278 | 1124.6 | 842.2 | |
| 0 | 4 | 0 | 2 | 10.20 | 341.67 | 19.06 | 280.27 | 0.3281 | 809.0 | 666.0 | |
| 10 | -9 | 5 | -9 | 9.46 | 341.50 | 18.89 | 278.06 | 0.3240 | 1408.3 | 999999 | |
| 0 | 12 | 0 | 6 | 10.35 | 340.84 | 18.23 | 281.08 | 0.3150 | 521.0 | 460.1 | |
| 0 | 5 | 0 | 2 | 9.97 | 339.56 | 16.96 | 280.41 | 0.2933 | -404.0 | -300.6 | |
| 5 | 92 | 3 | 47 | 11.04 | 339.16 | 16.56 | 284.29 | 0.2899 | -1012.7 | -778.3 | |
| 32 | -14 | 16 | -14 | 11.06 | 338.62 | 16.02 | 284.74 | 0.2813 | -1630.9 | 999999 | |
| 0 | 6 | 0 | 3 | 12.72 | 335.94 | 13.33 | 293.67 | 0.2467 | 741.0 | 663.2 | |
| 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. | |