SOHO MDI 2000-10-05 14:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36 | 320 | 44 | 388 | -12.05 | 352.62 | 63.45 | 253.49 | 0.9096 | 116.8 | 107.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 135 | 24 | 205 | -11.17 | 358.17 | 69.00 | 255.79 | 0.9463 | -419.8 | -97.2 | |
| 0 | 11 | 0 | 13 | -12.89 | 351.06 | 61.89 | 252.37 | 0.9040 | -498.0 | -376.7 | |
| 0 | 2 | 0 | 2 | -12.51 | 350.47 | 61.30 | 252.64 | 0.8991 | -289.0 | -356.5 | |
| 1 | 11 | 1 | 12 | -11.79 | 349.86 | 60.69 | 253.25 | 0.8933 | -393.5 | -313.7 | |
| 0 | 5 | 0 | 5 | -13.50 | 349.40 | 60.23 | 251.28 | 0.8931 | -204.0 | -218.6 | |
| 0 | 4 | 0 | 4 | -13.35 | 347.91 | 58.74 | 251.02 | 0.8815 | 387.0 | 330.2 | |
| 0 | 8 | 0 | 8 | -12.96 | 347.69 | 58.52 | 251.39 | 0.8789 | -86.0 | -55.7 | |
| 0 | 3 | 0 | 3 | -11.68 | 346.71 | 57.54 | 252.52 | 0.8683 | 177.0 | 227.5 | |
| 0 | 3 | 0 | 3 | -14.17 | 346.71 | 57.55 | 249.76 | 0.8740 | 305.0 | 210.7 | |
| 0 | 5 | 0 | 5 | -13.76 | 346.33 | 57.16 | 250.09 | 0.8700 | 470.0 | 452.6 | |
| 0 | 3 | 0 | 3 | -11.55 | 345.35 | 56.18 | 252.27 | 0.8566 | 563.0 | 492.3 | |
| 6 | 84 | 6 | 81 | -12.61 | 345.40 | 56.23 | 251.09 | 0.8596 | 840.8 | 645.2 | |
| 3 | -12 | 3 | -12 | -12.13 | 345.03 | 55.86 | 251.52 | 0.8553 | 933.9 | 999999 | |
| 6 | -12 | 6 | -12 | -13.21 | 345.25 | 56.08 | 250.38 | 0.8597 | 867.5 | 999999 | |
| 4 | 46 | 4 | 44 | -13.91 | 345.29 | 56.12 | 249.61 | 0.8618 | 650.0 | 312.3 | |
| 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. | |