SOHO MDI 1999-04-11 09:35:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 243 | 31 | 143 | -18.24 | 233.29 | -29.28 | 115.90 | 0.5179 | -295.0 | 88.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 16 | 4 | 9 | -16.57 | 237.18 | -25.40 | 115.23 | 0.4564 | -1102.4 | -660.9 | |
| 0 | 3 | 0 | 2 | -16.95 | 236.94 | -25.64 | 115.85 | 0.4618 | -651.0 | -528.7 | |
| 14 | 79 | 8 | 45 | -17.42 | 235.78 | -26.80 | 115.95 | 0.4804 | -1564.1 | -929.9 | |
| 0 | 3 | 0 | 2 | -18.05 | 235.58 | -26.99 | 117.04 | 0.4865 | -282.0 | -348.9 | |
| 8 | -3 | 5 | -3 | -17.20 | 235.40 | -27.18 | 115.27 | 0.4845 | -1331.8 | 999999 | |
| 0 | 3 | 0 | 2 | -17.87 | 235.24 | -27.33 | 116.47 | 0.4902 | -622.0 | -499.9 | |
| 4 | 10 | 2 | 6 | -17.46 | 234.06 | -28.51 | 114.91 | 0.5041 | -594.2 | -616.9 | |
| 0 | 5 | 0 | 3 | -18.78 | 232.36 | -30.22 | 116.28 | 0.5335 | 543.0 | 484.9 | |
| 0 | 4 | 0 | 2 | -16.91 | 232.61 | -29.96 | 113.05 | 0.5214 | -204.0 | -120.8 | |
| 2 | 35 | 1 | 20 | -19.60 | 231.95 | -30.63 | 117.47 | 0.5431 | 1199.0 | 757.6 | |
| 3 | -10 | 2 | -10 | -19.98 | 231.53 | -31.05 | 117.88 | 0.5505 | 941.1 | 999999 | |
| 0 | 8 | 0 | 5 | -19.10 | 231.62 | -30.96 | 116.41 | 0.5448 | 813.0 | 812.5 | |
| 4 | 15 | 2 | 9 | -19.41 | 231.31 | -31.26 | 116.76 | 0.5503 | 1102.7 | 1042.1 | |
| 0 | 6 | 0 | 4 | -17.83 | 231.01 | -31.56 | 113.85 | 0.5470 | 637.0 | 484.8 | |
| 3 | 35 | 2 | 21 | -19.17 | 230.64 | -31.94 | 115.98 | 0.5580 | 988.1 | 754.9 | |
| 8 | 21 | 5 | 13 | -18.29 | 230.77 | -31.80 | 114.54 | 0.5522 | 1212.7 | 825.1 | |
| 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. | |