SOHO MDI 1999-12-03 20:47:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 126 | 649 | 197 | 965 | 10.45 | 308.61 | -70.23 | 79.04 | 0.9388 | 114.3 | 39.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 9 | 0 | 25 | 13.71 | 299.23 | -79.61 | 76.15 | 0.9850 | 265.0 | 180.4 | |
| 0 | 2 | 0 | 2 | 11.04 | 315.58 | -63.26 | 77.92 | 0.8982 | 230.0 | 276.7 | |
| 18 | 41 | 25 | 57 | 11.02 | 309.99 | -68.85 | 78.39 | 0.9361 | -509.9 | -164.2 | |
| 22 | 418 | 26 | 489 | 10.12 | 314.66 | -64.18 | 79.02 | 0.9045 | 1069.8 | 208.5 | |
| 18 | 136 | 39 | 300 | 11.39 | 302.66 | -76.17 | 78.40 | 0.9728 | -543.7 | -212.5 | |
| 11 | -4 | 13 | -4 | 10.13 | 312.98 | -65.85 | 79.14 | 0.9164 | 290.3 | 999999 | |
| 2 | -3 | 2 | -3 | 10.38 | 310.43 | -68.41 | 79.05 | 0.9332 | 223.0 | 999999 | |
| 17 | -4 | 21 | -4 | 9.76 | 313.89 | -64.95 | 79.47 | 0.9099 | 569.9 | 999999 | |
| 23 | -5 | 54 | -5 | 11.09 | 301.49 | -77.35 | 78.75 | 0.9772 | -119.9 | 999999 | |
| 15 | -4 | 17 | -4 | 9.43 | 314.58 | -64.25 | 79.79 | 0.9047 | 1136.7 | 999999 | |
| 0 | 3 | 0 | 4 | 9.83 | 310.45 | -68.39 | 79.64 | 0.9329 | 11.0 | -6.6 | |
| 0 | 24 | 0 | 48 | 9.93 | 303.36 | -75.48 | 79.88 | 0.9698 | -362.0 | -327.4 | |
| 0 | 5 | 0 | 14 | 10.06 | 299.19 | -79.65 | 79.87 | 0.9848 | 306.0 | 308.0 | |
| 0 | 11 | 0 | 26 | 9.37 | 300.81 | -78.02 | 80.53 | 0.9795 | -139.0 | -4.5 | |
| 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. | |