SOHO MDI 2000-07-10 20:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 423 | 43 | 390 | -18.50 | 49.31 | 53.65 | 244.97 | 0.8443 | -392.2 | -102.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 184 | 12 | 180 | -17.84 | 52.29 | 56.62 | 246.71 | 0.8674 | -554.0 | -206.3 | |
| 7 | -1 | 7 | -1 | -17.97 | 51.60 | 55.93 | 246.36 | 0.8622 | -664.4 | 999999 | |
| 3 | -1 | 3 | -1 | -17.84 | 50.79 | 55.13 | 246.26 | 0.8552 | -806.4 | 999999 | |
| 0 | 5 | 0 | 4 | -16.66 | 50.20 | 54.53 | 247.40 | 0.8472 | -627.0 | -665.9 | |
| 0 | 3 | 0 | 3 | -17.44 | 49.04 | 53.37 | 246.14 | 0.8393 | -413.0 | -416.6 | |
| 11 | 30 | 10 | 28 | -20.07 | 49.55 | 53.89 | 243.35 | 0.8511 | -625.0 | -385.2 | |
| 4 | 34 | 4 | 30 | -17.63 | 47.94 | 52.28 | 245.55 | 0.8302 | -353.5 | -143.5 | |
| 0 | 2 | 0 | 2 | -18.64 | 47.83 | 52.16 | 244.35 | 0.8323 | -566.0 | -498.2 | |
| 0 | 10 | 0 | 9 | -18.92 | 47.61 | 51.95 | 243.94 | 0.8313 | -4.0 | -135.9 | |
| 0 | 5 | 0 | 4 | -16.79 | 46.61 | 50.94 | 246.05 | 0.8156 | 197.0 | 238.3 | |
| 0 | 4 | 0 | 4 | -20.01 | 47.83 | 52.17 | 242.79 | 0.8366 | -721.0 | -591.5 | |
| 0 | 40 | 0 | 34 | -18.21 | 46.97 | 51.30 | 244.53 | 0.8233 | -229.0 | 27.6 | |
| 0 | 8 | 0 | 7 | -19.42 | 47.22 | 51.55 | 243.24 | 0.8294 | 206.0 | 64.4 | |
| 0 | 16 | 0 | 13 | -17.36 | 46.30 | 50.63 | 245.26 | 0.8146 | 742.0 | 599.4 | |
| 0 | 5 | 0 | 5 | -20.90 | 47.50 | 51.83 | 241.67 | 0.8366 | 269.0 | 152.0 | |
| 1 | 12 | 1 | 10 | -19.91 | 46.90 | 51.23 | 242.55 | 0.8282 | -618.8 | -417.0 | |
| 1 | 16 | 1 | 14 | -18.93 | 46.13 | 50.47 | 243.39 | 0.8182 | 604.7 | 616.6 | |
| 0 | 5 | 0 | 5 | -21.33 | 45.94 | 50.27 | 240.56 | 0.8248 | 323.0 | 242.7 | |
| 6 | 44 | 5 | 38 | -20.41 | 44.99 | 49.33 | 241.22 | 0.8132 | 766.6 | 111.5 | |
| 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. | |