SOHO MDI 2000-07-13 07:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40 | 194 | 22 | 103 | -10.34 | 306.83 | -16.18 | 132.40 | 0.3721 | -430.1 | -368.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 2 | -10.26 | 310.97 | -12.03 | 140.50 | 0.3240 | -960.0 | -911.6 | |
| 0 | 7 | 0 | 4 | -9.54 | 310.51 | -12.50 | 137.93 | 0.3200 | -1243.0 | -972.2 | |
| 0 | 5 | 0 | 3 | -9.71 | 310.05 | -12.96 | 137.26 | 0.3272 | -908.0 | -660.4 | |
| 3 | 8 | 2 | 4 | -10.08 | 309.54 | -13.47 | 136.94 | 0.3374 | -744.2 | -636.9 | |
| 0 | 6 | 0 | 3 | -10.34 | 309.07 | -13.94 | 136.49 | 0.3457 | -435.0 | -490.4 | |
| 0 | 6 | 0 | 3 | -9.24 | 308.99 | -14.01 | 134.01 | 0.3338 | 421.0 | 396.2 | |
| 0 | 4 | 0 | 2 | -10.63 | 308.68 | -14.33 | 136.30 | 0.3535 | -398.0 | -300.4 | |
| 2 | 11 | 1 | 6 | -10.28 | 307.83 | -15.18 | 133.93 | 0.3594 | 1179.1 | 806.9 | |
| 3 | 129 | 1 | 69 | -10.02 | 306.67 | -16.34 | 131.30 | 0.3704 | 1168.7 | -453.5 | |
| 12 | -9 | 7 | -9 | -9.86 | 306.42 | -16.58 | 130.56 | 0.3717 | 873.4 | 999999 | |
| 4 | -9 | 2 | -9 | -10.88 | 306.28 | -16.72 | 132.39 | 0.3842 | -1552.7 | 999999 | |
| 16 | -9 | 9 | -9 | -10.81 | 305.95 | -17.06 | 131.68 | 0.3874 | -1486.9 | 999999 | |
| -12 | -9 | -12 | -9 | -10.78 | 305.62 | -17.39 | 131.06 | 0.3911 | 999999 | 999999 | |
| 0 | 7 | 0 | 4 | -10.95 | 305.18 | -17.83 | 130.71 | 0.3982 | -589.0 | -631.4 | |
| 0 | 6 | 0 | 3 | -10.92 | 303.14 | -19.87 | 127.62 | 0.4232 | 930.0 | 706.8 | |
| 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. | |