SOHO MDI 2000-07-16 11:41:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68 | 335 | 35 | 167 | 2.90 | 271.33 | -9.91 | 100.23 | 0.1755 | -863.4 | -255.7 | |
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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 | 1.62 | 278.07 | -3.18 | 132.64 | 0.0756 | 728.0 | 644.0 | |
| 0 | 5 | 0 | 3 | 1.34 | 277.48 | -3.77 | 130.34 | 0.0866 | 751.0 | 623.4 | |
| 3 | 12 | 2 | 6 | 2.64 | 276.84 | -4.41 | 113.29 | 0.0840 | 1144.6 | 761.9 | |
| 0 | 5 | 0 | 2 | 3.59 | 276.52 | -4.73 | 101.33 | 0.0843 | 714.0 | 599.0 | |
| 0 | 6 | 0 | 3 | 2.87 | 275.65 | -5.60 | 106.52 | 0.1021 | 690.0 | 486.9 | |
| 5 | 75 | 2 | 37 | 3.58 | 275.60 | -5.64 | 99.53 | 0.1000 | 1400.7 | 844.0 | |
| 7 | -6 | 4 | -6 | 3.34 | 275.17 | -6.08 | 101.04 | 0.1082 | 1240.3 | 999999 | |
| 0 | 4 | 0 | 2 | 3.54 | 271.49 | -9.76 | 95.56 | 0.1708 | -771.0 | -661.2 | |
| 26 | 174 | 13 | 88 | 3.04 | 269.44 | -11.81 | 96.91 | 0.2069 | -1874.0 | -736.1 | |
| 0 | 13 | 0 | 6 | 1.45 | 269.41 | -11.84 | 104.32 | 0.2127 | -1087.0 | -880.1 | |
| 7 | -9 | 4 | -9 | 2.75 | 269.20 | -12.05 | 98.08 | 0.2116 | -1247.8 | 999999 | |
| 9 | -9 | 4 | -9 | 3.70 | 269.10 | -12.14 | 93.55 | 0.2113 | -1446.1 | 999999 | |
| 5 | 29 | 3 | 15 | 1.56 | 268.76 | -12.49 | 103.10 | 0.2229 | -1133.8 | -769.6 | |
| 6 | -13 | 3 | -13 | 1.16 | 268.64 | -12.61 | 104.69 | 0.2266 | -1017.1 | 999999 | |
| 0 | 7 | 0 | 3 | 2.74 | 268.59 | -12.66 | 97.70 | 0.2219 | -466.0 | -465.8 | |
| 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. | |