SOHO MDI 2000-07-10 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75 | 513 | 43 | 293 | -19.44 | 16.70 | 17.50 | 215.30 | 0.4920 | -150.9 | -32.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 165 | 4 | 96 | -18.65 | 21.59 | 22.39 | 223.55 | 0.5259 | -1357.6 | -668.7 | |
| 8 | -1 | 5 | -1 | -18.81 | 21.16 | 21.96 | 222.79 | 0.5232 | -1376.9 | 999999 | |
| 9 | -1 | 5 | -1 | -18.33 | 21.05 | 21.85 | 223.31 | 0.5171 | -1743.6 | 999999 | |
| 0 | 3 | 0 | 2 | -16.45 | 20.59 | 21.39 | 225.45 | 0.4929 | 385.0 | 287.0 | |
| 11 | 26 | 6 | 15 | -17.71 | 20.25 | 21.06 | 223.15 | 0.5024 | -1450.3 | -996.2 | |
| 0 | 14 | 0 | 8 | -18.57 | 20.27 | 21.07 | 221.97 | 0.5117 | -1025.0 | -914.2 | |
| 0 | 5 | 0 | 3 | -18.77 | 19.94 | 20.74 | 221.25 | 0.5106 | -824.0 | -640.6 | |
| 0 | 3 | 0 | 2 | -17.10 | 19.47 | 20.27 | 222.98 | 0.4877 | -763.0 | -667.3 | |
| 0 | 7 | 0 | 4 | -17.17 | 19.04 | 19.84 | 222.26 | 0.4841 | -1218.0 | -930.7 | |
| 0 | 3 | 0 | 2 | -17.89 | 18.94 | 19.74 | 221.10 | 0.4910 | -510.0 | -468.3 | |
| 0 | 7 | 0 | 4 | -19.72 | 18.23 | 19.03 | 217.62 | 0.5049 | -1118.0 | -885.5 | |
| 6 | 34 | 4 | 19 | -18.72 | 17.89 | 18.69 | 218.44 | 0.4902 | 1081.9 | 885.4 | |
| 0 | 5 | 0 | 3 | -19.33 | 17.96 | 18.76 | 217.75 | 0.4978 | -927.0 | -777.8 | |
| 3 | -12 | 2 | -12 | -18.21 | 17.70 | 18.50 | 218.86 | 0.4824 | 1307.2 | 999999 | |
| 0 | 9 | 0 | 5 | -19.93 | 17.77 | 18.57 | 216.69 | 0.5030 | -980.0 | -918.0 | |
| 0 | 5 | 0 | 3 | -20.09 | 17.43 | 18.23 | 216.00 | 0.5020 | -1136.0 | -878.2 | |
| 0 | 5 | 0 | 3 | -20.12 | 16.68 | 17.48 | 214.84 | 0.4957 | -413.0 | -680.4 | |
| 0 | 4 | 0 | 2 | -20.18 | 15.19 | 15.99 | 212.46 | 0.4838 | -657.0 | -571.1 | |
| 3 | 10 | 2 | 6 | -20.82 | 14.82 | 15.62 | 211.11 | 0.4890 | -1064.7 | -708.3 | |
| 0 | 5 | 0 | 3 | -17.32 | 13.92 | 14.72 | 213.91 | 0.4367 | -1003.0 | -755.3 | |
| 6 | 48 | 3 | 27 | -20.49 | 13.25 | 14.05 | 208.90 | 0.4726 | 945.9 | 418.7 | |
| 5 | -21 | 3 | -21 | -20.92 | 12.90 | 13.70 | 207.83 | 0.4758 | 955.2 | 999999 | |
| 0 | 4 | 0 | 2 | -17.04 | 12.57 | 13.38 | 211.80 | 0.4215 | -916.0 | -681.5 | |
| 0 | 12 | 0 | 6 | -20.64 | 12.18 | 12.98 | 206.87 | 0.4670 | 1356.0 | 940.4 | |
| 0 | 15 | 0 | 8 | -21.08 | 12.17 | 12.97 | 206.41 | 0.4728 | 1080.0 | 711.3 | |
| 0 | 5 | 0 | 3 | -21.65 | 12.09 | 12.89 | 205.71 | 0.4800 | -331.0 | -315.4 | |
| 0 | 4 | 0 | 2 | -19.99 | 11.95 | 12.75 | 207.15 | 0.4564 | 345.0 | 476.8 | |
| 0 | 5 | 0 | 3 | -20.55 | 11.78 | 12.58 | 206.26 | 0.4629 | 860.0 | 873.8 | |
| 5 | 19 | 3 | 11 | -20.94 | 11.72 | 12.53 | 205.77 | 0.4679 | 1186.5 | 909.9 | |
| 3 | 91 | 2 | 51 | -20.80 | 10.89 | 11.69 | 204.40 | 0.4604 | 1560.8 | 1105.0 | |
| 8 | -30 | 4 | -30 | -20.79 | 10.50 | 11.30 | 203.69 | 0.4579 | 1758.4 | 999999 | |
| 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. | |