SOHO MDI 2000-01-27 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62 | 503 | 34 | 275 | -29.23 | 22.59 | 2.98 | 186.57 | 0.4069 | -1603.8 | -385.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -27.56 | 23.81 | 4.20 | 189.85 | 0.3814 | -301.0 | -331.9 | |
| 59 | 394 | 32 | 213 | -28.97 | 23.69 | 4.08 | 188.92 | 0.4035 | -1947.7 | -675.6 | |
| 0 | 5 | 0 | 3 | -30.03 | 22.80 | 3.19 | 186.65 | 0.4182 | -608.0 | -554.6 | |
| 0 | 4 | 0 | 2 | -27.32 | 22.50 | 2.90 | 186.92 | 0.3745 | 315.0 | 144.5 | |
| 0 | 3 | 0 | 2 | -30.28 | 21.83 | 2.23 | 184.59 | 0.4208 | 567.0 | 441.6 | |
| 0 | 12 | 0 | 6 | -29.91 | 20.67 | 1.07 | 182.25 | 0.4137 | 715.0 | 602.1 | |
| 0 | 4 | 0 | 2 | -29.45 | 20.49 | 0.89 | 181.91 | 0.4062 | 766.0 | 648.6 | |
| 0 | 3 | 0 | 2 | -29.99 | 20.23 | 0.63 | 181.31 | 0.4149 | 608.0 | 493.6 | |
| 0 | 20 | 0 | 11 | -29.74 | 19.70 | 0.09 | 180.20 | 0.4107 | 751.0 | 710.0 | |
| 3 | 8 | 2 | 5 | -31.52 | 18.49 | -1.12 | 177.82 | 0.4392 | 817.5 | 591.3 | |
| 0 | 5 | 0 | 3 | -30.33 | 17.93 | -1.68 | 176.54 | 0.4209 | 677.0 | 733.0 | |
| 0 | 10 | 0 | 6 | -30.28 | 17.04 | -2.57 | 174.71 | 0.4212 | 925.0 | 918.7 | |
| 0 | 19 | 0 | 10 | -30.54 | 16.72 | -2.89 | 174.13 | 0.4257 | 1090.0 | 843.7 | |
| 0 | 5 | 0 | 3 | -30.57 | 16.05 | -3.56 | 172.79 | 0.4275 | 1030.0 | 902.3 | |
| 0 | 3 | 0 | 2 | -30.78 | 15.37 | -4.23 | 171.53 | 0.4322 | 938.0 | 757.0 | |
| 0 | 5 | 0 | 3 | -31.20 | 14.77 | -4.84 | 170.53 | 0.4402 | 877.0 | 673.8 | |
| 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. | |