SOHO MDI 2000-11-11 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58 | 429 | 30 | 225 | -12.53 | 176.77 | 10.00 | 212.03 | 0.3208 | 1530.0 | 450.4 | |
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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 | -16.19 | 179.67 | 12.91 | 213.00 | 0.3957 | -720.0 | -626.0 | |
| 0 | 14 | 0 | 7 | -13.03 | 179.20 | 12.44 | 217.04 | 0.3499 | -1125.0 | -864.6 | |
| 0 | 11 | 0 | 6 | -12.55 | 178.61 | 11.85 | 216.59 | 0.3378 | -118.0 | -135.6 | |
| 10 | 326 | 5 | 171 | -13.25 | 177.56 | 10.80 | 212.89 | 0.3374 | 1303.0 | 700.3 | |
| 18 | -4 | 9 | -4 | -12.21 | 177.40 | 10.63 | 214.28 | 0.3217 | 1918.9 | 999999 | |
| 15 | -4 | 8 | -4 | -12.85 | 177.10 | 10.34 | 212.44 | 0.3278 | 1522.0 | 999999 | |
| 15 | -4 | 8 | -4 | -12.69 | 176.74 | 9.97 | 211.79 | 0.3222 | 1799.7 | 999999 | |
| 0 | 8 | 0 | 4 | -13.56 | 175.89 | 9.13 | 208.22 | 0.3277 | 727.0 | 568.8 | |
| 0 | 6 | 0 | 3 | -12.99 | 175.63 | 8.87 | 208.38 | 0.3175 | 973.0 | 763.9 | |
| 0 | 5 | 0 | 3 | -13.43 | 175.49 | 8.72 | 207.33 | 0.3227 | 810.0 | 677.3 | |
| 0 | 5 | 0 | 3 | -9.97 | 175.22 | 8.46 | 212.53 | 0.2706 | -528.0 | -484.0 | |
| 0 | 12 | 0 | 6 | -8.63 | 174.64 | 7.87 | 213.54 | 0.2463 | -1041.0 | -782.3 | |
| 0 | 5 | 0 | 3 | -9.65 | 174.07 | 7.31 | 209.49 | 0.2559 | -770.0 | -675.0 | |
| 0 | 6 | 0 | 3 | -8.51 | 174.05 | 7.28 | 211.79 | 0.2391 | -627.0 | -466.4 | |
| 0 | 20 | 0 | 10 | -13.17 | 172.89 | 6.13 | 200.28 | 0.3013 | -843.0 | -519.1 | |
| 0 | 8 | 0 | 4 | -12.57 | 171.89 | 5.13 | 197.82 | 0.2863 | -672.0 | -530.8 | |
| 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. | |