SOHO MDI 2000-11-07 09:55:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 487 | 35 | 319 | 19.15 | 255.21 | 38.57 | 295.70 | 0.6548 | 1211.1 | 353.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 404 | 6 | 269 | 18.83 | 257.08 | 40.44 | 294.27 | 0.6758 | 846.6 | 500.4 | |
| 44 | -1 | 29 | -1 | 19.10 | 256.36 | 39.72 | 294.94 | 0.6682 | 1420.2 | 999999 | |
| 0 | 8 | 0 | 5 | 17.80 | 255.79 | 39.15 | 293.28 | 0.6567 | 1193.0 | 955.5 | |
| 0 | 3 | 0 | 2 | 13.66 | 254.45 | 37.81 | 287.46 | 0.6267 | -334.0 | -460.6 | |
| 0 | 5 | 0 | 3 | 17.54 | 255.26 | 38.61 | 293.11 | 0.6493 | 647.0 | 582.6 | |
| 0 | 4 | 0 | 3 | 17.26 | 253.25 | 36.61 | 293.52 | 0.6234 | -573.0 | -495.4 | |
| 0 | 3 | 0 | 2 | 18.50 | 253.20 | 36.55 | 295.44 | 0.6277 | -488.0 | -370.2 | |
| 0 | 5 | 0 | 3 | 18.31 | 250.52 | 33.87 | 296.51 | 0.5935 | -650.0 | -494.2 | |
| 0 | 4 | 0 | 2 | 20.37 | 246.40 | 29.76 | 302.47 | 0.5537 | -750.0 | -711.5 | |
| 0 | 17 | 0 | 10 | 20.22 | 245.95 | 29.30 | 302.57 | 0.5471 | -861.0 | -759.1 | |
| 0 | 14 | 0 | 8 | 20.03 | 245.53 | 28.89 | 302.58 | 0.5408 | -913.0 | -869.8 | |
| 0 | 9 | 0 | 5 | 20.34 | 244.75 | 28.11 | 303.71 | 0.5332 | -724.0 | -648.3 | |
| 0 | 5 | 0 | 3 | 22.75 | 243.99 | 27.35 | 308.28 | 0.5418 | -867.0 | -725.7 | |
| 0 | 6 | 0 | 4 | 24.23 | 243.81 | 27.16 | 310.74 | 0.5516 | -529.0 | -570.2 | |
| 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. | |