SOHO MDI 2000-07-18 13:01:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76 | 459 | 47 | 285 | 19.04 | 289.35 | 35.32 | 295.67 | 0.6080 | 302.3 | 172.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19 | 273 | 12 | 174 | 18.40 | 291.40 | 37.37 | 293.65 | 0.6310 | 1426.5 | 622.0 | |
| 12 | -1 | 8 | -1 | 19.30 | 291.32 | 37.29 | 295.06 | 0.6335 | 1134.4 | 999999 | |
| 5 | -1 | 3 | -1 | 18.13 | 291.02 | 36.99 | 293.39 | 0.6252 | 1517.6 | 999999 | |
| 8 | -1 | 5 | -1 | 18.74 | 291.02 | 36.98 | 294.34 | 0.6275 | 1673.1 | 999999 | |
| 0 | 4 | 0 | 3 | 25.88 | 292.31 | 38.28 | 304.04 | 0.6749 | 578.0 | 538.8 | |
| 0 | 15 | 0 | 9 | 19.01 | 289.78 | 35.75 | 295.30 | 0.6132 | 914.0 | 669.6 | |
| 4 | 9 | 2 | 5 | 18.93 | 287.93 | 33.89 | 296.09 | 0.5896 | -622.8 | -444.1 | |
| 0 | 5 | 0 | 3 | 18.74 | 286.49 | 32.45 | 296.58 | 0.5703 | -462.0 | -404.9 | |
| 5 | 17 | 3 | 11 | 21.00 | 286.76 | 32.72 | 300.07 | 0.5854 | -819.1 | -582.8 | |
| 2 | -9 | 1 | -9 | 21.25 | 286.72 | 32.69 | 300.49 | 0.5863 | -569.4 | 999999 | |
| 21 | 108 | 13 | 64 | 18.98 | 285.70 | 31.66 | 297.43 | 0.5614 | -1532.8 | -756.3 | |
| 0 | 6 | 0 | 3 | 19.98 | 285.47 | 31.44 | 299.22 | 0.5638 | -580.0 | -538.4 | |
| 0 | 12 | 0 | 7 | 20.72 | 285.54 | 31.51 | 300.39 | 0.5688 | -665.0 | -518.7 | |
| 0 | 5 | 0 | 3 | 20.56 | 284.47 | 30.43 | 300.84 | 0.5545 | -785.0 | -693.5 | |
| 0 | 5 | 0 | 3 | 21.09 | 284.49 | 30.45 | 301.71 | 0.5580 | -401.0 | -382.6 | |
| 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. | |