SOHO MDI 2000-11-07 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 385 | 54 | 280 | -12.17 | 175.61 | -44.73 | 110.35 | 0.7360 | 319.8 | 131.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10 | 62 | 7 | 44 | -13.69 | 177.36 | -42.98 | 113.02 | 0.7220 | 914.0 | 280.5 | |
| 7 | 159 | 5 | 114 | -12.52 | 177.56 | -42.78 | 111.55 | 0.7152 | 1267.6 | 684.3 | |
| 0 | 4 | 0 | 3 | -14.48 | 176.90 | -43.44 | 113.84 | 0.7302 | 175.0 | 82.2 | |
| 8 | -2 | 6 | -2 | -12.33 | 177.28 | -43.06 | 111.18 | 0.7178 | 1016.5 | 999999 | |
| 5 | -2 | 4 | -2 | -12.68 | 176.72 | -43.63 | 111.41 | 0.7254 | 1038.3 | 999999 | |
| 14 | -2 | 10 | -2 | -13.17 | 176.44 | -43.90 | 111.94 | 0.7303 | 760.6 | 999999 | |
| 8 | 21 | 5 | 15 | -12.81 | 175.64 | -44.70 | 111.14 | 0.7378 | 501.4 | 148.6 | |
| 0 | 6 | 0 | 4 | -12.09 | 175.57 | -44.77 | 110.19 | 0.7360 | 685.0 | 573.1 | |
| 0 | 12 | 0 | 9 | -10.37 | 174.97 | -45.37 | 107.72 | 0.7373 | -677.0 | -686.9 | |
| 5 | 114 | 4 | 86 | -10.77 | 174.16 | -46.18 | 107.95 | 0.7475 | -972.0 | -584.1 | |
| 3 | -10 | 2 | -10 | -10.68 | 173.49 | -46.85 | 107.62 | 0.7545 | -842.4 | 999999 | |
| 9 | -10 | 7 | -10 | -10.58 | 173.11 | -47.23 | 107.37 | 0.7584 | -1028.2 | 999999 | |
| 5 | -10 | 4 | -10 | -10.81 | 172.42 | -47.92 | 107.44 | 0.7665 | -648.4 | 999999 | |
| 0 | 4 | 0 | 3 | -10.92 | 171.87 | -48.47 | 107.40 | 0.7727 | -459.0 | -368.6 | |
| 0 | 3 | 0 | 2 | -10.06 | 171.69 | -48.65 | 106.26 | 0.7723 | -459.0 | -466.5 | |
| 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. | |