SOHO MDI 2000-11-02 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83 | 466 | 53 | 297 | -22.97 | 304.95 | 28.39 | 224.34 | 0.6281 | -903.6 | -473.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15 | 93 | 10 | 60 | -22.49 | 307.53 | 30.97 | 227.33 | 0.6489 | -1303.4 | -625.0 | |
| 8 | 203 | 5 | 131 | -23.90 | 305.94 | 29.38 | 224.21 | 0.6456 | -1187.7 | -468.0 | |
| 7 | -2 | 4 | -2 | -24.15 | 305.71 | 29.15 | 223.70 | 0.6457 | -997.1 | 999999 | |
| 6 | -2 | 4 | -2 | -23.80 | 305.48 | 28.92 | 223.91 | 0.6404 | -1376.4 | 999999 | |
| 13 | -2 | 9 | -2 | -23.69 | 305.07 | 28.51 | 223.64 | 0.6357 | -1294.2 | 999999 | |
| 0 | 3 | 0 | 2 | -23.08 | 304.83 | 28.27 | 224.14 | 0.6280 | -648.0 | -620.8 | |
| 0 | 14 | 0 | 9 | -25.00 | 304.86 | 28.30 | 221.92 | 0.6455 | -592.0 | -389.0 | |
| 0 | 5 | 0 | 3 | -21.71 | 303.78 | 27.22 | 224.79 | 0.6055 | 192.0 | 181.1 | |
| 0 | 4 | 0 | 2 | -20.13 | 303.42 | 26.86 | 226.46 | 0.5875 | -774.0 | -681.1 | |
| 5 | 39 | 3 | 25 | -22.65 | 303.70 | 27.14 | 223.54 | 0.6133 | -1185.6 | -843.0 | |
| 18 | 64 | 11 | 39 | -20.75 | 302.99 | 26.43 | 225.20 | 0.5888 | -1167.8 | -726.3 | |
| 0 | 6 | 0 | 4 | -25.40 | 303.71 | 27.15 | 220.35 | 0.6391 | 383.0 | 207.5 | |
| 0 | 3 | 0 | 2 | -25.42 | 303.24 | 26.68 | 219.84 | 0.6352 | 459.0 | 426.6 | |
| 0 | 3 | 0 | 2 | -20.71 | 301.88 | 25.32 | 224.07 | 0.5774 | -606.0 | -505.4 | |
| 0 | 3 | 0 | 2 | -22.42 | 300.51 | 23.94 | 220.40 | 0.5811 | 561.0 | 567.8 | |
| 11 | 26 | 7 | 16 | -22.40 | 299.77 | 23.21 | 219.58 | 0.5742 | 1054.7 | 709.8 | |
| 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. | |