SOHO MDI 2000-11-04 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 86 | 588 | 47 | 311 | 2.35 | 271.66 | 20.57 | 266.24 | 0.3532 | 1648.8 | 599.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38 | 515 | 21 | 274 | 2.00 | 273.08 | 21.99 | 265.71 | 0.3770 | 1749.2 | 695.9 | |
| 5 | -1 | 3 | -1 | 3.25 | 272.56 | 21.48 | 268.96 | 0.3672 | 1179.6 | 999999 | |
| 19 | -1 | 10 | -1 | 2.21 | 272.38 | 21.29 | 266.10 | 0.3653 | 1529.4 | 999999 | |
| 24 | -1 | 13 | -1 | 2.76 | 272.22 | 21.14 | 267.56 | 0.3621 | 1978.3 | 999999 | |
| 0 | 5 | 0 | 3 | 4.26 | 272.09 | 21.01 | 271.73 | 0.3593 | 671.0 | 641.4 | |
| -3 | -1 | -3 | -1 | 1.99 | 271.92 | 20.84 | 265.37 | 0.3582 | 999999 | 999999 | |
| 0 | 6 | 0 | 3 | 1.42 | 271.63 | 20.54 | 263.68 | 0.3545 | 1103.0 | 942.9 | |
| 0 | 4 | 0 | 2 | 0.89 | 269.78 | 18.70 | 261.32 | 0.3257 | 811.0 | 710.7 | |
| 0 | 6 | 0 | 3 | 2.47 | 265.86 | 14.77 | 264.90 | 0.2569 | 827.0 | 747.1 | |
| 0 | 4 | 0 | 2 | 0.34 | 263.71 | 12.62 | 254.57 | 0.2277 | 749.0 | 630.7 | |
| 0 | 4 | 0 | 2 | 4.59 | 262.88 | 11.79 | 273.79 | 0.2051 | -515.0 | -545.8 | |
| 0 | 14 | 0 | 7 | 3.25 | 262.66 | 11.58 | 267.15 | 0.2016 | -856.0 | -606.3 | |
| 0 | 3 | 0 | 1 | 1.52 | 262.37 | 11.29 | 258.40 | 0.2007 | -170.0 | -223.9 | |
| 0 | 13 | 0 | 7 | 2.94 | 262.27 | 11.18 | 265.47 | 0.1952 | -1001.0 | -899.2 | |
| 0 | 5 | 0 | 3 | 2.44 | 262.18 | 11.10 | 262.86 | 0.1947 | -927.0 | -733.1 | |
| 0 | 5 | 0 | 2 | 0.75 | 262.06 | 10.97 | 254.27 | 0.1986 | 797.0 | 632.3 | |
| 0 | 4 | 0 | 2 | 3.23 | 260.78 | 9.70 | 266.38 | 0.1693 | -666.0 | -643.3 | |
| 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. | |