SOHO MDI 2000-11-05 10:28:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78 | 437 | 46 | 249 | 2.42 | 272.10 | 29.40 | 268.17 | 0.4925 | 1531.0 | 643.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17 | 382 | 10 | 219 | 2.22 | 273.47 | 30.78 | 267.90 | 0.5138 | 1408.4 | 699.4 | |
| 22 | -1 | 13 | -1 | 2.04 | 273.07 | 30.37 | 267.50 | 0.5078 | 1566.4 | 999999 | |
| -2 | -1 | -2 | -1 | 1.93 | 272.75 | 30.06 | 267.24 | 0.5032 | 999999 | 999999 | |
| 0 | 4 | 0 | 2 | 3.90 | 272.76 | 30.07 | 271.16 | 0.5021 | 657.0 | 645.1 | |
| 4 | -1 | 3 | -1 | 3.24 | 272.70 | 30.00 | 269.85 | 0.5013 | 1009.4 | 999999 | |
| 6 | -1 | 4 | -1 | 2.21 | 272.53 | 29.84 | 267.77 | 0.4996 | 1529.1 | 999999 | |
| 25 | -1 | 14 | -1 | 2.68 | 272.32 | 29.63 | 268.68 | 0.4960 | 1873.3 | 999999 | |
| 4 | -1 | 2 | -1 | 3.14 | 272.34 | 29.64 | 269.62 | 0.4959 | 1526.8 | 999999 | |
| 0 | 5 | 0 | 3 | 1.55 | 271.59 | 28.90 | 266.27 | 0.4861 | 498.0 | 515.7 | |
| 0 | 7 | 0 | 4 | 3.51 | 271.51 | 28.81 | 270.33 | 0.4831 | 829.0 | 710.2 | |
| 0 | 3 | 0 | 2 | 0.83 | 271.23 | 28.54 | 264.71 | 0.4818 | 438.0 | 399.3 | |
| 0 | 5 | 0 | 3 | 0.86 | 270.23 | 27.54 | 264.53 | 0.4663 | 720.0 | 577.6 | |
| 0 | 16 | 0 | 8 | 2.53 | 265.82 | 23.13 | 267.46 | 0.3945 | 516.0 | 526.5 | |
| 0 | 5 | 0 | 3 | 2.12 | 263.41 | 20.71 | 265.88 | 0.3559 | -583.0 | -643.8 | |
| 0 | 5 | 0 | 2 | 3.21 | 262.85 | 20.15 | 268.89 | 0.3456 | -723.0 | -781.0 | |
| 0 | 5 | 0 | 3 | 4.75 | 257.10 | 14.41 | 274.19 | 0.2498 | -799.0 | -596.1 | |
| 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. | |