SOHO MDI 2000-11-04 17:03:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91 | 591 | 48 | 311 | 2.39 | 272.06 | 19.80 | 266.11 | 0.3409 | 1702.6 | 644.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 11 | 0 | 6 | 4.88 | 273.24 | 20.99 | 273.46 | 0.3591 | 139.0 | 304.9 | |
| 40 | 530 | 21 | 280 | 2.00 | 273.05 | 20.80 | 265.36 | 0.3576 | 1788.6 | 696.5 | |
| 5 | -2 | 3 | -2 | 3.24 | 272.58 | 20.32 | 268.79 | 0.3484 | 1163.8 | 999999 | |
| 6 | -2 | 3 | -2 | 2.25 | 272.40 | 20.14 | 265.88 | 0.3465 | 1656.1 | 999999 | |
| 34 | -2 | 18 | -2 | 2.79 | 272.16 | 19.90 | 267.41 | 0.3419 | 1913.2 | 999999 | |
| 6 | -2 | 3 | -2 | 1.99 | 272.07 | 19.81 | 265.03 | 0.3415 | 1556.5 | 999999 | |
| 0 | 5 | 0 | 2 | 4.34 | 271.99 | 19.73 | 271.95 | 0.3384 | 673.0 | 704.5 | |
| 0 | 9 | 0 | 4 | 1.42 | 271.61 | 19.36 | 263.20 | 0.3352 | 1059.0 | 907.9 | |
| 0 | 3 | 0 | 2 | 0.84 | 269.82 | 17.57 | 260.54 | 0.3073 | 762.0 | 637.2 | |
| 0 | 5 | 0 | 3 | -2.14 | 268.51 | 16.25 | 249.84 | 0.2992 | 432.0 | 298.1 | |
| 0 | 3 | 0 | 2 | 3.80 | 265.94 | 13.68 | 270.02 | 0.2371 | 536.0 | 474.2 | |
| 0 | 3 | 0 | 1 | 4.61 | 262.91 | 10.65 | 274.19 | 0.1856 | -659.0 | -569.5 | |
| 0 | 3 | 0 | 2 | 2.43 | 262.14 | 9.89 | 261.78 | 0.1741 | -832.0 | -649.4 | |
| 0 | 6 | 0 | 3 | 1.43 | 262.06 | 9.80 | 256.07 | 0.1762 | -528.0 | -480.7 | |
| 0 | 5 | 0 | 2 | 0.74 | 261.98 | 9.72 | 252.17 | 0.1782 | 785.0 | 553.4 | |
| 0 | 8 | 0 | 4 | 3.21 | 260.67 | 8.41 | 265.56 | 0.1471 | -646.0 | -605.2 | |
| 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. | |