SOHO MDI 2000-11-03 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99 | 683 | 50 | 343 | 2.37 | 271.90 | 8.52 | 259.40 | 0.1509 | 1879.7 | 745.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36 | 625 | 18 | 313 | 2.06 | 273.08 | 9.69 | 258.96 | 0.1722 | 1981.6 | 789.1 | |
| 12 | -1 | 6 | -1 | 1.99 | 272.61 | 9.22 | 257.96 | 0.1646 | 2085.3 | 999999 | |
| 5 | -1 | 3 | -1 | 3.18 | 272.38 | 9.00 | 265.11 | 0.1575 | 1452.6 | 999999 | |
| 7 | -1 | 4 | -1 | 2.15 | 272.02 | 8.64 | 258.16 | 0.1541 | 1542.0 | 999999 | |
| 32 | -1 | 16 | -1 | 2.92 | 271.99 | 8.61 | 263.11 | 0.1513 | 2111.7 | 999999 | |
| 0 | 6 | 0 | 3 | -0.28 | 271.75 | 8.36 | 243.10 | 0.1638 | 907.0 | 683.5 | |
| 7 | -1 | 3 | -1 | 2.85 | 271.48 | 8.10 | 262.15 | 0.1427 | 1619.6 | 999999 | |
| 0 | 11 | 0 | 5 | 0.23 | 270.97 | 7.59 | 243.77 | 0.1479 | 969.0 | 741.8 | |
| 0 | 5 | 0 | 3 | 0.66 | 270.23 | 6.85 | 244.20 | 0.1331 | 655.0 | 511.0 | |
| 0 | 8 | 0 | 4 | -2.29 | 266.95 | 3.57 | 209.63 | 0.1264 | 726.0 | 690.8 | |
| 0 | 6 | 0 | 3 | 3.38 | 266.38 | 2.99 | 258.43 | 0.0535 | 863.0 | 719.6 | |
| 0 | 5 | 0 | 3 | 5.04 | 265.26 | 1.88 | 299.13 | 0.0376 | -846.0 | -641.0 | |
| 0 | 6 | 0 | 3 | 1.96 | 265.14 | 1.76 | 220.79 | 0.0471 | 685.0 | 566.9 | |
| 0 | 4 | 0 | 2 | 2.62 | 264.26 | 0.87 | 212.25 | 0.0286 | -526.0 | -366.9 | |
| 0 | 4 | 0 | 2 | 2.07 | 254.83 | -8.55 | 102.46 | 0.1529 | -923.0 | -813.4 | |
| 0 | 3 | 0 | 2 | 5.64 | 253.66 | -9.72 | 80.01 | 0.1715 | -538.0 | -491.7 | |
| 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. | |