SOHO MDI 2000-11-03 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 105 | 693 | 52 | 349 | 2.35 | 271.66 | 10.03 | 261.08 | 0.1766 | 1846.4 | 674.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38 | 618 | 19 | 312 | 2.06 | 273.12 | 11.49 | 260.82 | 0.2027 | 1947.9 | 767.5 | |
| 13 | -1 | 6 | -1 | 1.95 | 272.61 | 10.98 | 259.82 | 0.1944 | 2093.5 | 999999 | |
| 5 | -1 | 2 | -1 | 3.18 | 272.46 | 10.84 | 266.13 | 0.1890 | 1370.7 | 999999 | |
| 6 | -1 | 3 | -1 | 2.42 | 272.34 | 10.71 | 261.99 | 0.1884 | 1601.9 | 999999 | |
| 7 | -1 | 4 | -1 | 2.11 | 272.06 | 10.44 | 260.13 | 0.1846 | 1560.1 | 999999 | |
| 30 | -1 | 15 | -1 | 2.88 | 272.03 | 10.40 | 264.28 | 0.1821 | 2086.4 | 999999 | |
| 0 | 7 | 0 | 3 | -0.43 | 271.78 | 10.15 | 246.73 | 0.1928 | 758.0 | 657.1 | |
| 6 | -1 | 3 | -1 | 2.93 | 271.52 | 9.89 | 264.21 | 0.1733 | 1682.6 | 999999 | |
| 0 | 14 | 0 | 7 | 0.16 | 270.92 | 9.30 | 247.86 | 0.1752 | 875.0 | 728.8 | |
| 0 | 3 | 0 | 2 | 5.23 | 268.08 | 6.45 | 281.22 | 0.1146 | -487.0 | -443.0 | |
| 0 | 10 | 0 | 5 | -2.43 | 267.36 | 5.73 | 221.85 | 0.1502 | 614.0 | 500.7 | |
| 0 | 4 | 0 | 2 | 5.63 | 264.44 | 2.81 | 300.66 | 0.0570 | -638.0 | -573.6 | |
| 0 | 6 | 0 | 3 | 2.94 | 263.58 | 1.95 | 242.00 | 0.0387 | -600.0 | -529.5 | |
| 0 | 19 | 0 | 9 | 3.98 | 262.38 | 0.76 | 270.20 | 0.0132 | -821.0 | -674.2 | |
| 0 | 4 | 0 | 2 | 2.15 | 254.90 | -6.73 | 105.06 | 0.1218 | -684.0 | -606.6 | |
| 0 | 8 | 0 | 4 | 3.06 | 253.34 | -8.28 | 96.11 | 0.1454 | -837.0 | -693.7 | |
| 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. | |