SOHO MDI 2000-11-03 16:29:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 117 | 697 | 57 | 347 | 2.55 | 271.59 | 5.85 | 256.12 | 0.1052 | 1858.4 | 685.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39 | 628 | 19 | 313 | 2.06 | 273.10 | 7.36 | 255.34 | 0.1329 | 2008.5 | 766.3 | |
| 18 | -1 | 9 | -1 | 1.95 | 272.60 | 6.85 | 253.43 | 0.1250 | 2034.3 | 999999 | |
| 6 | -1 | 3 | -1 | 3.19 | 272.41 | 6.67 | 263.11 | 0.1173 | 1392.8 | 999999 | |
| 5 | -1 | 2 | -1 | 2.57 | 272.33 | 6.59 | 257.81 | 0.1178 | 1512.8 | 999999 | |
| 6 | -1 | 3 | -1 | 2.19 | 272.02 | 6.27 | 253.92 | 0.1142 | 1597.8 | 999999 | |
| 43 | -1 | 21 | -1 | 2.96 | 271.98 | 6.24 | 260.56 | 0.1105 | 1962.9 | 999999 | |
| 0 | 6 | 0 | 3 | 0.54 | 270.35 | 4.61 | 233.09 | 0.1009 | 760.0 | 622.5 | |
| 0 | 19 | 0 | 9 | 3.37 | 266.23 | 0.49 | 216.88 | 0.0142 | 700.0 | 576.4 | |
| 0 | 4 | 0 | 2 | 2.40 | 265.08 | -0.67 | 157.50 | 0.0306 | 609.0 | 516.4 | |
| 0 | 4 | 0 | 2 | 2.71 | 264.19 | -1.55 | 130.02 | 0.0355 | -570.0 | -440.3 | |
| 0 | 12 | 0 | 6 | 3.09 | 263.38 | -2.36 | 111.26 | 0.0444 | -799.0 | -611.5 | |
| 0 | 4 | 0 | 2 | 4.44 | 263.26 | -2.48 | 80.19 | 0.0440 | -740.0 | -605.7 | |
| 0 | 4 | 0 | 2 | 5.13 | 261.63 | -4.11 | 74.68 | 0.0744 | -690.0 | -540.3 | |
| 0 | 10 | 0 | 5 | 4.22 | 258.19 | -7.56 | 88.20 | 0.1318 | -609.0 | -320.7 | |
| 0 | 6 | 0 | 3 | 5.12 | 255.95 | -9.79 | 83.19 | 0.1714 | -739.0 | -567.6 | |
| 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. | |