SOHO MDI 2000-11-02 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99 | 674 | 62 | 426 | 19.59 | 250.29 | -35.94 | 63.19 | 0.6209 | 139.0 | -9.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 26.54 | 257.28 | -28.94 | 48.10 | 0.5840 | 469.0 | 452.8 | |
| 13 | 350 | 8 | 213 | 19.28 | 253.21 | -33.01 | 62.16 | 0.5838 | 1414.5 | 571.6 | |
| 36 | -2 | 22 | -2 | 19.06 | 252.87 | -33.35 | 62.70 | 0.5871 | 1473.2 | 999999 | |
| -3 | -2 | -3 | -2 | 18.58 | 252.93 | -33.30 | 63.44 | 0.5840 | 999999 | 999999 | |
| -3 | -2 | -3 | -2 | 18.57 | 252.54 | -33.68 | 63.67 | 0.5888 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | 19.67 | 251.09 | -35.13 | 62.70 | 0.6121 | 316.0 | 182.1 | |
| 13 | 44 | 8 | 28 | 20.27 | 249.97 | -36.25 | 62.36 | 0.6285 | -465.1 | -309.2 | |
| 0 | 8 | 0 | 5 | 18.55 | 249.96 | -36.26 | 65.00 | 0.6210 | -620.0 | -457.7 | |
| 0 | 6 | 0 | 4 | 16.30 | 250.43 | -35.80 | 68.32 | 0.6064 | -346.0 | -247.7 | |
| 0 | 4 | 0 | 2 | 20.88 | 248.98 | -37.24 | 61.96 | 0.6430 | 171.0 | 85.7 | |
| 0 | 9 | 0 | 6 | 18.99 | 249.19 | -37.03 | 64.67 | 0.6324 | 414.0 | 202.0 | |
| 0 | 7 | 0 | 5 | 19.64 | 248.29 | -37.93 | 64.11 | 0.6459 | -592.0 | -485.9 | |
| 0 | 10 | 0 | 6 | 18.87 | 248.19 | -38.03 | 65.29 | 0.6441 | -606.0 | -542.5 | |
| 15 | 216 | 10 | 143 | 20.83 | 246.94 | -39.28 | 62.97 | 0.6667 | -1460.2 | -742.9 | |
| 0 | 3 | 0 | 2 | 18.68 | 247.46 | -38.76 | 65.88 | 0.6522 | -601.0 | -479.1 | |
| 16 | -14 | 10 | -14 | 20.14 | 246.83 | -39.39 | 64.01 | 0.6652 | -1271.0 | 999999 | |
| 6 | -14 | 4 | -14 | 20.81 | 246.47 | -39.76 | 63.21 | 0.6721 | -808.0 | 999999 | |
| 0 | 5 | 0 | 4 | 21.56 | 246.00 | -40.22 | 62.34 | 0.6804 | -607.0 | -515.2 | |
| 0 | 4 | 0 | 3 | 19.03 | 246.36 | -39.86 | 65.80 | 0.6666 | -703.0 | -585.4 | |
| 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. | |