SOHO MDI 2000-11-02 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102 | 488 | 65 | 317 | -23.06 | 305.02 | 30.22 | 225.94 | 0.6464 | -795.9 | -392.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 3 | -17.59 | 310.10 | 35.29 | 237.06 | 0.6586 | 70.0 | 75.8 | |
| 17 | 87 | 11 | 58 | -22.53 | 307.55 | 32.75 | 228.79 | 0.6665 | -1236.7 | -617.3 | |
| 22 | 213 | 14 | 140 | -23.98 | 306.01 | 31.21 | 225.76 | 0.6632 | -1073.7 | -368.0 | |
| -3 | -3 | -3 | -3 | -24.18 | 305.67 | 30.87 | 225.22 | 0.6618 | 999999 | 999999 | |
| 5 | -3 | 3 | -3 | -23.79 | 305.52 | 30.72 | 225.56 | 0.6570 | -1374.4 | 999999 | |
| 15 | -3 | 10 | -3 | -23.68 | 305.10 | 30.30 | 225.31 | 0.6522 | -1278.9 | 999999 | |
| 0 | 5 | 0 | 3 | -23.11 | 304.86 | 30.06 | 225.78 | 0.6451 | -540.0 | -533.5 | |
| 4 | 13 | 2 | 9 | -25.07 | 304.83 | 30.03 | 223.45 | 0.6615 | -452.6 | -345.1 | |
| 2 | 55 | 1 | 35 | -23.09 | 304.27 | 29.47 | 225.27 | 0.6393 | -806.2 | -710.2 | |
| 0 | 5 | 0 | 3 | -21.57 | 303.68 | 28.88 | 226.60 | 0.6205 | 164.0 | 178.2 | |
| 16 | 58 | 10 | 36 | -20.62 | 303.20 | 28.40 | 227.36 | 0.6074 | -1144.2 | -700.6 | |
| 4 | -9 | 3 | -9 | -22.72 | 303.66 | 28.86 | 225.15 | 0.6303 | -1129.9 | 999999 | |
| 3 | 17 | 2 | 11 | -25.51 | 303.53 | 28.73 | 221.75 | 0.6537 | 471.7 | 408.5 | |
| 3 | -13 | 2 | -13 | -25.50 | 303.23 | 28.43 | 221.49 | 0.6510 | 769.3 | 999999 | |
| 11 | 31 | 7 | 19 | -22.37 | 299.75 | 24.94 | 221.59 | 0.5898 | 1065.8 | 660.1 | |
| 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. | |