SOHO MDI 2000-11-03 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68 | 509 | 35 | 260 | -10.28 | 277.35 | 5.18 | 200.32 | 0.2755 | -1033.1 | -439.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 2 | -11.81 | 281.58 | 9.41 | 210.43 | 0.3176 | -614.0 | -516.8 | |
| 41 | 315 | 21 | 162 | -9.37 | 280.01 | 7.84 | 210.16 | 0.2691 | -2032.0 | -691.1 | |
| 10 | 57 | 5 | 29 | -9.87 | 278.37 | 6.20 | 203.87 | 0.2641 | -1464.5 | -733.8 | |
| 0 | 4 | 0 | 2 | -7.84 | 277.20 | 5.03 | 202.86 | 0.2247 | -869.0 | -833.8 | |
| 0 | 6 | 0 | 3 | -8.08 | 277.01 | 4.84 | 201.68 | 0.2272 | -915.0 | -742.3 | |
| 0 | 4 | 0 | 2 | -8.63 | 276.82 | 4.65 | 200.07 | 0.2348 | -602.0 | -578.4 | |
| 0 | 3 | 0 | 1 | -14.25 | 275.05 | 2.88 | 188.80 | 0.3194 | -827.0 | -730.5 | |
| 0 | 7 | 0 | 4 | -10.84 | 274.30 | 2.13 | 188.09 | 0.2609 | -750.0 | -643.7 | |
| 0 | 5 | 0 | 3 | -15.02 | 273.14 | 0.97 | 182.87 | 0.3289 | -525.0 | -351.3 | |
| 0 | 5 | 0 | 2 | -12.84 | 270.61 | -1.56 | 174.78 | 0.2933 | -545.0 | -422.7 | |
| 0 | 6 | 0 | 3 | -13.89 | 270.32 | -1.85 | 174.21 | 0.3112 | -939.0 | -688.0 | |
| 0 | 4 | 0 | 2 | -13.12 | 269.93 | -2.24 | 172.67 | 0.2992 | 505.0 | 361.8 | |
| 0 | 11 | 0 | 6 | -16.58 | 269.78 | -2.39 | 173.53 | 0.3564 | -899.0 | -729.1 | |
| 6 | 34 | 3 | 17 | -11.72 | 269.63 | -2.54 | 170.94 | 0.2766 | 1344.0 | 1031.6 | |
| 0 | 12 | 0 | 6 | -13.44 | 269.49 | -2.67 | 171.42 | 0.3056 | 960.0 | 784.1 | |
| 6 | -14 | 3 | -14 | -11.68 | 269.28 | -2.89 | 169.68 | 0.2770 | 1412.6 | 999999 | |
| 0 | 5 | 0 | 3 | -14.46 | 268.09 | -4.08 | 167.76 | 0.3265 | 769.0 | 702.5 | |
| 5 | 22 | 3 | 11 | -13.53 | 267.55 | -4.62 | 165.48 | 0.3135 | 1205.6 | 972.8 | |
| 0 | 4 | 0 | 2 | -9.61 | 263.69 | -8.48 | 148.32 | 0.2782 | 529.0 | 437.5 | |
| 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. | |