SOHO MDI 2000-11-01 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 126 | 609 | 68 | 331 | -10.55 | 275.53 | -18.60 | 129.40 | 0.4035 | -346.5 | -125.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38 | 259 | 20 | 137 | -9.30 | 279.40 | -14.73 | 132.73 | 0.3431 | -2018.4 | -746.4 | |
| 17 | -1 | 9 | -1 | -9.90 | 279.01 | -15.12 | 133.26 | 0.3544 | -1212.4 | 999999 | |
| 0 | 5 | 0 | 2 | -10.66 | 278.81 | -15.32 | 134.44 | 0.3653 | -613.0 | -445.1 | |
| 8 | 46 | 4 | 25 | -10.04 | 278.27 | -15.86 | 132.19 | 0.3647 | -967.5 | -603.6 | |
| 3 | -4 | 2 | -4 | -9.69 | 277.96 | -16.17 | 130.91 | 0.3648 | -999.0 | 999999 | |
| 0 | 5 | 0 | 3 | -10.86 | 277.00 | -17.13 | 131.66 | 0.3888 | -307.0 | -194.9 | |
| 5 | 13 | 3 | 7 | -9.40 | 276.88 | -17.25 | 128.47 | 0.3753 | -867.4 | -684.0 | |
| 0 | 7 | 0 | 4 | -7.66 | 276.84 | -17.29 | 124.56 | 0.3593 | -830.0 | -725.0 | |
| 5 | 13 | 2 | 7 | -9.01 | 276.33 | -17.80 | 126.78 | 0.3787 | -1010.6 | -833.0 | |
| 15 | 74 | 8 | 40 | -11.16 | 276.08 | -18.05 | 130.76 | 0.4031 | 1260.9 | 877.2 | |
| 3 | -10 | 2 | -10 | -10.53 | 275.87 | -18.26 | 129.20 | 0.3993 | 1389.7 | 999999 | |
| 0 | 12 | 0 | 7 | -10.12 | 274.65 | -19.48 | 126.62 | 0.4107 | -710.0 | -602.9 | |
| 0 | 4 | 0 | 2 | -12.09 | 271.39 | -22.74 | 126.09 | 0.4697 | 944.0 | 681.6 | |
| 0 | 5 | 0 | 3 | -11.71 | 270.74 | -23.39 | 124.66 | 0.4746 | 524.0 | 392.3 | |
| 0 | 9 | 0 | 5 | -16.19 | 269.76 | -24.37 | 130.86 | 0.5260 | -629.0 | -584.4 | |
| 0 | 6 | 0 | 3 | -13.34 | 269.93 | -24.20 | 126.55 | 0.4986 | 373.0 | 343.0 | |
| 18 | 117 | 10 | 66 | -11.71 | 269.49 | -24.64 | 123.30 | 0.4905 | 1541.4 | 692.1 | |
| -17 | -17 | -17 | -17 | -11.84 | 269.17 | -24.96 | 123.19 | 0.4955 | 999999 | 999999 | |
| 14 | 34 | 8 | 20 | -12.99 | 268.22 | -25.91 | 124.17 | 0.5167 | 1203.1 | 673.1 | |
| 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. | |