SOHO MDI 2000-11-01 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 111 | 2 | 63 | -27.15 | 292.46 | -2.54 | 175.66 | 0.5249 | 926.3 | 744.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | -28.65 | 295.12 | 0.11 | 180.18 | 0.5453 | 933.0 | 733.8 | |
| 0 | 6 | 0 | 3 | -29.15 | 294.90 | -0.11 | 179.83 | 0.5527 | 480.0 | 426.9 | |
| 0 | 4 | 0 | 2 | -26.96 | 294.90 | -0.11 | 179.81 | 0.5203 | 705.0 | 534.0 | |
| 0 | 3 | 0 | 2 | -25.53 | 294.56 | -0.45 | 179.19 | 0.4987 | 689.0 | 558.6 | |
| 0 | 2 | 0 | 1 | -25.62 | 294.30 | -0.70 | 178.72 | 0.5002 | 662.0 | 539.9 | |
| 0 | 2 | 0 | 1 | -29.43 | 294.10 | -0.91 | 178.58 | 0.5569 | 606.0 | 539.2 | |
| 0 | 3 | 0 | 2 | -26.47 | 293.61 | -1.40 | 177.55 | 0.5133 | 715.0 | 660.9 | |
| 0 | 4 | 0 | 3 | -26.88 | 293.22 | -1.79 | 176.91 | 0.5197 | 1037.0 | 881.9 | |
| 0 | 9 | 0 | 5 | -27.10 | 292.91 | -2.10 | 176.41 | 0.5233 | 873.0 | 632.4 | |
| 0 | 4 | 0 | 2 | -25.22 | 292.77 | -2.24 | 175.90 | 0.4952 | 1068.0 | 852.8 | |
| 0 | 15 | 0 | 9 | -26.52 | 292.53 | -2.48 | 175.68 | 0.5150 | 1129.0 | 1014.7 | |
| 0 | 4 | 0 | 2 | -29.67 | 292.46 | -2.55 | 176.04 | 0.5614 | 659.0 | 632.5 | |
| 3 | 19 | 2 | 11 | -26.56 | 292.14 | -2.86 | 175.01 | 0.5162 | 1212.3 | 935.3 | |
| 0 | 3 | 0 | 2 | -26.66 | 291.49 | -3.51 | 173.91 | 0.5185 | 882.0 | 767.2 | |
| 0 | 7 | 0 | 4 | -27.56 | 291.34 | -3.67 | 173.85 | 0.5321 | 876.0 | 709.2 | |
| 0 | 4 | 0 | 2 | -27.11 | 290.83 | -4.18 | 172.89 | 0.5263 | 554.0 | 430.3 | |
| 0 | 4 | 0 | 2 | -28.89 | 290.45 | -4.56 | 172.74 | 0.5531 | 629.0 | 536.4 | |
| 0 | 5 | 0 | 3 | -27.93 | 290.05 | -4.95 | 171.84 | 0.5399 | 734.0 | 615.8 | |
| 0 | 2 | 0 | 1 | -27.03 | 290.01 | -5.00 | 171.49 | 0.5268 | 681.0 | 555.2 | |
| 0 | 5 | 0 | 3 | -26.89 | 289.49 | -5.51 | 170.59 | 0.5260 | 827.0 | 640.5 | |
| 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. | |