SOHO MDI 2000-11-01 18:01:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 135 | 0 | 78 | -27.08 | 291.04 | -0.22 | 179.59 | 0.5223 | 693.2 | 637.4 | |
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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 | -28.68 | 294.98 | 3.72 | 185.99 | 0.5482 | 798.0 | 663.7 | |
| 0 | 5 | 0 | 3 | -29.46 | 294.03 | 2.78 | 184.35 | 0.5583 | 535.0 | 382.2 | |
| 0 | 6 | 0 | 3 | -27.36 | 293.24 | 1.99 | 183.36 | 0.5266 | 774.0 | 611.8 | |
| 0 | 2 | 0 | 1 | -27.44 | 292.94 | 1.68 | 182.84 | 0.5277 | 806.0 | 667.0 | |
| 0 | 6 | 0 | 3 | -25.52 | 292.83 | 1.57 | 182.85 | 0.4986 | 910.0 | 687.4 | |
| 0 | 12 | 0 | 7 | -26.54 | 292.54 | 1.28 | 182.24 | 0.5139 | 1081.0 | 921.6 | |
| 0 | 11 | 0 | 6 | -27.31 | 292.55 | 1.29 | 182.19 | 0.5254 | 765.0 | 648.7 | |
| 0 | 9 | 0 | 5 | -26.54 | 292.11 | 0.85 | 181.49 | 0.5137 | 1199.0 | 987.4 | |
| 0 | 4 | 0 | 2 | -26.86 | 291.89 | 0.64 | 181.10 | 0.5183 | 921.0 | 816.4 | |
| 0 | 10 | 0 | 6 | -27.49 | 291.16 | -0.10 | 179.84 | 0.5277 | 601.0 | 627.6 | |
| 0 | 7 | 0 | 4 | -26.86 | 290.99 | -0.27 | 179.54 | 0.5183 | 793.0 | 713.1 | |
| 0 | 3 | 0 | 2 | -28.68 | 290.28 | -0.98 | 178.42 | 0.5454 | 690.0 | 576.0 | |
| 0 | 8 | 0 | 5 | -26.86 | 290.12 | -1.13 | 178.04 | 0.5185 | 1080.0 | 890.6 | |
| 0 | 15 | 0 | 9 | -27.63 | 289.73 | -1.53 | 177.43 | 0.5302 | 764.0 | 661.9 | |
| 0 | 12 | 0 | 7 | -26.95 | 289.43 | -1.82 | 176.86 | 0.5204 | 674.0 | 579.4 | |
| 0 | 5 | 0 | 3 | -24.81 | 289.08 | -2.17 | 175.94 | 0.4884 | 778.0 | 585.0 | |
| 0 | 5 | 0 | 3 | -26.46 | 288.79 | -2.46 | 175.69 | 0.5136 | -399.0 | -241.5 | |
| 0 | 4 | 0 | 2 | -25.74 | 288.04 | -3.22 | 174.22 | 0.5039 | -500.0 | -515.9 | |
| 0 | 7 | 0 | 4 | -27.23 | 287.48 | -3.78 | 173.59 | 0.5269 | 901.0 | 717.0 | |
| 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. | |