SOHO MDI 2001-02-06 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 332 | 25 | 202 | 24.55 | 113.39 | 15.49 | 334.47 | 0.5706 | 1040.2 | 223.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27 | 170 | 16 | 102 | 22.99 | 116.71 | 18.81 | 328.51 | 0.5705 | 1477.3 | 529.9 | |
| 6 | 33 | 4 | 20 | 24.88 | 112.05 | 14.15 | 336.71 | 0.5633 | 1018.6 | 722.0 | |
| 0 | 10 | 0 | 6 | 24.47 | 111.69 | 13.80 | 336.91 | 0.5559 | 892.0 | 870.5 | |
| 3 | -2 | 2 | -2 | 25.19 | 111.73 | 13.84 | 337.40 | 0.5656 | 577.2 | 999999 | |
| 4 | 36 | 2 | 22 | 25.34 | 110.83 | 12.94 | 338.83 | 0.5628 | 821.6 | 274.5 | |
| 0 | 5 | 0 | 3 | 26.16 | 110.93 | 13.03 | 339.27 | 0.5741 | 69.0 | -87.5 | |
| 0 | 4 | 0 | 3 | 26.97 | 110.62 | 12.73 | 340.25 | 0.5834 | -509.0 | -409.4 | |
| 2 | 21 | 1 | 13 | 26.78 | 110.20 | 12.31 | 340.72 | 0.5788 | -990.0 | -653.4 | |
| 0 | 9 | 0 | 6 | 26.23 | 110.10 | 12.21 | 340.52 | 0.5710 | -944.0 | -744.9 | |
| 0 | 7 | 0 | 4 | 28.26 | 110.29 | 12.39 | 341.52 | 0.5987 | -698.0 | -620.5 | |
| 0 | 5 | 0 | 3 | 26.63 | 109.70 | 11.81 | 341.35 | 0.5745 | -1082.0 | -967.4 | |
| 0 | 3 | 0 | 2 | 27.36 | 109.34 | 11.45 | 342.32 | 0.5826 | -927.0 | -834.7 | |
| 0 | 12 | 0 | 7 | 26.77 | 107.97 | 10.08 | 344.00 | 0.5691 | -899.0 | -863.1 | |
| 0 | 5 | 0 | 3 | 27.55 | 107.78 | 9.88 | 344.70 | 0.5790 | -806.0 | -727.0 | |
| 0 | 3 | 0 | 2 | 27.13 | 107.61 | 9.71 | 344.73 | 0.5726 | -592.0 | -511.1 | |
| 0 | 9 | 0 | 6 | 28.91 | 101.94 | 4.04 | 353.89 | 0.5826 | -627.0 | -642.1 | |
| 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. | |