SOHO MDI 2001-02-01 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34 | 386 | 27 | 318 | 24.90 | 115.01 | -44.37 | 52.41 | 0.8005 | 1094.8 | 200.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 5 | 25.88 | 117.77 | -41.61 | 49.80 | 0.7845 | -313.0 | -331.2 | |
| 28 | 208 | 22 | 162 | 23.78 | 117.45 | -41.93 | 52.30 | 0.7752 | 1347.7 | 552.2 | |
| 6 | 48 | 5 | 39 | 25.37 | 116.26 | -43.12 | 51.26 | 0.7941 | 807.9 | 243.0 | |
| 0 | 4 | 0 | 3 | 25.98 | 115.27 | -44.11 | 51.17 | 0.8055 | 89.0 | 129.9 | |
| 0 | 5 | 0 | 4 | 24.40 | 114.57 | -44.81 | 53.28 | 0.8030 | 286.0 | 279.7 | |
| 0 | 6 | 0 | 5 | 26.24 | 113.62 | -45.76 | 51.80 | 0.8199 | 206.0 | 116.4 | |
| 0 | 3 | 0 | 3 | 23.59 | 114.75 | -44.63 | 54.06 | 0.7974 | 291.0 | 380.1 | |
| 0 | 3 | 0 | 3 | 30.19 | 111.14 | -48.24 | 48.99 | 0.8566 | -373.0 | -277.0 | |
| 0 | 6 | 0 | 5 | 23.49 | 113.91 | -45.47 | 54.64 | 0.8041 | 248.0 | 213.8 | |
| 0 | 2 | 0 | 1 | 24.81 | 112.68 | -46.70 | 53.84 | 0.8205 | 182.0 | 73.0 | |
| 0 | 2 | 0 | 2 | 24.00 | 112.88 | -46.50 | 54.61 | 0.8151 | 271.0 | 190.3 | |
| 0 | 5 | 0 | 5 | 27.32 | 110.94 | -48.44 | 52.05 | 0.8452 | 260.0 | 177.4 | |
| 0 | 7 | 0 | 6 | 24.72 | 112.23 | -47.15 | 54.17 | 0.8237 | 164.0 | -53.3 | |
| 0 | 12 | 0 | 11 | 24.22 | 112.34 | -47.04 | 54.65 | 0.8205 | -543.0 | -557.1 | |
| 0 | 2 | 0 | 2 | 25.17 | 110.98 | -48.40 | 54.30 | 0.8356 | -687.0 | -713.2 | |
| 0 | 43 | 0 | 40 | 26.96 | 109.90 | -49.48 | 52.94 | 0.8512 | -825.0 | -556.9 | |
| 0 | 8 | 0 | 7 | 24.91 | 110.99 | -48.39 | 54.58 | 0.8343 | -881.0 | -763.6 | |
| 0 | 11 | 0 | 11 | 28.85 | 107.43 | -51.95 | 52.11 | 0.8760 | -352.0 | -231.5 | |
| 0 | 4 | 0 | 4 | 29.34 | 106.56 | -52.82 | 51.99 | 0.8834 | -55.0 | -76.0 | |
| 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. | |