SOHO MDI 2001-02-01 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52 | 424 | 40 | 334 | 24.84 | 114.97 | -41.77 | 50.94 | 0.7788 | 837.7 | 166.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 2 | 26.42 | 118.11 | -38.64 | 47.29 | 0.7634 | -259.0 | -335.8 | |
| 0 | 9 | 0 | 7 | 26.07 | 117.91 | -38.83 | 47.79 | 0.7627 | -632.0 | -469.8 | |
| 34 | 217 | 25 | 162 | 23.75 | 117.48 | -39.26 | 50.63 | 0.7517 | 1356.4 | 564.0 | |
| 8 | 50 | 7 | 39 | 25.29 | 116.28 | -40.46 | 49.70 | 0.7716 | 796.4 | 179.3 | |
| 0 | 8 | 0 | 6 | 24.38 | 116.03 | -40.71 | 50.86 | 0.7682 | 321.0 | 363.6 | |
| 0 | 3 | 0 | 2 | 24.41 | 114.56 | -42.19 | 51.75 | 0.7810 | 461.0 | 335.0 | |
| 0 | 4 | 0 | 3 | 23.96 | 114.63 | -42.12 | 52.20 | 0.7779 | 462.0 | 442.2 | |
| 0 | 4 | 0 | 3 | 26.36 | 113.47 | -43.28 | 50.28 | 0.8009 | 319.0 | 266.5 | |
| 0 | 3 | 0 | 2 | 23.71 | 114.44 | -42.30 | 52.59 | 0.7782 | 333.0 | 417.1 | |
| 0 | 5 | 0 | 4 | 30.10 | 111.24 | -45.51 | 47.64 | 0.8373 | -235.0 | -206.3 | |
| 0 | 9 | 0 | 8 | 27.33 | 110.79 | -45.95 | 50.75 | 0.8268 | 272.0 | 70.2 | |
| 10 | 62 | 8 | 52 | 24.44 | 111.86 | -44.88 | 53.26 | 0.8039 | -439.3 | -436.7 | |
| 0 | 26 | 0 | 23 | 27.11 | 109.65 | -47.09 | 51.58 | 0.8343 | -794.0 | -638.2 | |
| 0 | 5 | 0 | 5 | 28.99 | 108.41 | -48.33 | 50.25 | 0.8519 | -633.0 | -519.3 | |
| 0 | 1 | 0 | 1 | 24.88 | 110.19 | -46.55 | 53.68 | 0.8197 | -644.0 | -597.7 | |
| 0 | 16 | 0 | 15 | 28.72 | 107.32 | -49.43 | 51.08 | 0.8584 | -402.0 | -261.8 | |
| 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. | |