SOHO MDI 2001-02-04 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35 | 330 | 20 | 191 | 24.18 | 115.03 | -7.46 | 12.89 | 0.5220 | 1383.7 | 425.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 202 | 18 | 115 | 23.34 | 117.18 | -5.31 | 9.78 | 0.5024 | 1689.5 | 591.9 | |
| 3 | 10 | 2 | 6 | 24.65 | 115.42 | -7.06 | 12.30 | 0.5267 | 884.4 | 737.9 | |
| 0 | 13 | 0 | 7 | 23.37 | 115.07 | -7.41 | 13.51 | 0.5092 | 1096.0 | 849.0 | |
| 0 | 6 | 0 | 4 | 23.24 | 114.40 | -8.08 | 14.74 | 0.5099 | 877.0 | 715.2 | |
| 0 | 9 | 0 | 5 | 24.68 | 113.67 | -8.81 | 15.20 | 0.5332 | 746.0 | 610.3 | |
| 0 | 5 | 0 | 3 | 23.26 | 113.52 | -8.97 | 16.26 | 0.5136 | 571.0 | 567.2 | |
| 0 | 3 | 0 | 2 | 23.85 | 112.62 | -9.86 | 17.40 | 0.5259 | 674.0 | 646.7 | |
| 0 | 2 | 0 | 1 | 23.19 | 112.59 | -9.90 | 17.88 | 0.5167 | 634.0 | 587.2 | |
| 0 | 6 | 0 | 3 | 19.33 | 112.73 | -9.76 | 20.40 | 0.4608 | 969.0 | 791.1 | |
| 0 | 5 | 0 | 3 | 25.34 | 112.12 | -10.37 | 17.31 | 0.5489 | 644.0 | 530.3 | |
| 0 | 15 | 0 | 9 | 25.08 | 111.58 | -10.91 | 18.31 | 0.5477 | 771.0 | 515.5 | |
| 0 | 10 | 0 | 6 | 24.46 | 111.42 | -11.07 | 18.96 | 0.5399 | 845.0 | 590.7 | |
| 0 | 3 | 0 | 2 | 28.81 | 110.85 | -11.64 | 17.17 | 0.6012 | -728.0 | -697.6 | |
| 0 | 3 | 0 | 2 | 27.53 | 110.15 | -12.34 | 18.90 | 0.5873 | -493.0 | -519.5 | |
| 0 | 8 | 0 | 5 | 27.63 | 109.56 | -12.93 | 19.66 | 0.5914 | -941.0 | -750.0 | |
| 0 | 5 | 0 | 3 | 29.05 | 108.93 | -13.56 | 19.62 | 0.6127 | -521.0 | -515.2 | |
| 0 | 3 | 0 | 2 | 29.43 | 108.74 | -13.74 | 19.63 | 0.6184 | -503.0 | -439.7 | |
| 0 | 4 | 0 | 2 | 27.75 | 108.79 | -13.70 | 20.65 | 0.5966 | -752.0 | -670.2 | |
| 0 | 3 | 0 | 2 | 29.77 | 108.47 | -14.02 | 19.77 | 0.6240 | -667.0 | -611.8 | |
| 0 | 15 | 0 | 9 | 27.43 | 108.56 | -13.93 | 21.17 | 0.5937 | -842.0 | -843.8 | |
| 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. | |