| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.62 | 25.43 | 2.40 | 13.13 | -20.47 | 67.65 | 8.06 | 207.51 | 0.2805 | -36.9 | -159.3 | |
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back to the solar disc SDO HMI 2011-02-12 04:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.83 | 0.00 | 1.47 | -20.04 | 71.94 | 12.35 | 220.72 | 0.3093 | 877.0 | 756.8 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -20.35 | 71.86 | 12.27 | 219.88 | 0.3123 | 899.0 | 819.2 | |
| 4.62 | 5.14 | 2.40 | 2.67 | -20.11 | 71.62 | 12.03 | 219.86 | 0.3067 | 1074.9 | 862.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -21.67 | 71.42 | 11.83 | 216.16 | 0.3244 | 771.0 | 632.7 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -20.12 | 71.07 | 11.48 | 218.57 | 0.3012 | 923.0 | 808.1 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -20.23 | 70.34 | 10.75 | 216.57 | 0.2951 | 862.0 | 657.2 | |
| 0.00 | 1.97 | 0.00 | 1.01 | -20.77 | 64.69 | 5.10 | 198.84 | 0.2587 | -1137.0 | -894.2 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -20.87 | 64.47 | 4.88 | 197.97 | 0.2590 | -927.0 | -777.9 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -19.86 | 64.25 | 4.66 | 198.51 | 0.2418 | -1082.0 | -971.8 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -19.87 | 63.97 | 4.38 | 197.46 | 0.2403 | -910.0 | -809.5 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -20.84 | 63.65 | 4.06 | 195.11 | 0.2547 | -748.0 | -572.7 | |
| 0.00 | 2.14 | 0.00 | 1.10 | -21.06 | 63.18 | 3.59 | 193.22 | 0.2563 | -781.0 | -636.6 | |
| 0.00 | 2.05 | 0.00 | 1.05 | -20.94 | 62.98 | 3.39 | 192.65 | 0.2536 | -1008.0 | -729.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -20.73 | 62.28 | 2.69 | 190.25 | 0.2477 | -887.0 | -716.2 | |
| 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. | |