| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.83 | 406.89 | 35.97 | 212.46 | -18.14 | 352.17 | 6.58 | 200.10 | 0.3189 | 1131.8 | 465.7 | |
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back to the solar disc SDO HMI 2011-12-14 16:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.27 | 301.37 | 23.61 | 157.08 | -17.82 | 352.34 | 6.75 | 200.92 | 0.3148 | 1492.1 | 492.4 | |
| 13.95 | 63.98 | 7.32 | 33.62 | -18.99 | 352.11 | 6.52 | 198.96 | 0.3317 | 1078.8 | 261.6 | |
| 3.74 | 9.27 | 1.96 | 4.85 | -18.59 | 351.50 | 5.90 | 197.69 | 0.3222 | 1181.5 | 845.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -18.16 | 351.48 | 5.89 | 198.09 | 0.3154 | 279.0 | 399.1 | |
| 0.00 | 1.96 | 0.00 | 1.03 | -19.15 | 351.42 | 5.83 | 196.95 | 0.3307 | 806.0 | 687.7 | |
| 3.32 | 12.59 | 1.74 | 6.61 | -19.52 | 351.22 | 5.62 | 196.05 | 0.3356 | 836.8 | 795.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.96 | 351.13 | 5.54 | 196.33 | 0.3264 | 706.0 | 557.5 | |
| 2.55 | -6.00 | 1.34 | -6.00 | -19.56 | 350.93 | 5.34 | 195.26 | 0.3348 | 883.7 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -15.15 | 350.71 | 5.12 | 199.16 | 0.2637 | -793.0 | -676.0 | |
| 0.00 | 1.96 | 0.00 | 1.01 | -15.46 | 350.66 | 5.07 | 198.59 | 0.2683 | -699.0 | -637.3 | |
| 0.00 | 2.21 | 0.00 | 1.16 | -19.84 | 350.69 | 5.10 | 194.38 | 0.3383 | 603.0 | 607.7 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -20.52 | 350.62 | 5.03 | 193.66 | 0.3489 | 602.0 | 503.8 | |
| 0.00 | 5.28 | 0.00 | 2.78 | -20.24 | 350.55 | 4.95 | 193.68 | 0.3442 | 897.0 | 658.3 | |
| 0.00 | 2.47 | 0.00 | 1.30 | -19.90 | 350.47 | 4.88 | 193.74 | 0.3384 | 743.0 | 547.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -19.49 | 350.12 | 4.52 | 193.06 | 0.3305 | 804.0 | 655.8 | |
| 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. | |