SDO HMI 2011-01-01 07:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.71 | 185.82 | 32.95 | 120.90 | 34.10 | 267.51 | 16.53 | 338.64 | 0.6497 | -53.7 | 23.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.31 | 96.53 | 13.25 | 63.12 | 33.49 | 269.86 | 18.88 | 335.52 | 0.6536 | -1099.0 | -265.4 | |
| 2.97 | 3.48 | 1.93 | 2.26 | 33.51 | 268.71 | 17.73 | 336.83 | 0.6476 | -782.3 | -777.3 | |
| 1.78 | 5.35 | 1.16 | 3.48 | 33.98 | 268.33 | 17.35 | 337.60 | 0.6512 | -672.5 | -706.0 | |
| 0.00 | 0.68 | 0.00 | 0.43 | 31.69 | 266.36 | 15.37 | 338.34 | 0.6134 | 708.0 | 670.5 | |
| 2.97 | 4.76 | 1.94 | 3.10 | 34.62 | 266.75 | 15.76 | 339.85 | 0.6512 | -762.8 | -584.9 | |
| 0.00 | 1.27 | 0.00 | 0.82 | 34.59 | 264.85 | 13.87 | 342.05 | 0.6426 | 717.0 | 583.4 | |
| 0.34 | 1.27 | 0.21 | 0.81 | 33.22 | 264.55 | 13.57 | 341.60 | 0.6242 | 878.0 | 808.7 | |
| 0.00 | 0.93 | 0.00 | 0.59 | 33.40 | 264.54 | 13.56 | 341.72 | 0.6264 | 768.0 | 691.5 | |
| 5.18 | 71.55 | 3.38 | 46.29 | 35.53 | 264.75 | 13.77 | 342.70 | 0.6539 | 705.9 | 510.1 | |
| 2.80 | -9.00 | 1.82 | -9.00 | 35.08 | 264.67 | 13.69 | 342.54 | 0.6479 | 833.7 | 999999 | |
| 1.53 | -9.00 | 1.00 | -9.00 | 35.30 | 264.71 | 13.73 | 342.62 | 0.6509 | 777.6 | 999999 | |
| 2.97 | -9.00 | 1.91 | -9.00 | 34.36 | 264.18 | 13.20 | 342.72 | 0.6370 | 974.5 | 999999 | |
| 9.86 | -9.00 | 6.35 | -9.00 | 34.77 | 264.10 | 13.12 | 343.05 | 0.6418 | 1031.6 | 999999 | |
| 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. | |