SDO HMI 2011-11-27 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.84 | 200.58 | 18.52 | 128.16 | 14.44 | 251.85 | 37.30 | 291.53 | 0.6330 | -490.6 | -336.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.79 | 184.07 | 17.21 | 118.24 | 14.26 | 252.41 | 37.86 | 290.95 | 0.6393 | -1131.2 | -397.7 | |
| 2.05 | -1.00 | 1.31 | -1.00 | 14.52 | 251.81 | 37.26 | 291.58 | 0.6326 | -916.2 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 17.12 | 251.63 | 37.08 | 295.57 | 0.6412 | -693.0 | -593.6 | |
| 0.00 | 1.37 | 0.00 | 0.88 | 17.40 | 251.54 | 37.00 | 296.03 | 0.6414 | -450.0 | -436.6 | |
| 0.00 | 1.37 | 0.00 | 0.88 | 16.82 | 251.18 | 36.63 | 295.35 | 0.6343 | -625.0 | -545.4 | |
| 0.00 | 1.71 | 0.00 | 1.01 | 12.93 | 245.32 | 30.77 | 292.19 | 0.5406 | 671.0 | 652.5 | |
| 0.00 | 0.51 | 0.00 | 0.31 | 16.99 | 244.82 | 30.27 | 299.44 | 0.5558 | 549.0 | 587.0 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 13.67 | 244.19 | 29.64 | 294.18 | 0.5289 | 761.0 | 603.5 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 17.65 | 243.58 | 29.03 | 301.46 | 0.5443 | 617.0 | 488.4 | |
| 0.00 | 2.22 | 0.00 | 1.28 | 13.41 | 242.86 | 28.32 | 294.59 | 0.5095 | 743.0 | 564.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 17.84 | 243.37 | 28.82 | 301.94 | 0.5428 | 845.0 | 660.3 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 18.86 | 243.38 | 28.83 | 303.59 | 0.5499 | 651.0 | 518.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 18.31 | 243.02 | 28.48 | 302.98 | 0.5418 | 764.0 | 626.7 | |
| 0.00 | 1.20 | 0.00 | 0.70 | 17.60 | 242.55 | 28.00 | 302.21 | 0.5310 | 753.0 | 674.6 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 17.97 | 242.57 | 28.03 | 302.80 | 0.5339 | 619.0 | 504.6 | |
| 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. | |