SDO HMI 2011-12-16 10:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.59 | 321.92 | 28.98 | 191.75 | -18.33 | 352.13 | 29.58 | 237.41 | 0.5585 | 993.4 | 400.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.47 | 0.00 | 1.45 | -15.33 | 352.02 | 29.48 | 242.30 | 0.5381 | -671.0 | -532.2 | |
| 7.74 | 298.69 | 4.65 | 178.05 | -19.18 | 352.45 | 29.91 | 236.35 | 0.5680 | 825.8 | 395.0 | |
| 39.06 | -2.00 | 23.27 | -2.00 | -18.09 | 352.21 | 29.66 | 237.86 | 0.5578 | 1281.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -20.03 | 351.22 | 28.68 | 234.01 | 0.5594 | 524.0 | 403.2 | |
| 0.00 | 3.23 | 0.00 | 1.92 | -19.69 | 350.97 | 28.43 | 234.33 | 0.5540 | 883.0 | 682.1 | |
| 0.00 | 1.53 | 0.00 | 0.91 | -19.91 | 351.02 | 28.48 | 234.03 | 0.5561 | 640.0 | 518.0 | |
| 1.79 | 2.81 | 1.06 | 1.66 | -19.35 | 350.84 | 28.30 | 234.75 | 0.5499 | 871.2 | 787.4 | |
| 0.00 | 3.32 | 0.00 | 1.97 | -19.94 | 350.63 | 28.09 | 233.64 | 0.5518 | 693.0 | 646.1 | |
| 0.00 | 0.51 | 0.00 | 0.29 | -14.71 | 349.77 | 27.23 | 241.70 | 0.5047 | -537.0 | -458.2 | |
| 0.00 | 2.72 | 0.00 | 1.61 | -19.57 | 350.49 | 27.95 | 234.09 | 0.5474 | 925.0 | 765.6 | |
| 0.00 | 1.87 | 0.00 | 1.09 | -17.89 | 350.15 | 27.61 | 236.50 | 0.5310 | 654.0 | 513.6 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -19.35 | 350.41 | 27.87 | 234.37 | 0.5448 | 657.0 | 546.6 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -21.86 | 350.66 | 28.12 | 230.76 | 0.5671 | 692.0 | 598.2 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -20.72 | 345.98 | 23.44 | 227.72 | 0.5048 | 673.0 | 557.6 | |
| 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. | |