SDO HMI 2011-10-25 14:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.16 | 190.25 | 26.81 | 153.08 | -21.64 | 331.40 | 45.62 | 237.40 | 0.7907 | -464.0 | -300.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.86 | -19.08 | 338.01 | 52.23 | 243.26 | 0.8386 | 259.0 | 207.4 | |
| 0.00 | 1.13 | 0.00 | 0.98 | -17.77 | 336.90 | 51.12 | 244.32 | 0.8247 | 573.0 | 543.0 | |
| 0.00 | 3.73 | 0.00 | 3.32 | -18.90 | 337.32 | 51.54 | 243.20 | 0.8321 | 666.0 | 506.0 | |
| 3.47 | 3.99 | 3.05 | 3.51 | -19.05 | 336.78 | 50.99 | 242.81 | 0.8279 | 630.2 | 667.0 | |
| 0.00 | 4.60 | 0.00 | 4.04 | -19.62 | 336.57 | 50.79 | 242.08 | 0.8281 | 242.0 | 359.5 | |
| 1.48 | 6.51 | 1.27 | 5.62 | -19.09 | 335.94 | 50.16 | 242.43 | 0.8208 | 738.8 | 472.8 | |
| 0.00 | 1.30 | 0.00 | 1.05 | -21.74 | 331.65 | 45.86 | 237.44 | 0.7932 | -403.0 | -303.9 | |
| 5.90 | 166.81 | 4.71 | 132.73 | -21.34 | 331.07 | 45.29 | 237.61 | 0.7862 | -714.9 | -395.0 | |
| 0.00 | 0.87 | 0.00 | 0.70 | -22.08 | 331.33 | 45.54 | 236.89 | 0.7920 | -285.0 | -192.2 | |
| 1.82 | -8.00 | 1.46 | -8.00 | -21.80 | 331.03 | 45.24 | 237.06 | 0.7879 | -461.6 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.27 | -20.98 | 330.66 | 44.88 | 237.81 | 0.7807 | -604.0 | -533.8 | |
| 1.82 | -8.00 | 1.46 | -8.00 | -22.09 | 330.87 | 45.09 | 236.65 | 0.7879 | -554.1 | 999999 | |
| 18.67 | -8.00 | 14.86 | -8.00 | -22.20 | 330.50 | 44.72 | 236.33 | 0.7851 | -951.9 | 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. | |