SDO HMI 2011-10-25 19:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.74 | 173.71 | 20.97 | 147.58 | -21.62 | 331.34 | 48.31 | 238.70 | 0.8143 | -455.6 | -289.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.22 | 0.00 | 1.17 | -18.80 | 337.73 | 54.71 | 244.47 | 0.8583 | 202.0 | 144.0 | |
| 0.00 | 1.91 | 0.00 | 1.78 | -17.81 | 336.89 | 53.87 | 245.29 | 0.8486 | 618.0 | 536.8 | |
| 2.17 | 10.42 | 2.06 | 9.89 | -18.96 | 337.20 | 54.18 | 244.11 | 0.8545 | 757.8 | 493.0 | |
| 0.00 | 3.91 | 0.00 | 3.69 | -19.48 | 336.86 | 53.84 | 243.41 | 0.8533 | 367.0 | 354.6 | |
| 0.00 | 0.95 | 0.00 | 0.89 | -19.04 | 336.54 | 53.52 | 243.79 | 0.8493 | 566.0 | 568.2 | |
| 0.00 | 0.95 | 0.00 | 0.88 | -19.14 | 336.22 | 53.20 | 243.55 | 0.8470 | 626.0 | 569.3 | |
| 0.00 | 1.04 | 0.00 | 0.96 | -19.16 | 335.96 | 52.94 | 243.44 | 0.8449 | 625.0 | 614.9 | |
| 0.00 | 1.30 | 0.00 | 1.11 | -21.65 | 331.55 | 48.52 | 238.81 | 0.8162 | -514.0 | -384.3 | |
| 5.30 | 23.09 | 4.45 | 19.37 | -21.35 | 330.93 | 47.90 | 238.87 | 0.8096 | -701.2 | -344.2 | |
| 0.43 | 128.92 | 0.37 | 107.84 | -21.70 | 330.84 | 47.82 | 238.43 | 0.8103 | -579.2 | -416.9 | |
| 0.78 | -10.00 | 0.66 | -10.00 | -22.03 | 330.70 | 47.68 | 238.00 | 0.8104 | -569.4 | 999999 | |
| 8.77 | -10.00 | 7.36 | -10.00 | -22.34 | 330.46 | 47.43 | 237.53 | 0.8097 | -851.9 | 999999 | |
| 7.29 | -10.00 | 6.07 | -10.00 | -21.99 | 330.21 | 47.18 | 237.80 | 0.8060 | -1102.1 | 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. | |