SDO HMI 2011-01-02 06:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.47 | 118.87 | 24.61 | 85.40 | 33.85 | 267.78 | 29.43 | 325.68 | 0.7256 | -20.6 | -83.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.38 | 73.08 | 11.22 | 53.38 | 33.31 | 270.16 | 31.81 | 323.13 | 0.7365 | -954.9 | -302.8 | |
| 2.80 | 4.59 | 2.01 | 3.29 | 33.30 | 268.51 | 30.15 | 324.46 | 0.7247 | -703.8 | -520.7 | |
| 0.00 | 0.76 | 0.00 | 0.54 | 35.14 | 264.32 | 25.97 | 329.80 | 0.7140 | 410.0 | 248.9 | |
| 2.80 | 6.37 | 1.96 | 4.46 | 34.84 | 264.02 | 25.66 | 329.81 | 0.7091 | 621.9 | 565.3 | |
| 0.00 | 2.12 | 0.00 | 1.45 | 33.48 | 263.27 | 24.91 | 329.33 | 0.6910 | 874.0 | 628.2 | |
| 0.00 | 1.27 | 0.00 | 0.87 | 33.70 | 263.22 | 24.86 | 329.57 | 0.6929 | 655.0 | 617.3 | |
| 5.86 | 17.59 | 4.10 | 12.34 | 35.19 | 263.38 | 25.02 | 330.70 | 0.7088 | 784.1 | 332.6 | |
| 2.12 | 2.89 | 1.47 | 2.00 | 34.48 | 263.11 | 24.75 | 330.35 | 0.7000 | 732.0 | 576.9 | |
| 1.27 | -7.00 | 0.90 | -7.00 | 35.49 | 263.40 | 25.04 | 330.94 | 0.7119 | 343.7 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.71 | 34.66 | 262.89 | 24.53 | 330.71 | 0.7004 | 813.0 | 684.8 | |
| 0.00 | 1.36 | 0.00 | 0.94 | 34.77 | 262.80 | 24.45 | 330.88 | 0.7010 | 744.0 | 611.4 | |
| 1.44 | 7.82 | 1.00 | 5.42 | 34.87 | 262.56 | 24.21 | 331.20 | 0.7006 | 882.6 | 627.2 | |
| 2.80 | -12.00 | 1.95 | -12.00 | 35.10 | 262.51 | 24.16 | 331.43 | 0.7026 | 677.8 | 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. | |