SDO HMI 2011-10-09 23:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.12 | 208.91 | 18.55 | 116.74 | 23.48 | 154.12 | 22.26 | 311.30 | 0.4643 | -503.8 | -323.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.01 | 190.06 | 3.93 | 106.48 | 23.12 | 155.07 | 23.21 | 309.45 | 0.4712 | -1029.6 | -432.8 | |
| 26.11 | -1.00 | 14.62 | -1.00 | 23.33 | 154.68 | 22.82 | 310.23 | 0.4684 | -1289.8 | 999999 | |
| 0.00 | 2.02 | 0.00 | 1.11 | 22.21 | 153.65 | 21.78 | 309.37 | 0.4463 | 617.0 | 440.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 25.61 | 150.08 | 18.22 | 320.03 | 0.4407 | 786.0 | 625.0 | |
| 0.00 | 1.93 | 0.00 | 1.04 | 23.43 | 148.08 | 16.22 | 319.41 | 0.3956 | 747.0 | 710.0 | |
| 0.00 | 1.49 | 0.00 | 0.82 | 26.01 | 148.36 | 16.50 | 323.27 | 0.4286 | 702.0 | 559.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 25.90 | 147.93 | 16.07 | 323.78 | 0.4232 | 827.0 | 723.9 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 23.89 | 147.49 | 15.63 | 321.21 | 0.3949 | 868.0 | 678.2 | |
| 0.00 | 1.84 | 0.00 | 1.00 | 25.95 | 147.21 | 15.35 | 325.04 | 0.4172 | 639.0 | 585.5 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 28.15 | 146.75 | 14.89 | 328.93 | 0.4408 | 624.0 | 516.7 | |
| 0.00 | 1.75 | 0.00 | 0.97 | 28.41 | 146.40 | 14.54 | 329.85 | 0.4415 | 773.0 | 569.5 | |
| 0.00 | 3.42 | 0.00 | 1.85 | 26.23 | 144.98 | 13.11 | 329.40 | 0.4015 | 592.0 | 664.4 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 24.32 | 142.15 | 10.29 | 332.43 | 0.3532 | 842.0 | 724.7 | |
| 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. | |