SDO HMI 2011-10-11 05:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.24 | 116.27 | 21.63 | 59.60 | 19.95 | 109.99 | -5.38 | 20.14 | 0.2574 | 223.1 | 109.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.59 | 21.91 | 112.37 | -3.01 | 10.18 | 0.2770 | 794.0 | 553.8 | |
| 15.51 | 35.57 | 7.92 | 18.18 | 20.02 | 112.24 | -3.13 | 12.10 | 0.2461 | -1067.1 | -858.9 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 25.96 | 112.10 | -3.27 | 8.62 | 0.3442 | 774.0 | 593.0 | |
| 2.28 | -2.00 | 1.17 | -2.00 | 20.35 | 111.98 | -3.39 | 12.75 | 0.2526 | -713.8 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 21.50 | 111.79 | -3.58 | 12.39 | 0.2722 | 906.0 | 624.3 | |
| 0.70 | 5.96 | 0.36 | 3.05 | 19.92 | 111.13 | -4.25 | 16.31 | 0.2491 | -902.0 | -767.3 | |
| 0.00 | 1.93 | 0.00 | 0.98 | 19.58 | 110.92 | -4.46 | 17.51 | 0.2446 | -925.0 | -636.6 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 24.94 | 110.74 | -4.64 | 12.82 | 0.3318 | 719.0 | 594.8 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 19.94 | 110.01 | -5.37 | 20.23 | 0.2553 | 710.0 | 444.2 | |
| 0.00 | 3.94 | 0.00 | 2.02 | 19.84 | 109.63 | -5.75 | 21.67 | 0.2561 | 554.0 | 577.3 | |
| 6.75 | 52.83 | 3.46 | 27.10 | 19.80 | 109.09 | -6.29 | 23.55 | 0.2591 | 988.8 | 586.6 | |
| 1.49 | 5.43 | 0.76 | 2.78 | 19.37 | 109.11 | -6.27 | 24.22 | 0.2524 | 1040.8 | 932.4 | |
| 15.16 | -11.00 | 7.78 | -11.00 | 19.61 | 108.42 | -6.95 | 26.05 | 0.2608 | 1171.8 | 999999 | |
| 0.00 | 2.37 | 0.00 | 1.21 | 19.21 | 108.35 | -7.03 | 27.03 | 0.2554 | 810.0 | 705.3 | |
| 0.35 | 1.23 | 0.18 | 0.63 | 20.10 | 108.02 | -7.36 | 26.46 | 0.2712 | 781.2 | 590.5 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 21.12 | 102.59 | -12.79 | 38.40 | 0.3339 | -799.0 | -625.3 | |
| 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. | |