SDO HMI 2011-10-11 04:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.34 | 129.14 | 25.28 | 66.20 | 19.82 | 109.82 | -6.10 | 22.75 | 0.2594 | 233.1 | 267.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.68 | 22.16 | 112.71 | -3.21 | 10.66 | 0.2817 | 902.0 | 707.0 | |
| 11.83 | 35.48 | 6.05 | 18.14 | 20.14 | 112.21 | -3.71 | 14.12 | 0.2503 | -999.4 | -843.8 | |
| 4.91 | -2.00 | 2.51 | -2.00 | 19.80 | 112.16 | -3.77 | 14.68 | 0.2450 | -1200.8 | 999999 | |
| 2.54 | -2.00 | 1.30 | -2.00 | 19.98 | 111.86 | -4.06 | 15.55 | 0.2492 | -1038.1 | 999999 | |
| 1.84 | 5.43 | 0.94 | 2.78 | 19.92 | 111.10 | -4.82 | 18.38 | 0.2519 | -845.5 | -857.7 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 19.52 | 110.92 | -5.00 | 19.57 | 0.2465 | -998.0 | -770.4 | |
| 0.00 | 2.02 | 0.00 | 1.03 | 19.94 | 110.04 | -5.88 | 21.98 | 0.2584 | 704.0 | 395.6 | |
| 0.00 | 3.42 | 0.00 | 1.75 | 19.90 | 109.66 | -6.26 | 23.31 | 0.2603 | 878.0 | 647.5 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 20.61 | 109.34 | -6.58 | 23.22 | 0.2733 | -582.0 | -381.7 | |
| 0.00 | 7.01 | 0.00 | 3.59 | 19.40 | 109.20 | -6.72 | 25.68 | 0.2559 | 847.0 | 869.3 | |
| 7.10 | 67.73 | 3.64 | 34.77 | 19.83 | 109.12 | -6.80 | 25.19 | 0.2630 | 962.3 | 677.5 | |
| 21.12 | -11.00 | 10.84 | -11.00 | 19.64 | 108.46 | -7.47 | 27.63 | 0.2651 | 1116.6 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 19.24 | 108.31 | -7.61 | 28.84 | 0.2603 | 908.0 | 741.9 | |
| 0.00 | 3.50 | 0.00 | 1.80 | 20.10 | 108.05 | -7.88 | 28.03 | 0.2750 | 696.0 | 405.4 | |
| 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. | |