SDO HMI 2011-11-22 12:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.38 | 344.33 | 38.21 | 192.72 | 14.11 | 252.46 | -25.25 | 62.72 | 0.4675 | -611.4 | -392.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.97 | 0.00 | 1.07 | 17.19 | 257.91 | -19.81 | 50.80 | 0.4196 | -858.0 | -684.3 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 16.91 | 257.64 | -20.07 | 51.69 | 0.4203 | -843.0 | -592.9 | |
| 0.00 | 1.97 | 0.00 | 1.08 | 17.36 | 257.36 | -20.36 | 51.18 | 0.4280 | -692.0 | -469.9 | |
| 0.00 | 2.06 | 0.00 | 1.11 | 12.44 | 257.13 | -20.59 | 61.88 | 0.3910 | -657.0 | -531.8 | |
| 2.31 | 3.00 | 1.29 | 1.67 | 16.28 | 254.09 | -23.63 | 57.03 | 0.4606 | 752.4 | 676.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 17.04 | 253.92 | -23.80 | 55.76 | 0.4686 | -769.0 | -588.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 16.36 | 253.30 | -24.42 | 57.66 | 0.4714 | -683.0 | -563.6 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 16.42 | 252.95 | -24.76 | 57.88 | 0.4764 | 703.0 | 478.9 | |
| 40.10 | 285.70 | 22.33 | 159.32 | 13.89 | 252.96 | -24.75 | 62.75 | 0.4591 | -1233.7 | -451.7 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 15.19 | 252.26 | -25.45 | 60.83 | 0.4770 | -590.0 | -353.2 | |
| 1.46 | -9.00 | 0.82 | -9.00 | 14.49 | 252.32 | -25.40 | 62.12 | 0.4717 | -544.6 | 999999 | |
| 6.51 | -9.00 | 3.65 | -9.00 | 13.97 | 252.35 | -25.37 | 63.11 | 0.4681 | -882.2 | 999999 | |
| 1.20 | -9.00 | 0.67 | -9.00 | 14.16 | 252.29 | -25.42 | 62.80 | 0.4700 | -737.2 | 999999 | |
| 8.57 | -9.00 | 4.79 | -9.00 | 13.55 | 252.26 | -25.45 | 64.02 | 0.4667 | -983.7 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.73 | 15.09 | 251.94 | -25.78 | 61.29 | 0.4807 | -704.0 | -571.2 | |
| 1.46 | 2.83 | 0.83 | 1.60 | 15.70 | 251.62 | -26.10 | 60.43 | 0.4890 | 602.2 | 721.6 | |
| 0.77 | -9.00 | 0.43 | -9.00 | 13.27 | 251.92 | -25.79 | 64.83 | 0.4699 | -490.2 | 999999 | |
| 1.89 | 3.51 | 1.05 | 1.97 | 12.58 | 251.86 | -25.85 | 66.27 | 0.4668 | -875.3 | -726.2 | |
| 1.20 | 1.54 | 0.67 | 0.86 | 12.91 | 251.79 | -25.92 | 65.66 | 0.4696 | -547.2 | -548.5 | |
| 0.00 | 3.94 | 0.00 | 2.23 | 15.02 | 251.40 | -26.32 | 61.86 | 0.4876 | -788.0 | -538.1 | |
| 0.00 | 2.91 | 0.00 | 1.64 | 13.78 | 251.49 | -26.23 | 64.17 | 0.4788 | -736.0 | -589.9 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 12.75 | 251.57 | -26.14 | 66.12 | 0.4719 | -503.0 | -364.4 | |
| 0.00 | 3.00 | 0.00 | 1.69 | 14.05 | 251.35 | -26.36 | 63.75 | 0.4823 | -655.0 | -532.9 | |
| 0.00 | 2.49 | 0.00 | 1.41 | 13.93 | 251.13 | -26.59 | 64.16 | 0.4846 | 56.0 | -95.6 | |
| 0.00 | 2.40 | 0.00 | 1.36 | 14.47 | 250.79 | -26.93 | 63.39 | 0.4925 | -723.0 | -659.3 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 25.18 | 247.48 | -30.24 | 48.86 | 0.6074 | -685.0 | -484.8 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 17.56 | 249.10 | -28.62 | 59.18 | 0.5339 | -679.0 | -568.4 | |
| 2.31 | 4.46 | 1.33 | 2.57 | 14.75 | 249.30 | -28.42 | 63.96 | 0.5143 | 907.7 | 707.6 | |
| 0.00 | 1.37 | 0.00 | 0.80 | 14.73 | 248.39 | -29.33 | 64.61 | 0.5265 | 743.0 | 507.9 | |
| 0.60 | 2.83 | 0.35 | 1.67 | 16.31 | 247.78 | -29.93 | 62.27 | 0.5432 | 902.3 | 776.0 | |
| 0.00 | 2.14 | 0.00 | 1.26 | 15.42 | 247.82 | -29.89 | 63.77 | 0.5377 | 808.0 | 628.3 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 15.73 | 247.60 | -30.12 | 63.40 | 0.5424 | 760.0 | 659.2 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 15.94 | 247.56 | -30.15 | 63.05 | 0.5440 | 744.0 | 618.3 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 15.95 | 246.59 | -31.12 | 63.66 | 0.5568 | 628.0 | 425.1 | |
| 0.00 | 1.29 | 0.00 | 0.77 | 16.77 | 246.01 | -31.71 | 62.67 | 0.5686 | 764.0 | 629.9 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 18.19 | 244.36 | -33.36 | 61.44 | 0.5970 | 614.0 | 523.1 | |
| 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. | |