SDO HMI 2011-11-22 14:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.92 | 361.51 | 42.04 | 200.85 | 14.05 | 252.28 | -24.34 | 62.02 | 0.4544 | -597.2 | -349.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.84 | 17.29 | 257.89 | -18.73 | 49.10 | 0.4074 | -752.0 | -463.4 | |
| 0.00 | 1.88 | 0.00 | 1.03 | 18.11 | 257.30 | -19.32 | 48.36 | 0.4225 | -855.0 | -551.5 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 12.51 | 257.26 | -19.36 | 60.32 | 0.3742 | -766.0 | -612.2 | |
| 0.00 | 3.51 | 0.00 | 1.90 | 12.43 | 255.45 | -21.17 | 62.51 | 0.3992 | -898.0 | -711.8 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 16.93 | 254.12 | -22.50 | 54.57 | 0.4512 | -626.0 | -517.7 | |
| 1.46 | 2.23 | 0.81 | 1.23 | 16.26 | 254.10 | -22.52 | 55.88 | 0.4459 | 821.8 | 713.4 | |
| 41.38 | 296.94 | 22.85 | 164.28 | 13.90 | 252.97 | -23.64 | 61.74 | 0.4439 | -1282.5 | -444.2 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 14.78 | 252.44 | -24.18 | 60.48 | 0.4571 | -700.0 | -512.9 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 15.23 | 252.25 | -24.37 | 59.76 | 0.4627 | -488.0 | -379.1 | |
| 10.37 | -7.00 | 5.76 | -7.00 | 14.05 | 252.32 | -24.30 | 62.04 | 0.4538 | -874.1 | 999999 | |
| 13.11 | -7.00 | 7.27 | -7.00 | 13.53 | 252.21 | -24.41 | 63.18 | 0.4520 | -932.6 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.01 | 15.13 | 251.89 | -24.73 | 60.28 | 0.4669 | -776.0 | -687.1 | |
| 2.23 | 3.60 | 1.25 | 2.02 | 15.68 | 251.65 | -24.97 | 59.46 | 0.4738 | 673.8 | 487.6 | |
| 2.31 | 3.26 | 1.28 | 1.80 | 12.53 | 251.92 | -24.70 | 65.48 | 0.4502 | -780.4 | -799.7 | |
| 1.03 | 1.37 | 0.57 | 0.76 | 12.89 | 251.75 | -24.87 | 64.88 | 0.4547 | -656.0 | -549.2 | |
| 0.00 | 5.31 | 0.00 | 2.98 | 15.10 | 251.35 | -25.26 | 60.83 | 0.4739 | -712.0 | -720.8 | |
| 4.03 | -7.00 | 2.25 | -7.00 | 13.82 | 251.47 | -25.14 | 63.21 | 0.4641 | -621.1 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 12.41 | 251.63 | -24.99 | 65.97 | 0.4536 | -600.0 | -517.8 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 12.74 | 251.56 | -25.06 | 65.34 | 0.4565 | -528.0 | -384.7 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 14.76 | 251.19 | -25.43 | 61.62 | 0.4739 | -706.0 | -607.7 | |
| 0.00 | 3.17 | 0.00 | 1.78 | 14.45 | 250.79 | -25.83 | 62.55 | 0.4774 | -828.0 | -666.5 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 12.27 | 250.67 | -25.95 | 66.95 | 0.4666 | 634.0 | 504.3 | |
| 0.00 | 2.23 | 0.00 | 1.26 | 14.19 | 249.97 | -26.65 | 63.69 | 0.4871 | 868.0 | 658.6 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 17.60 | 249.16 | -27.46 | 58.16 | 0.5194 | -604.0 | -475.4 | |
| 0.00 | 3.51 | 0.00 | 2.00 | 14.67 | 249.36 | -27.26 | 63.26 | 0.4982 | 965.0 | 818.4 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 14.62 | 248.15 | -28.47 | 64.22 | 0.5143 | 712.0 | 609.1 | |
| 0.00 | 3.60 | 0.00 | 2.10 | 16.23 | 247.73 | -28.89 | 61.66 | 0.5291 | 1000.0 | 776.0 | |
| 0.00 | 3.17 | 0.00 | 1.84 | 15.47 | 247.85 | -28.77 | 62.91 | 0.5231 | 871.0 | 753.2 | |
| 0.00 | 1.29 | 0.00 | 0.74 | 14.65 | 247.90 | -28.71 | 64.34 | 0.5178 | 647.0 | 467.8 | |
| 0.00 | 3.08 | 0.00 | 1.79 | 15.28 | 247.77 | -28.84 | 63.29 | 0.5230 | 723.0 | 563.8 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 15.74 | 247.46 | -29.16 | 62.72 | 0.5298 | 711.0 | 635.2 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 16.78 | 245.96 | -30.65 | 61.96 | 0.5552 | 869.0 | 739.0 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 16.82 | 244.43 | -32.18 | 62.89 | 0.5750 | 621.0 | 520.6 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 12.65 | 244.26 | -32.36 | 69.98 | 0.5580 | 548.0 | 459.0 | |
| 0.00 | 1.37 | 0.00 | 0.86 | 19.00 | 242.36 | -34.25 | 60.73 | 0.6124 | 627.0 | 524.6 | |
| 0.00 | 1.03 | 0.00 | 0.65 | 19.36 | 241.48 | -35.14 | 60.72 | 0.6249 | 598.0 | 478.4 | |
| 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. | |