SDO HMI 2011-12-01 10:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.47 | 258.59 | 18.61 | 161.80 | 20.46 | 192.85 | 32.66 | 303.98 | 0.6120 | -232.9 | -200.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.73 | 18.81 | 198.38 | 38.18 | 298.00 | 0.6650 | -479.0 | -417.2 | |
| 8.71 | 192.56 | 5.55 | 122.16 | 19.90 | 194.91 | 34.72 | 301.54 | 0.6306 | -836.8 | -370.0 | |
| 18.20 | -2.00 | 11.52 | -2.00 | 19.66 | 194.50 | 34.31 | 301.44 | 0.6245 | -1213.7 | 999999 | |
| 0.00 | 2.65 | 0.00 | 1.67 | 21.74 | 193.21 | 33.01 | 305.32 | 0.6225 | -681.0 | -565.7 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 17.35 | 192.02 | 31.83 | 299.58 | 0.5811 | -715.0 | -601.9 | |
| 0.00 | 1.79 | 0.00 | 1.10 | 19.17 | 192.33 | 32.13 | 302.19 | 0.5959 | -721.0 | -638.4 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 22.13 | 192.02 | 31.83 | 306.75 | 0.6119 | -758.0 | -538.9 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 22.29 | 192.02 | 31.83 | 306.97 | 0.6131 | -655.0 | -542.1 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 21.48 | 191.00 | 30.81 | 306.60 | 0.5959 | -726.0 | -541.8 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 21.29 | 190.92 | 30.72 | 306.38 | 0.5936 | -974.0 | -761.4 | |
| 0.00 | 1.37 | 0.00 | 0.83 | 20.63 | 190.66 | 30.46 | 305.62 | 0.5859 | -770.0 | -648.8 | |
| 1.11 | 1.88 | 0.68 | 1.15 | 20.85 | 190.67 | 30.48 | 305.93 | 0.5876 | -801.6 | -720.9 | |
| 0.00 | 1.28 | 0.00 | 0.79 | 22.20 | 190.99 | 30.80 | 307.65 | 0.6010 | -615.0 | -489.2 | |
| 0.00 | 1.79 | 0.00 | 1.10 | 21.38 | 190.35 | 30.16 | 306.99 | 0.5879 | -842.0 | -633.0 | |
| 0.00 | 1.71 | 0.00 | 1.00 | 15.61 | 189.00 | 28.81 | 298.91 | 0.5323 | -748.0 | -577.0 | |
| 0.00 | 2.22 | 0.00 | 1.33 | 21.43 | 188.14 | 27.95 | 308.96 | 0.5633 | 704.0 | 530.0 | |
| 0.00 | 1.62 | 0.00 | 0.97 | 21.88 | 187.55 | 27.36 | 310.17 | 0.5603 | 810.0 | 637.0 | |
| 0.00 | 2.82 | 0.00 | 1.67 | 22.01 | 186.51 | 26.31 | 311.38 | 0.5499 | 807.0 | 709.6 | |
| 1.45 | 2.90 | 0.86 | 1.72 | 22.39 | 186.51 | 26.32 | 311.94 | 0.5533 | 770.8 | 672.4 | |
| 0.00 | 2.05 | 0.00 | 1.21 | 22.20 | 186.26 | 26.07 | 311.91 | 0.5489 | 757.0 | 645.4 | |
| 0.00 | 1.20 | 0.00 | 0.70 | 21.82 | 186.05 | 25.85 | 311.57 | 0.5432 | 897.0 | 756.0 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 22.59 | 186.05 | 25.86 | 312.68 | 0.5500 | 665.0 | 576.1 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 22.21 | 185.87 | 25.68 | 312.31 | 0.5446 | 891.0 | 781.8 | |
| 0.00 | 3.84 | 0.00 | 2.26 | 22.97 | 185.07 | 24.87 | 314.28 | 0.5430 | 808.0 | 750.2 | |
| 0.00 | 2.22 | 0.00 | 1.33 | 25.19 | 185.53 | 25.34 | 316.86 | 0.5685 | 667.0 | 573.8 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 25.55 | 185.54 | 25.35 | 317.32 | 0.5720 | 494.0 | 410.9 | |
| 0.00 | 9.48 | 0.00 | 5.61 | 23.84 | 184.85 | 24.66 | 315.74 | 0.5488 | 689.0 | 611.3 | |
| 0.00 | 1.88 | 0.00 | 1.10 | 23.10 | 184.67 | 24.47 | 314.89 | 0.5400 | 678.0 | 655.6 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 24.07 | 184.68 | 24.49 | 316.23 | 0.5493 | 612.0 | 513.6 | |
| 0.00 | 1.62 | 0.00 | 0.99 | 26.73 | 185.27 | 25.07 | 319.13 | 0.5807 | 563.0 | 396.6 | |
| 0.00 | 3.16 | 0.00 | 1.85 | 22.95 | 184.43 | 24.23 | 314.93 | 0.5360 | 797.0 | 675.9 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 26.18 | 185.03 | 24.84 | 318.67 | 0.5731 | 687.0 | 517.1 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 25.95 | 184.94 | 24.75 | 318.47 | 0.5700 | 591.0 | 600.2 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 26.80 | 185.03 | 24.83 | 319.47 | 0.5791 | 706.0 | 582.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 23.97 | 184.17 | 23.97 | 316.67 | 0.5432 | 829.0 | 724.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 25.40 | 184.28 | 24.09 | 318.47 | 0.5582 | 683.0 | 594.4 | |
| 0.00 | 2.22 | 0.00 | 1.33 | 26.21 | 184.35 | 24.16 | 319.46 | 0.5670 | 838.0 | 591.6 | |
| 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. | |