| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.25 | 192.82 | 22.71 | 103.46 | -16.55 | 266.38 | -12.98 | 145.95 | 0.3856 | 128.1 | -11.5 | |
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back to the solar disc SDO HMI 2011-11-22 09:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.38 | -21.31 | 269.50 | -9.86 | 158.02 | 0.4281 | 606.0 | 561.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -17.97 | 269.01 | -10.35 | 153.39 | 0.3831 | 789.0 | 480.2 | |
| 0.00 | 3.69 | 0.00 | 1.99 | -18.79 | 268.70 | -10.65 | 153.72 | 0.3970 | 720.0 | 564.0 | |
| 0.00 | 10.63 | 0.00 | 5.61 | -15.32 | 268.72 | -10.64 | 149.06 | 0.3479 | 111.0 | 368.4 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -15.84 | 268.69 | -10.67 | 149.79 | 0.3555 | 853.0 | 602.2 | |
| 0.00 | 3.26 | 0.00 | 1.72 | -14.85 | 268.55 | -10.80 | 147.94 | 0.3429 | -993.0 | -826.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -15.75 | 268.47 | -10.88 | 149.16 | 0.3560 | 825.0 | 613.1 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -15.10 | 268.48 | -10.88 | 148.16 | 0.3470 | -796.0 | -613.9 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -11.78 | 268.41 | -10.94 | 141.98 | 0.3030 | 879.0 | 734.4 | |
| 0.00 | 2.06 | 0.00 | 1.09 | -15.51 | 268.21 | -11.15 | 148.17 | 0.3549 | 1031.0 | 853.1 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -12.88 | 268.21 | -11.14 | 143.67 | 0.3195 | 1004.0 | 853.3 | |
| 17.14 | 57.61 | 9.16 | 30.79 | -16.79 | 267.79 | -11.57 | 149.14 | 0.3760 | 1144.4 | 440.3 | |
| 0.00 | 3.09 | 0.00 | 1.64 | -16.16 | 267.76 | -11.60 | 148.17 | 0.3677 | 852.0 | 678.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -15.42 | 267.52 | -11.84 | 146.49 | 0.3597 | 773.0 | 614.0 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -11.21 | 267.51 | -11.84 | 138.53 | 0.3054 | 766.0 | 596.4 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -21.30 | 266.39 | -12.97 | 152.09 | 0.4487 | 679.0 | 506.8 | |
| 0.00 | 3.51 | 0.00 | 1.89 | -17.17 | 266.52 | -12.83 | 147.07 | 0.3920 | -264.0 | -102.6 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -16.58 | 266.53 | -12.82 | 146.20 | 0.3841 | 677.0 | 429.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -13.32 | 266.73 | -12.63 | 141.09 | 0.3401 | 864.0 | 685.0 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -17.86 | 266.44 | -12.91 | 147.89 | 0.4019 | 682.0 | 532.0 | |
| 0.00 | 11.06 | 0.00 | 5.95 | -16.99 | 266.22 | -13.14 | 146.18 | 0.3923 | -832.0 | -615.4 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -16.05 | 266.22 | -13.14 | 144.75 | 0.3800 | 678.0 | 441.0 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -17.49 | 265.64 | -13.72 | 145.80 | 0.4041 | 772.0 | 704.6 | |
| 0.00 | 2.57 | 0.00 | 1.38 | -16.59 | 265.52 | -13.84 | 144.19 | 0.3935 | -905.0 | -767.8 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -18.22 | 265.26 | -14.10 | 146.13 | 0.4169 | 747.0 | 522.6 | |
| 7.54 | 32.06 | 4.05 | 17.21 | -15.84 | 265.16 | -14.20 | 142.31 | 0.3876 | -935.9 | -534.6 | |
| 2.14 | 8.40 | 1.16 | 4.56 | -17.47 | 264.75 | -14.61 | 144.09 | 0.4120 | 480.8 | -153.3 | |
| 12.09 | 21.95 | 6.53 | 11.85 | -16.53 | 264.63 | -14.73 | 142.42 | 0.4014 | -1036.8 | -782.2 | |
| 3.34 | 4.63 | 1.81 | 2.51 | -17.03 | 264.40 | -14.96 | 142.79 | 0.4099 | -874.6 | -758.1 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -18.78 | 263.27 | -16.09 | 143.42 | 0.4421 | 581.0 | 454.6 | |
| 0.00 | 1.54 | 0.00 | 0.84 | -16.42 | 263.29 | -16.06 | 139.85 | 0.4135 | -846.0 | -753.4 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -18.37 | 262.43 | -16.93 | 141.45 | 0.4452 | -804.0 | -594.1 | |
| 0.00 | 2.31 | 0.00 | 1.29 | -19.40 | 261.60 | -17.76 | 141.62 | 0.4654 | -572.0 | -540.0 | |
| 0.00 | 2.06 | 0.00 | 1.15 | -18.51 | 261.27 | -18.09 | 139.84 | 0.4584 | -379.0 | -369.1 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -16.73 | 260.74 | -18.62 | 136.25 | 0.4440 | -645.0 | -543.8 | |
| 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. | |