| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 86.29 | 418.57 | 45.69 | 220.67 | 15.20 | 232.31 | -14.64 | 45.45 | 0.3404 | -545.2 | -278.1 | |
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back to the solar disc SDO HMI 2011-11-24 20:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.58 | 15.03 | 236.58 | -10.37 | 36.99 | 0.2901 | -832.0 | -534.4 | |
| 7.02 | 21.14 | 3.62 | 10.91 | 13.54 | 235.47 | -11.47 | 43.28 | 0.2834 | -1074.4 | -718.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 16.46 | 235.31 | -11.63 | 37.19 | 0.3214 | 818.0 | 550.6 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 13.26 | 234.86 | -12.08 | 45.43 | 0.2873 | -1174.0 | -929.5 | |
| 0.00 | 3.08 | 0.00 | 1.62 | 17.22 | 234.25 | -12.70 | 38.09 | 0.3418 | -926.0 | -755.1 | |
| 48.54 | 279.23 | 25.31 | 145.59 | 14.96 | 234.24 | -12.71 | 42.78 | 0.3143 | -1431.8 | -457.6 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 12.81 | 234.36 | -12.59 | 47.76 | 0.2883 | -923.0 | -747.3 | |
| 0.68 | -6.00 | 0.36 | -6.00 | 14.65 | 233.94 | -13.00 | 44.12 | 0.3141 | -978.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.27 | 233.38 | -13.56 | 39.78 | 0.3514 | -933.0 | -519.3 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 14.98 | 232.41 | -14.53 | 46.49 | 0.3358 | -995.0 | -824.0 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.23 | 232.17 | -14.77 | 42.22 | 0.3640 | -795.0 | -593.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 17.45 | 232.12 | -14.82 | 41.90 | 0.3670 | -782.0 | -655.2 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 14.55 | 232.28 | -14.66 | 47.71 | 0.3327 | -704.0 | -507.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.26 | 231.88 | -15.06 | 42.70 | 0.3675 | -877.0 | -664.7 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 12.10 | 232.15 | -14.79 | 54.05 | 0.3098 | 882.0 | 653.5 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 14.03 | 231.87 | -15.07 | 49.67 | 0.3324 | -830.0 | -652.6 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 16.28 | 231.58 | -15.36 | 45.22 | 0.3599 | -945.0 | -741.7 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 17.41 | 231.39 | -15.56 | 43.31 | 0.3747 | -789.0 | -607.0 | |
| 0.34 | 2.57 | 0.18 | 1.38 | 18.34 | 231.27 | -15.67 | 41.78 | 0.3865 | -866.2 | -679.0 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 16.40 | 231.28 | -15.66 | 45.51 | 0.3646 | -806.0 | -594.6 | |
| 3.00 | 4.62 | 1.59 | 2.46 | 16.03 | 231.05 | -15.89 | 46.67 | 0.3633 | -884.3 | -854.3 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 16.75 | 228.99 | -17.95 | 48.55 | 0.3955 | -658.0 | -528.2 | |
| 0.60 | 1.46 | 0.33 | 0.79 | 17.35 | 227.75 | -19.19 | 49.18 | 0.4163 | -901.6 | -794.0 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 17.81 | 227.57 | -19.37 | 48.57 | 0.4230 | -865.0 | -685.7 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 19.14 | 226.95 | -20.00 | 47.03 | 0.4434 | -514.0 | -446.6 | |
| 0.00 | 2.05 | 0.00 | 1.12 | 16.76 | 226.73 | -20.21 | 51.71 | 0.4233 | 992.0 | 760.3 | |
| 0.00 | 1.80 | 0.00 | 0.98 | 15.90 | 226.73 | -20.22 | 53.41 | 0.4157 | 890.0 | 724.2 | |
| 0.94 | 4.28 | 0.51 | 2.33 | 15.69 | 226.59 | -20.36 | 54.03 | 0.4156 | 817.8 | 580.0 | |
| 0.00 | 1.88 | 0.00 | 1.03 | 17.06 | 226.37 | -20.57 | 51.59 | 0.4305 | 909.0 | 766.6 | |
| 6.59 | 12.24 | 3.60 | 6.68 | 15.62 | 226.07 | -20.88 | 54.80 | 0.4218 | 952.9 | 504.3 | |
| 0.00 | 4.02 | 0.00 | 2.21 | 16.62 | 225.66 | -21.29 | 53.32 | 0.4356 | 790.0 | 697.9 | |
| 7.70 | 53.33 | 4.22 | 29.28 | 15.98 | 225.66 | -21.28 | 54.56 | 0.4300 | 1198.5 | 708.3 | |
| 2.23 | -32.00 | 1.22 | -32.00 | 16.38 | 225.42 | -21.52 | 54.08 | 0.4365 | 859.3 | 999999 | |
| 8.65 | -32.00 | 4.75 | -32.00 | 15.89 | 225.25 | -21.70 | 55.25 | 0.4346 | 853.6 | 999999 | |
| 0.00 | 3.94 | 0.00 | 2.16 | 15.34 | 225.17 | -21.77 | 56.42 | 0.4311 | 516.0 | 522.3 | |
| 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. | |