SDO HMI 2011-11-30 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 |
| 66.38 | 233.28 | 34.61 | 121.73 | 18.98 | 170.94 | -2.43 | 7.02 | 0.3158 | -104.5 | 19.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.30 | 175.02 | 1.64 | 355.08 | 0.3166 | -878.0 | -674.6 | |
| 3.67 | 91.44 | 1.91 | 47.49 | 18.24 | 174.23 | 0.85 | 357.27 | 0.2981 | -1095.5 | -602.3 | |
| 18.54 | -2.00 | 9.63 | -2.00 | 18.46 | 173.92 | 0.54 | 358.28 | 0.3015 | -1278.7 | 999999 | |
| 2.56 | -2.00 | 1.33 | -2.00 | 18.58 | 173.23 | -0.14 | 0.45 | 0.3035 | -1044.2 | 999999 | |
| 3.59 | 5.30 | 1.87 | 2.76 | 18.86 | 173.11 | -0.27 | 0.83 | 0.3082 | -938.0 | -651.5 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 18.27 | 172.98 | -0.39 | 1.25 | 0.2984 | -734.0 | -562.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.68 | 172.70 | -0.67 | 2.10 | 0.3052 | -681.0 | -497.3 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.96 | 172.67 | -0.71 | 2.16 | 0.3099 | -811.0 | -627.4 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.08 | 172.57 | -0.80 | 2.43 | 0.3120 | -737.0 | -615.4 | |
| 7.01 | 8.55 | 3.65 | 4.45 | 18.96 | 172.04 | -1.33 | 4.07 | 0.3105 | -871.3 | -592.4 | |
| 0.00 | 1.79 | 0.00 | 0.93 | 18.43 | 171.99 | -1.39 | 4.39 | 0.3018 | -162.0 | -265.0 | |
| 0.00 | 3.33 | 0.00 | 1.73 | 18.77 | 171.23 | -2.14 | 6.61 | 0.3086 | 111.0 | 38.3 | |
| 5.64 | 6.32 | 2.93 | 3.28 | 18.24 | 171.15 | -2.23 | 7.10 | 0.3001 | 1008.3 | 767.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 19.05 | 171.10 | -2.27 | 6.89 | 0.3135 | -905.0 | -657.1 | |
| 1.28 | 1.45 | 0.67 | 0.75 | 18.27 | 170.83 | -2.54 | 8.06 | 0.3013 | 801.3 | 824.0 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.92 | 170.82 | -2.55 | 7.78 | 0.3121 | -947.0 | -779.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.17 | 170.79 | -2.58 | 7.77 | 0.3162 | -579.0 | -524.8 | |
| 0.00 | 2.82 | 0.00 | 1.47 | 19.45 | 170.69 | -2.68 | 7.94 | 0.3211 | -781.0 | -742.9 | |
| 0.00 | 2.56 | 0.00 | 1.34 | 19.98 | 170.27 | -3.10 | 8.88 | 0.3308 | -1056.0 | -844.4 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 20.01 | 169.93 | -3.45 | 9.84 | 0.3322 | -885.0 | -602.4 | |
| 2.05 | 3.08 | 1.07 | 1.61 | 19.20 | 169.66 | -3.71 | 11.08 | 0.3198 | 945.8 | 862.8 | |
| 0.00 | 3.33 | 0.00 | 1.74 | 18.86 | 169.64 | -3.74 | 11.37 | 0.3143 | 958.0 | 824.7 | |
| 1.45 | 7.86 | 0.76 | 4.11 | 18.99 | 169.23 | -4.15 | 12.49 | 0.3177 | 984.9 | 905.9 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.20 | 168.88 | -4.49 | 12.60 | 0.3386 | 728.0 | 549.1 | |
| 1.54 | 3.93 | 0.80 | 2.06 | 19.23 | 168.84 | -4.53 | 13.40 | 0.3232 | 861.4 | 650.1 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.86 | 168.48 | -4.90 | 14.75 | 0.3186 | 873.0 | 797.4 | |
| 0.00 | 2.99 | 0.00 | 1.58 | 20.73 | 168.17 | -5.21 | 14.11 | 0.3498 | 943.0 | 771.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.23 | 168.15 | -5.22 | 14.53 | 0.3419 | 658.0 | 465.6 | |
| 1.79 | 4.27 | 0.94 | 2.25 | 20.01 | 167.97 | -5.40 | 15.19 | 0.3392 | 989.6 | 745.2 | |
| 13.59 | 51.10 | 7.12 | 26.77 | 19.36 | 167.74 | -5.63 | 16.39 | 0.3298 | 1058.0 | 710.3 | |
| 1.11 | 7.86 | 0.59 | 4.14 | 20.29 | 167.67 | -5.70 | 15.74 | 0.3449 | 811.0 | 788.3 | |
| 2.56 | -30.00 | 1.34 | -30.00 | 18.98 | 167.66 | -5.72 | 16.96 | 0.3243 | 1143.4 | 999999 | |
| 0.00 | 3.42 | 0.00 | 1.80 | 20.42 | 167.48 | -5.89 | 16.14 | 0.3478 | 586.0 | 565.4 | |
| 0.00 | 3.67 | 0.00 | 1.94 | 19.95 | 166.96 | -6.41 | 17.91 | 0.3429 | 812.0 | 611.2 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 19.45 | 166.51 | -6.87 | 19.60 | 0.3375 | 914.0 | 751.2 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 19.23 | 166.26 | -7.11 | 20.48 | 0.3356 | 970.0 | 728.1 | |
| 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. | |