SDO HMI 2011-11-30 18:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85.57 | 283.79 | 44.65 | 148.09 | 18.97 | 171.47 | 2.50 | 352.32 | 0.3165 | 35.5 | -82.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.39 | 0.00 | 1.25 | 18.12 | 174.87 | 5.90 | 341.66 | 0.3120 | -685.0 | -483.5 | |
| 1.20 | 131.36 | 0.62 | 68.50 | 18.40 | 174.51 | 5.54 | 343.00 | 0.3145 | -529.4 | -501.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.33 | 174.41 | 5.44 | 344.14 | 0.3288 | -554.0 | -399.5 | |
| 0.77 | -2.00 | 0.40 | -2.00 | 18.37 | 174.35 | 5.38 | 343.43 | 0.3133 | -838.9 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 19.67 | 174.33 | 5.36 | 344.66 | 0.3339 | 609.0 | 396.7 | |
| 27.33 | -2.00 | 14.25 | -2.00 | 18.59 | 173.95 | 4.98 | 344.79 | 0.3149 | -1269.6 | 999999 | |
| 1.88 | 8.28 | 0.98 | 4.33 | 18.93 | 173.36 | 4.39 | 346.77 | 0.3180 | -979.0 | -770.9 | |
| 1.79 | -7.00 | 0.94 | -7.00 | 18.87 | 173.14 | 4.17 | 347.37 | 0.3162 | -953.0 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 18.56 | 172.79 | 3.82 | 348.19 | 0.3099 | -693.0 | -508.2 | |
| 6.06 | 7.86 | 3.16 | 4.10 | 18.87 | 172.42 | 3.45 | 349.49 | 0.3138 | -1003.3 | -708.6 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 19.40 | 171.68 | 2.71 | 351.97 | 0.3205 | -724.0 | -533.2 | |
| 4.70 | 8.03 | 2.45 | 4.18 | 18.87 | 171.55 | 2.58 | 352.12 | 0.3115 | -986.4 | -711.5 | |
| 3.84 | 7.86 | 2.00 | 4.08 | 18.31 | 171.26 | 2.29 | 352.75 | 0.3016 | 912.4 | 862.3 | |
| 0.00 | 3.33 | 0.00 | 1.74 | 19.30 | 171.12 | 2.14 | 353.59 | 0.3178 | -649.0 | -656.8 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 18.22 | 170.73 | 1.76 | 354.39 | 0.2991 | 1032.0 | 885.9 | |
| 0.00 | 4.01 | 0.00 | 2.09 | 18.47 | 170.67 | 1.70 | 354.66 | 0.3031 | 1071.0 | 808.1 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 19.93 | 170.46 | 1.49 | 355.69 | 0.3271 | -873.0 | -654.3 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 20.15 | 170.09 | 1.12 | 356.81 | 0.3303 | -735.0 | -546.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 20.40 | 169.87 | 0.90 | 357.47 | 0.3343 | -660.0 | -548.3 | |
| 0.68 | 3.93 | 0.36 | 2.05 | 19.49 | 169.61 | 0.64 | 358.09 | 0.3191 | 1031.0 | 697.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.99 | 169.58 | 0.61 | 358.14 | 0.3108 | 308.0 | 298.6 | |
| 2.05 | 13.67 | 1.07 | 7.11 | 18.78 | 169.27 | 0.30 | 359.08 | 0.3070 | 993.7 | 829.3 | |
| 5.89 | -22.00 | 3.07 | -22.00 | 19.02 | 169.08 | 0.11 | 359.67 | 0.3112 | 1185.9 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.96 | 168.89 | -0.08 | 0.22 | 0.3433 | 651.0 | 522.7 | |
| 0.00 | 2.31 | 0.00 | 1.20 | 19.30 | 168.86 | -0.11 | 0.33 | 0.3158 | 959.0 | 809.3 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 21.47 | 168.48 | -0.49 | 1.31 | 0.3516 | 783.0 | 541.0 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.84 | 168.36 | -0.61 | 1.88 | 0.3082 | 984.0 | 694.2 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 20.93 | 168.29 | -0.68 | 1.86 | 0.3429 | 834.0 | 651.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 21.63 | 168.19 | -0.78 | 2.05 | 0.3544 | 795.0 | 684.5 | |
| 2.73 | 7.60 | 1.43 | 3.97 | 19.37 | 167.98 | -0.99 | 2.95 | 0.3173 | 1039.6 | 729.1 | |
| 3.93 | 6.49 | 2.06 | 3.40 | 20.12 | 167.76 | -1.21 | 3.47 | 0.3299 | 976.4 | 665.6 | |
| 1.45 | 6.92 | 0.76 | 3.63 | 20.46 | 167.60 | -1.37 | 3.85 | 0.3357 | 785.8 | 660.6 | |
| 14.95 | 41.00 | 7.80 | 21.37 | 19.37 | 167.55 | -1.43 | 4.26 | 0.3177 | 1111.3 | 554.0 | |
| 4.10 | -33.00 | 2.14 | -33.00 | 18.93 | 167.55 | -1.42 | 4.35 | 0.3105 | 1172.6 | 999999 | |
| 0.00 | 3.07 | 0.00 | 1.61 | 20.05 | 167.32 | -1.65 | 4.74 | 0.3294 | 1021.0 | 792.0 | |
| 0.85 | 4.18 | 0.45 | 2.20 | 20.08 | 167.07 | -1.90 | 5.45 | 0.3303 | 916.2 | 671.1 | |
| 1.37 | 2.82 | 0.71 | 1.47 | 19.30 | 166.54 | -2.43 | 7.25 | 0.3184 | 913.8 | 821.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.68 | 165.75 | -3.22 | 9.36 | 0.3264 | 785.0 | 570.5 | |
| 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. | |