SDO HMI 2011-11-30 14:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.85 | 260.90 | 37.46 | 135.97 | 18.95 | 171.30 | 0.12 | 359.40 | 0.3129 | -16.5 | -53.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.96 | 0.00 | 1.02 | 18.13 | 174.71 | 3.53 | 348.77 | 0.3019 | -959.0 | -669.2 | |
| 1.96 | 121.13 | 1.02 | 62.99 | 18.29 | 174.34 | 3.16 | 350.02 | 0.3033 | -909.7 | -520.8 | |
| 19.99 | -2.00 | 10.39 | -2.00 | 18.48 | 173.94 | 2.76 | 351.37 | 0.3053 | -1321.5 | 999999 | |
| 0.77 | -2.00 | 0.40 | -2.00 | 18.38 | 173.56 | 2.38 | 352.49 | 0.3029 | -951.1 | 999999 | |
| 4.19 | -2.00 | 2.18 | -2.00 | 18.66 | 173.50 | 2.32 | 352.79 | 0.3074 | -1030.0 | 999999 | |
| 3.59 | -2.00 | 1.87 | -2.00 | 18.91 | 173.26 | 2.08 | 353.64 | 0.3110 | -892.3 | 999999 | |
| 0.00 | 3.67 | 0.00 | 1.91 | 18.69 | 172.85 | 1.67 | 354.82 | 0.3067 | -881.0 | -712.2 | |
| 0.00 | 3.08 | 0.00 | 1.60 | 19.00 | 172.79 | 1.61 | 355.10 | 0.3118 | -875.0 | -715.3 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.23 | 172.75 | 1.57 | 354.98 | 0.2988 | -865.0 | -762.9 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.54 | 172.25 | 1.07 | 356.63 | 0.3034 | -639.0 | -446.2 | |
| 5.81 | 7.18 | 3.02 | 3.74 | 18.88 | 172.19 | 1.01 | 356.88 | 0.3090 | -930.0 | -656.3 | |
| 0.00 | 2.48 | 0.00 | 1.29 | 18.97 | 171.41 | 0.23 | 359.29 | 0.3101 | -1050.0 | -832.7 | |
| 0.00 | 2.31 | 0.00 | 1.20 | 18.32 | 171.38 | 0.20 | 359.36 | 0.2993 | 833.0 | 603.3 | |
| 1.20 | 1.71 | 0.62 | 0.89 | 18.94 | 171.13 | -0.05 | 0.15 | 0.3096 | -824.4 | -795.7 | |
| 0.00 | 5.72 | 0.00 | 2.97 | 18.26 | 171.13 | -0.05 | 0.15 | 0.2982 | 828.0 | 767.5 | |
| 0.00 | 4.10 | 0.00 | 2.14 | 19.35 | 170.91 | -0.27 | 0.80 | 0.3164 | -796.0 | -673.6 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.26 | 170.79 | -0.39 | 1.25 | 0.2983 | 1175.0 | 874.8 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.41 | 170.70 | -0.48 | 1.53 | 0.3009 | 805.0 | 683.9 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 19.97 | 170.38 | -0.80 | 2.32 | 0.3270 | -1024.0 | -767.5 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 20.06 | 169.94 | -1.24 | 3.57 | 0.3289 | -956.0 | -731.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.79 | 169.79 | -1.39 | 4.30 | 0.3079 | 910.0 | 736.9 | |
| 2.05 | 5.55 | 1.07 | 2.90 | 19.38 | 169.63 | -1.55 | 4.63 | 0.3179 | 906.2 | 847.7 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 19.50 | 169.44 | -1.74 | 5.16 | 0.3202 | 721.0 | 601.1 | |
| 3.93 | 11.53 | 2.05 | 6.01 | 19.10 | 169.16 | -2.02 | 6.11 | 0.3140 | 1103.2 | 941.7 | |
| 1.71 | 2.22 | 0.89 | 1.16 | 19.28 | 168.85 | -2.33 | 6.98 | 0.3177 | 885.6 | 858.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.22 | 168.80 | -2.38 | 6.75 | 0.3331 | 840.0 | 637.1 | |
| 0.00 | 2.48 | 0.00 | 1.29 | 18.82 | 168.38 | -2.80 | 8.58 | 0.3110 | 1010.0 | 769.5 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 20.88 | 168.25 | -2.93 | 7.99 | 0.3451 | 1043.0 | 741.1 | |
| 3.84 | 7.26 | 2.01 | 3.80 | 19.41 | 168.12 | -3.06 | 9.05 | 0.3214 | 988.7 | 792.1 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 20.44 | 168.04 | -3.14 | 8.76 | 0.3384 | 721.0 | 588.5 | |
| 3.84 | 4.78 | 2.02 | 2.51 | 20.03 | 167.86 | -3.32 | 9.47 | 0.3323 | 959.8 | 676.6 | |
| 1.20 | 7.69 | 0.63 | 4.04 | 20.41 | 167.66 | -3.52 | 9.82 | 0.3389 | 798.2 | 643.2 | |
| 14.44 | 39.04 | 7.55 | 20.39 | 19.38 | 167.65 | -3.53 | 10.43 | 0.3222 | 1104.4 | 649.1 | |
| 3.33 | -33.00 | 1.74 | -33.00 | 18.94 | 167.63 | -3.55 | 10.76 | 0.3151 | 1209.1 | 999999 | |
| 0.00 | 2.56 | 0.00 | 1.35 | 20.00 | 167.42 | -3.76 | 10.72 | 0.3330 | 902.0 | 751.4 | |
| 0.00 | 5.21 | 0.00 | 2.74 | 20.03 | 167.01 | -4.17 | 11.83 | 0.3348 | 743.0 | 656.0 | |
| 0.00 | 2.99 | 0.00 | 1.56 | 19.31 | 166.55 | -4.62 | 13.61 | 0.3249 | 852.0 | 793.4 | |
| 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. | |