SDO HMI 2011-11-30 21:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95.13 | 319.23 | 49.72 | 166.83 | 18.92 | 171.85 | 4.53 | 346.46 | 0.3219 | -35.8 | -110.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.54 | 165.12 | 0.81 | 86.40 | 18.91 | 175.00 | 7.69 | 337.68 | 0.3347 | 618.4 | -502.5 | |
| 1.96 | -1.00 | 1.03 | -1.00 | 19.06 | 174.79 | 7.47 | 338.42 | 0.3357 | -836.5 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.42 | 174.65 | 7.34 | 336.73 | 0.3099 | -698.0 | -536.1 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 19.50 | 174.62 | 7.30 | 339.35 | 0.3414 | -102.0 | -121.0 | |
| 0.60 | -1.00 | 0.31 | -1.00 | 18.38 | 174.41 | 7.10 | 338.62 | 0.3230 | -887.7 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.81 | 174.22 | 6.91 | 340.71 | 0.3439 | 177.0 | 261.9 | |
| 26.39 | -1.00 | 13.81 | -1.00 | 18.60 | 174.04 | 6.73 | 339.87 | 0.3242 | -1303.0 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 19.81 | 173.55 | 6.24 | 342.44 | 0.3405 | 557.0 | 368.2 | |
| 4.95 | -1.00 | 2.59 | -1.00 | 18.91 | 173.36 | 6.05 | 342.07 | 0.3254 | -971.0 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.00 | 173.05 | 5.74 | 343.02 | 0.3253 | -716.0 | -593.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.66 | 172.92 | 5.60 | 343.08 | 0.3193 | -1024.0 | -826.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.63 | 172.66 | 5.35 | 343.77 | 0.3176 | -871.0 | -632.3 | |
| 6.41 | 8.03 | 3.35 | 4.20 | 18.88 | 172.55 | 5.23 | 344.33 | 0.3210 | -957.1 | -676.6 | |
| 8.54 | 23.75 | 4.46 | 12.39 | 18.85 | 171.76 | 4.45 | 346.56 | 0.3173 | -1047.8 | -346.8 | |
| 1.79 | -14.00 | 0.94 | -14.00 | 18.98 | 171.45 | 4.14 | 347.55 | 0.3181 | -763.2 | 999999 | |
| 1.88 | 2.82 | 0.98 | 1.47 | 19.32 | 171.37 | 4.05 | 348.04 | 0.3234 | -822.6 | -724.2 | |
| 2.22 | 7.69 | 1.15 | 4.00 | 18.23 | 171.22 | 3.90 | 347.71 | 0.3052 | 953.1 | 778.0 | |
| 0.00 | 6.15 | 0.00 | 3.20 | 18.51 | 170.72 | 3.41 | 349.41 | 0.3081 | 624.0 | 568.7 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.23 | 170.72 | 3.40 | 349.24 | 0.3035 | 928.0 | 735.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.91 | 170.56 | 3.25 | 350.68 | 0.3305 | -789.0 | -590.8 | |
| 0.00 | 3.84 | 0.00 | 2.00 | 18.70 | 169.79 | 2.48 | 352.35 | 0.3087 | 892.0 | 781.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.32 | 169.74 | 2.42 | 352.78 | 0.3189 | 744.0 | 581.4 | |
| 0.85 | 2.56 | 0.45 | 1.34 | 19.57 | 169.61 | 2.30 | 353.24 | 0.3227 | 985.4 | 789.3 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.98 | 169.43 | 2.12 | 353.91 | 0.3291 | 813.0 | 706.6 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 19.41 | 169.08 | 1.77 | 354.75 | 0.3192 | 645.0 | 604.9 | |
| 7.43 | 16.14 | 3.87 | 8.41 | 19.04 | 168.98 | 1.67 | 354.93 | 0.3129 | 1107.6 | 809.2 | |
| 0.00 | 2.39 | 0.00 | 1.25 | 19.38 | 168.89 | 1.58 | 355.30 | 0.3184 | 945.0 | 725.9 | |
| 4.70 | 43.14 | 2.45 | 22.49 | 19.45 | 167.92 | 0.61 | 358.20 | 0.3186 | 909.7 | 733.1 | |
| 3.84 | 6.49 | 2.02 | 3.40 | 20.19 | 167.73 | 0.42 | 358.80 | 0.3309 | 939.8 | 672.6 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 20.45 | 167.58 | 0.26 | 359.26 | 0.3350 | 838.0 | 775.0 | |
| 14.69 | -28.00 | 7.67 | -28.00 | 19.35 | 167.48 | 0.17 | 359.50 | 0.3169 | 1091.9 | 999999 | |
| 4.95 | -28.00 | 2.58 | -28.00 | 18.95 | 167.48 | 0.17 | 359.49 | 0.3101 | 1110.9 | 999999 | |
| 2.39 | 8.03 | 1.25 | 4.21 | 20.10 | 167.13 | -0.18 | 0.51 | 0.3293 | 867.0 | 844.2 | |
| 0.00 | 2.39 | 0.00 | 1.25 | 19.20 | 166.51 | -0.80 | 2.42 | 0.3145 | 1030.0 | 805.5 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 19.48 | 166.04 | -1.27 | 3.78 | 0.3196 | 876.0 | 647.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 19.54 | 165.60 | -1.71 | 5.06 | 0.3212 | 772.0 | 626.4 | |
| 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. | |