| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.59 | 290.97 | 51.56 | 152.26 | 18.95 | 171.80 | 5.04 | 345.08 | 0.3247 | -21.3 | -173.9 | |
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back to the solar disc SDO HMI 2011-11-30 22:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.79 | 153.08 | 0.94 | 80.21 | 18.96 | 175.02 | 8.26 | 336.28 | 0.3393 | 635.0 | -526.6 | |
| 2.65 | -1.00 | 1.39 | -1.00 | 19.12 | 174.81 | 8.05 | 337.02 | 0.3402 | -787.7 | 999999 | |
| 0.00 | 2.31 | 0.00 | 1.22 | 19.40 | 174.73 | 7.97 | 337.56 | 0.3439 | -254.0 | -105.4 | |
| 23.92 | -1.00 | 12.53 | -1.00 | 18.59 | 174.06 | 7.30 | 338.33 | 0.3276 | -1307.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 19.81 | 173.51 | 6.75 | 341.11 | 0.3431 | 275.0 | 267.2 | |
| 5.13 | -1.00 | 2.69 | -1.00 | 18.93 | 173.41 | 6.65 | 340.46 | 0.3291 | -1011.8 | 999999 | |
| 3.93 | -1.00 | 2.06 | -1.00 | 18.62 | 173.40 | 6.64 | 340.15 | 0.3242 | -990.3 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 18.97 | 173.07 | 6.31 | 341.43 | 0.3277 | -754.0 | -582.1 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 18.69 | 172.93 | 6.17 | 341.51 | 0.3226 | -1031.0 | -750.2 | |
| 0.00 | 2.14 | 0.00 | 1.12 | 18.63 | 172.65 | 5.89 | 342.25 | 0.3202 | -836.0 | -641.5 | |
| 4.95 | 7.26 | 2.59 | 3.80 | 18.87 | 172.62 | 5.86 | 342.56 | 0.3240 | -972.9 | -787.8 | |
| 7.86 | 17.43 | 4.11 | 9.11 | 18.91 | 171.90 | 5.14 | 344.61 | 0.3211 | -1064.5 | -773.4 | |
| 1.79 | -12.00 | 0.94 | -12.00 | 18.97 | 171.59 | 4.83 | 345.56 | 0.3208 | -858.6 | 999999 | |
| 1.71 | 1.96 | 0.89 | 1.03 | 19.34 | 171.38 | 4.62 | 346.45 | 0.3259 | -774.2 | -812.3 | |
| 2.31 | 6.58 | 1.20 | 3.42 | 18.22 | 171.17 | 4.40 | 346.19 | 0.3071 | 973.4 | 782.8 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.63 | 170.80 | 4.04 | 347.60 | 0.3122 | 353.0 | 244.7 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.19 | 170.70 | 3.94 | 347.59 | 0.3048 | 790.0 | 634.7 | |
| 1.88 | 2.31 | 0.98 | 1.20 | 18.47 | 170.58 | 3.82 | 348.15 | 0.3089 | 895.3 | 927.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.90 | 170.58 | 3.82 | 349.08 | 0.3322 | -778.0 | -608.1 | |
| 0.00 | 2.48 | 0.00 | 1.29 | 18.66 | 169.71 | 2.95 | 350.90 | 0.3094 | 970.0 | 857.7 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 19.34 | 169.63 | 2.87 | 351.50 | 0.3204 | 846.0 | 600.4 | |
| 2.31 | 3.50 | 1.21 | 1.83 | 19.59 | 169.60 | 2.84 | 351.69 | 0.3244 | 897.4 | 684.4 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 20.03 | 169.48 | 2.72 | 352.23 | 0.3313 | 919.0 | 669.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.78 | 169.37 | 2.61 | 352.00 | 0.3106 | 751.0 | 578.3 | |
| 8.03 | 13.67 | 4.19 | 7.13 | 19.06 | 168.96 | 2.20 | 353.33 | 0.3143 | 1069.4 | 839.8 | |
| 1.20 | 1.88 | 0.62 | 0.98 | 19.41 | 168.84 | 2.08 | 353.82 | 0.3197 | 768.2 | 682.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 21.51 | 168.27 | 1.51 | 356.01 | 0.3535 | 785.0 | 498.2 | |
| 4.87 | 43.05 | 2.54 | 22.46 | 19.47 | 167.84 | 1.08 | 356.80 | 0.3194 | 863.2 | 648.8 | |
| 1.20 | 3.16 | 0.63 | 1.66 | 20.19 | 167.69 | 0.93 | 357.36 | 0.3312 | 1066.3 | 880.6 | |
| 0.68 | 3.50 | 0.36 | 1.84 | 20.44 | 167.59 | 0.83 | 357.66 | 0.3353 | 877.5 | 796.0 | |
| 5.81 | -28.00 | 3.03 | -28.00 | 18.94 | 167.46 | 0.70 | 357.85 | 0.3103 | 1078.2 | 999999 | |
| 13.92 | -28.00 | 7.27 | -28.00 | 19.38 | 167.43 | 0.67 | 357.99 | 0.3176 | 1081.8 | 999999 | |
| 2.65 | 9.74 | 1.39 | 5.11 | 20.06 | 167.18 | 0.42 | 358.79 | 0.3288 | 944.1 | 731.0 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 19.13 | 166.49 | -0.27 | 0.81 | 0.3133 | 1061.0 | 733.8 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 19.44 | 166.09 | -0.68 | 2.01 | 0.3186 | 904.0 | 615.9 | |
| 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. | |