SDO HMI 2011-12-17 18:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.58 | 86.78 | 10.94 | 47.11 | 21.77 | 301.29 | -3.67 | 6.79 | 0.4052 | -45.0 | 151.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.59 | 18.62 | 312.25 | 7.28 | 340.47 | 0.3610 | 890.0 | 629.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.65 | 307.48 | 2.52 | 353.36 | 0.3597 | -880.0 | -709.7 | |
| 0.00 | 1.87 | 0.00 | 0.99 | 18.99 | 307.22 | 2.26 | 353.82 | 0.3484 | -972.0 | -742.0 | |
| 0.00 | 2.04 | 0.00 | 1.08 | 19.90 | 307.14 | 2.18 | 354.32 | 0.3632 | -840.0 | -572.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.08 | 306.97 | 2.01 | 354.53 | 0.3496 | -781.0 | -667.5 | |
| 0.00 | 2.81 | 0.00 | 1.49 | 19.52 | 306.92 | 1.96 | 354.80 | 0.3567 | -554.0 | -415.5 | |
| 0.00 | 2.38 | 0.00 | 1.26 | 19.17 | 306.79 | 1.83 | 355.05 | 0.3508 | -1006.0 | -785.6 | |
| 17.09 | 21.85 | 9.09 | 11.62 | 20.09 | 306.61 | 1.65 | 355.74 | 0.3655 | -992.6 | -659.3 | |
| 0.00 | 2.30 | 0.00 | 1.21 | 19.14 | 306.32 | 1.36 | 356.31 | 0.3497 | -716.0 | -694.9 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 14.86 | 306.17 | 1.21 | 355.79 | 0.2784 | -759.0 | -620.4 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 19.49 | 305.95 | 0.99 | 357.37 | 0.3551 | 652.0 | 522.8 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 19.80 | 305.64 | 0.67 | 358.23 | 0.3600 | -777.0 | -465.4 | |
| 3.49 | 5.61 | 1.85 | 2.97 | 19.55 | 305.35 | 0.39 | 358.96 | 0.3558 | 799.4 | 404.3 | |
| 0.00 | 2.04 | 0.00 | 1.08 | 18.73 | 304.98 | 0.02 | 359.96 | 0.3423 | 765.0 | 521.0 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 20.31 | 303.12 | -1.84 | 4.69 | 0.3694 | -675.0 | -545.8 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 19.11 | 302.79 | -2.17 | 5.88 | 0.3503 | -925.0 | -769.3 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 18.89 | 301.74 | -3.23 | 8.82 | 0.3490 | -931.0 | -713.4 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 26.85 | 299.42 | -5.55 | 10.39 | 0.4799 | -709.0 | -581.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 22.40 | 297.20 | -7.76 | 17.33 | 0.4208 | 783.0 | 563.0 | |
| 0.00 | 2.98 | 0.00 | 1.67 | 25.90 | 296.39 | -8.57 | 16.41 | 0.4764 | 593.0 | 561.4 | |
| 0.00 | 2.55 | 0.00 | 1.49 | 29.65 | 295.19 | -9.77 | 16.06 | 0.5353 | 775.0 | 631.1 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 30.27 | 294.92 | -10.04 | 16.10 | 0.5451 | 674.0 | 566.6 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 30.06 | 294.87 | -10.09 | 16.30 | 0.5424 | 815.0 | 690.8 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 27.71 | 294.66 | -10.30 | 18.15 | 0.5103 | 676.0 | 547.6 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 23.02 | 295.03 | -9.93 | 21.18 | 0.4413 | 710.0 | 570.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 22.05 | 295.07 | -9.90 | 21.99 | 0.4271 | 878.0 | 756.5 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 29.48 | 294.31 | -10.65 | 17.51 | 0.5367 | 785.0 | 631.1 | |
| 0.00 | 4.08 | 0.00 | 2.23 | 21.51 | 294.65 | -10.31 | 23.35 | 0.4218 | 718.0 | 608.8 | |
| 0.00 | 1.87 | 0.00 | 1.02 | 21.29 | 294.57 | -10.39 | 23.74 | 0.4191 | 973.0 | 795.7 | |
| 0.00 | 2.21 | 0.00 | 1.22 | 22.93 | 294.25 | -10.71 | 22.74 | 0.4446 | 820.0 | 728.9 | |
| 0.00 | 2.98 | 0.00 | 1.62 | 21.22 | 294.29 | -10.67 | 24.38 | 0.4201 | 894.0 | 821.3 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 22.77 | 293.97 | -10.99 | 23.42 | 0.4440 | 758.0 | 629.1 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 29.90 | 293.09 | -11.87 | 19.07 | 0.5481 | 702.0 | 506.2 | |
| 0.00 | 2.47 | 0.00 | 1.40 | 25.22 | 292.46 | -12.50 | 23.79 | 0.4876 | 863.0 | 709.2 | |
| 0.00 | 2.81 | 0.00 | 1.60 | 25.72 | 292.17 | -12.79 | 23.81 | 0.4961 | 572.0 | 540.5 | |
| 0.00 | 1.70 | 0.00 | 0.95 | 21.50 | 289.71 | -15.25 | 32.44 | 0.4582 | 749.0 | 652.8 | |
| 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. | |