SDO HMI 2011-10-18 00:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 97.53 | 604.74 | 59.51 | 368.80 | 27.35 | 55.36 | 29.59 | 311.02 | 0.5829 | -727.1 | -321.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.70 | 531.64 | 0.43 | 326.00 | 28.06 | 56.40 | 30.62 | 311.15 | 0.5992 | -458.2 | -361.9 | |
| 80.09 | -1.00 | 49.08 | -1.00 | 27.40 | 56.07 | 30.30 | 310.45 | 0.5908 | -1254.2 | 999999 | |
| 4.10 | -1.00 | 2.46 | -1.00 | 26.68 | 54.10 | 28.32 | 311.03 | 0.5640 | -971.0 | 999999 | |
| 3.40 | 12.30 | 2.04 | 7.37 | 27.54 | 53.61 | 27.83 | 312.73 | 0.5657 | -847.9 | -705.4 | |
| 4.97 | -4.00 | 2.97 | -4.00 | 27.29 | 53.50 | 27.72 | 312.45 | 0.5625 | -973.6 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 25.80 | 53.00 | 27.22 | 310.65 | 0.5450 | 474.0 | 330.0 | |
| 0.00 | 0.35 | 0.00 | 0.22 | 31.74 | 54.67 | 28.89 | 317.58 | 0.6114 | -419.0 | -438.5 | |
| 0.00 | 0.70 | 0.00 | 0.42 | 27.72 | 53.24 | 27.46 | 313.32 | 0.5633 | -692.0 | -707.8 | |
| 0.00 | 1.22 | 0.00 | 0.75 | 30.47 | 53.97 | 28.20 | 316.51 | 0.5940 | -580.0 | -436.9 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 28.17 | 52.64 | 26.86 | 314.52 | 0.5608 | -674.0 | -581.2 | |
| 0.00 | 1.48 | 0.00 | 0.89 | 28.30 | 52.52 | 26.75 | 314.83 | 0.5608 | -963.0 | -767.4 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 29.54 | 52.64 | 26.86 | 316.46 | 0.5729 | -725.0 | -539.6 | |
| 0.00 | 0.61 | 0.00 | 0.36 | 28.44 | 52.26 | 26.48 | 315.28 | 0.5594 | -653.0 | -511.4 | |
| 0.00 | 2.01 | 0.00 | 1.18 | 27.10 | 51.83 | 26.05 | 313.73 | 0.5432 | 397.0 | 247.5 | |
| 0.00 | 1.22 | 0.00 | 0.74 | 30.20 | 52.68 | 26.90 | 317.32 | 0.5791 | -771.0 | -654.5 | |
| 0.00 | 2.97 | 0.00 | 1.75 | 27.45 | 51.85 | 26.07 | 314.24 | 0.5464 | 44.0 | 60.1 | |
| 4.27 | 19.28 | 2.53 | 11.44 | 27.84 | 51.91 | 26.13 | 314.75 | 0.5505 | 580.9 | -78.4 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 28.23 | 51.93 | 26.16 | 315.28 | 0.5542 | -725.0 | -604.0 | |
| 0.00 | 1.66 | 0.00 | 0.98 | 27.30 | 51.66 | 25.88 | 314.20 | 0.5431 | -356.0 | -310.5 | |
| 0.00 | 2.70 | 0.00 | 1.64 | 30.47 | 52.45 | 26.67 | 317.91 | 0.5793 | -791.0 | -689.9 | |
| 0.00 | 1.48 | 0.00 | 0.90 | 30.42 | 52.16 | 26.38 | 318.11 | 0.5761 | -753.0 | -621.6 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 27.78 | 51.03 | 25.25 | 315.53 | 0.5409 | -738.0 | -614.2 | |
| 0.00 | 1.66 | 0.00 | 0.92 | 20.90 | 47.79 | 22.02 | 307.54 | 0.4435 | 775.0 | 605.8 | |
| 0.00 | 1.57 | 0.00 | 0.88 | 23.76 | 48.24 | 22.47 | 312.20 | 0.4740 | 784.0 | 575.6 | |
| 0.00 | 3.23 | 0.00 | 1.82 | 24.04 | 48.29 | 22.52 | 312.62 | 0.4772 | 727.0 | 484.3 | |
| 0.00 | 1.74 | 0.00 | 0.96 | 20.69 | 47.49 | 21.71 | 307.49 | 0.4380 | 750.0 | 582.4 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 24.03 | 47.66 | 21.88 | 313.35 | 0.4700 | 681.0 | 529.5 | |
| 0.00 | 2.53 | 0.00 | 1.37 | 19.06 | 45.46 | 19.69 | 306.63 | 0.3985 | 780.0 | 664.7 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 27.97 | 46.66 | 20.88 | 320.72 | 0.4993 | 702.0 | 534.4 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 26.73 | 46.13 | 20.35 | 319.56 | 0.4809 | 624.0 | 450.7 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 27.40 | 45.25 | 19.48 | 321.71 | 0.4797 | 663.0 | 514.9 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 27.31 | 44.99 | 19.21 | 321.94 | 0.4762 | 619.0 | 553.9 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 26.78 | 44.40 | 18.62 | 321.97 | 0.4647 | 613.0 | 614.0 | |
| 0.00 | 1.13 | 0.00 | 0.63 | 27.20 | 43.41 | 17.63 | 324.00 | 0.4602 | 789.0 | 549.8 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 29.98 | 40.06 | 14.28 | 332.71 | 0.4679 | 741.0 | 586.5 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 29.63 | 39.44 | 13.66 | 333.31 | 0.4589 | 613.0 | 424.1 | |
| 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. | |