SDO HMI 2011-10-17 02:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 86.96 | 639.39 | 48.77 | 358.03 | 27.38 | 55.99 | 18.12 | 323.69 | 0.4672 | -949.9 | -397.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.71 | 0.00 | 1.55 | 28.67 | 58.32 | 20.45 | 322.18 | 0.5020 | 645.0 | 628.1 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 29.77 | 57.82 | 19.95 | 324.30 | 0.5096 | 817.0 | 608.8 | |
| 1.57 | 587.22 | 0.89 | 329.35 | 27.70 | 57.16 | 19.29 | 322.32 | 0.4805 | -817.4 | -431.5 | |
| 0.79 | -3.00 | 0.44 | -3.00 | 26.65 | 56.79 | 18.92 | 321.28 | 0.4653 | -1297.6 | 999999 | |
| 84.60 | -3.00 | 47.44 | -3.00 | 27.33 | 56.52 | 18.65 | 322.66 | 0.4704 | -1508.1 | 999999 | |
| 0.00 | 1.57 | 0.00 | 0.90 | 30.08 | 56.06 | 18.19 | 327.03 | 0.4983 | -637.0 | -452.1 | |
| 0.00 | 1.13 | 0.00 | 0.63 | 27.30 | 54.36 | 16.50 | 325.77 | 0.4505 | -975.0 | -804.7 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 27.53 | 54.26 | 16.39 | 326.25 | 0.4523 | -479.0 | -377.0 | |
| 0.00 | 1.40 | 0.00 | 0.81 | 32.01 | 55.00 | 17.13 | 330.76 | 0.5133 | -693.0 | -557.5 | |
| 0.00 | 1.92 | 0.00 | 1.06 | 27.58 | 53.53 | 15.66 | 327.46 | 0.4468 | -889.0 | -600.0 | |
| 0.00 | 1.57 | 0.00 | 0.91 | 32.63 | 54.23 | 16.36 | 332.49 | 0.5156 | -789.0 | -505.2 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 29.79 | 53.59 | 15.72 | 330.20 | 0.4751 | -754.0 | -611.0 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 30.68 | 53.73 | 15.87 | 331.03 | 0.4874 | -591.0 | -572.8 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 27.01 | 53.03 | 15.16 | 327.49 | 0.4354 | -686.0 | -570.2 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 27.78 | 53.14 | 15.27 | 328.36 | 0.4461 | -949.0 | -764.3 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 29.27 | 53.36 | 15.49 | 329.91 | 0.4668 | -725.0 | -590.5 | |
| 0.00 | 2.62 | 0.00 | 1.46 | 29.01 | 53.25 | 15.38 | 329.77 | 0.4626 | -890.0 | -697.7 | |
| 0.00 | 2.01 | 0.00 | 1.12 | 29.32 | 52.94 | 15.07 | 330.62 | 0.4641 | -877.0 | -687.2 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 27.77 | 52.40 | 14.53 | 329.55 | 0.4400 | -777.0 | -676.4 | |
| 0.00 | 1.13 | 0.00 | 0.62 | 27.58 | 52.34 | 14.47 | 329.40 | 0.4370 | -895.0 | -716.5 | |
| 0.00 | 1.48 | 0.00 | 0.82 | 27.84 | 52.20 | 14.33 | 329.97 | 0.4393 | -944.0 | -854.6 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 28.07 | 51.92 | 14.05 | 330.74 | 0.4401 | -751.0 | -580.9 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 29.47 | 51.90 | 14.03 | 332.46 | 0.4584 | -898.0 | -722.2 | |
| 0.00 | 1.48 | 0.00 | 0.83 | 29.48 | 51.55 | 13.68 | 333.04 | 0.4560 | -838.0 | -755.6 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 26.95 | 50.22 | 12.36 | 332.32 | 0.4123 | -897.0 | -734.5 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 23.42 | 46.95 | 9.08 | 334.57 | 0.3388 | 724.0 | 586.6 | |
| 0.00 | 4.71 | 0.00 | 2.52 | 27.00 | 44.95 | 7.09 | 343.16 | 0.3809 | 678.0 | 591.0 | |
| 0.00 | 2.01 | 0.00 | 1.07 | 26.91 | 44.54 | 6.68 | 344.00 | 0.3777 | 694.0 | 622.3 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 28.46 | 44.40 | 6.53 | 345.49 | 0.4009 | 425.0 | 345.8 | |
| 0.00 | 2.44 | 0.00 | 1.29 | 25.23 | 43.52 | 5.65 | 345.06 | 0.3470 | 881.0 | 732.8 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 22.53 | 42.49 | 4.62 | 345.55 | 0.2997 | 842.0 | 605.3 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 25.97 | 42.09 | 4.22 | 349.18 | 0.3536 | 798.0 | 585.4 | |
| 0.00 | 1.48 | 0.00 | 0.79 | 26.68 | 41.61 | 3.74 | 350.73 | 0.3636 | 828.0 | 635.1 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 29.03 | 41.59 | 3.72 | 351.84 | 0.4011 | 720.0 | 572.8 | |
| 0.00 | 1.75 | 0.00 | 0.94 | 28.51 | 41.47 | 3.60 | 351.89 | 0.3926 | 904.0 | 672.8 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 29.20 | 39.57 | 1.70 | 356.27 | 0.4005 | 654.0 | 596.9 | |
| 0.00 | 1.57 | 0.00 | 0.84 | 27.17 | 38.50 | 0.63 | 358.46 | 0.3668 | 895.0 | 709.5 | |
| 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. | |