SDO HMI 2011-10-18 05:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 92.50 | 574.67 | 58.01 | 359.82 | 27.47 | 55.24 | 32.20 | 309.26 | 0.6122 | -849.6 | -316.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.13 | 494.02 | 0.72 | 311.44 | 27.91 | 56.40 | 33.37 | 308.96 | 0.6273 | -664.6 | -339.8 | |
| 1.05 | -1.00 | 0.66 | -1.00 | 28.14 | 56.24 | 33.21 | 309.40 | 0.6272 | -540.8 | 999999 | |
| 78.63 | -1.00 | 49.50 | -1.00 | 27.44 | 55.96 | 32.92 | 308.60 | 0.6195 | -1366.4 | 999999 | |
| 0.00 | 2.01 | 0.00 | 1.24 | 26.83 | 54.49 | 31.46 | 308.78 | 0.5996 | -784.0 | -686.7 | |
| 1.22 | 2.88 | 0.75 | 1.77 | 26.72 | 54.18 | 31.15 | 308.85 | 0.5954 | -831.6 | -766.8 | |
| 3.23 | 8.29 | 1.98 | 5.09 | 26.77 | 53.80 | 30.77 | 309.20 | 0.5917 | -1010.9 | -738.9 | |
| 0.00 | 1.40 | 0.00 | 0.85 | 25.76 | 53.39 | 30.36 | 308.02 | 0.5800 | -694.0 | -547.5 | |
| 0.00 | 1.22 | 0.00 | 0.79 | 32.20 | 55.29 | 32.26 | 315.51 | 0.6468 | -654.0 | -559.0 | |
| 0.87 | 3.14 | 0.53 | 1.92 | 27.42 | 53.06 | 30.03 | 310.73 | 0.5884 | -989.9 | -753.4 | |
| 0.00 | 5.59 | 0.00 | 3.42 | 27.74 | 53.12 | 30.09 | 311.15 | 0.5915 | -961.0 | -686.0 | |
| 0.00 | 0.96 | 0.00 | 0.61 | 30.79 | 54.10 | 31.06 | 314.58 | 0.6246 | -632.0 | -505.6 | |
| 0.00 | 1.66 | 0.00 | 1.05 | 30.70 | 53.82 | 30.79 | 314.68 | 0.6212 | -712.0 | -626.3 | |
| 0.00 | 1.13 | 0.00 | 0.72 | 31.20 | 53.80 | 30.76 | 315.36 | 0.6249 | -624.0 | -495.5 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 28.36 | 52.34 | 29.30 | 312.68 | 0.5880 | -931.0 | -748.1 | |
| 2.18 | 19.29 | 1.33 | 11.72 | 28.21 | 52.17 | 29.14 | 312.59 | 0.5851 | -497.3 | -125.7 | |
| 0.00 | 1.48 | 0.00 | 0.90 | 27.68 | 51.71 | 28.67 | 312.22 | 0.5760 | 350.0 | 309.2 | |
| 4.19 | -15.00 | 2.54 | -15.00 | 27.97 | 51.75 | 28.72 | 312.60 | 0.5788 | 703.1 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.76 | 30.76 | 52.59 | 29.56 | 315.75 | 0.6098 | -536.0 | -575.3 | |
| 0.00 | 1.92 | 0.00 | 1.19 | 30.70 | 52.41 | 29.38 | 315.82 | 0.6076 | -949.0 | -804.1 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 27.17 | 51.34 | 28.30 | 311.81 | 0.5681 | -612.0 | -522.9 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 27.38 | 51.13 | 28.09 | 312.29 | 0.5674 | -703.0 | -529.1 | |
| 0.00 | 1.75 | 0.00 | 1.05 | 27.99 | 51.22 | 28.19 | 313.10 | 0.5734 | -776.0 | -607.3 | |
| 0.00 | 1.57 | 0.00 | 0.93 | 27.39 | 50.06 | 27.03 | 313.27 | 0.5563 | -825.0 | -707.3 | |
| 0.00 | 1.48 | 0.00 | 0.85 | 23.76 | 48.21 | 25.18 | 309.35 | 0.5056 | 647.0 | 550.4 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 23.58 | 48.00 | 24.96 | 309.26 | 0.5016 | 798.0 | 668.1 | |
| 0.00 | 4.54 | 0.00 | 2.60 | 23.99 | 48.08 | 25.04 | 309.86 | 0.5059 | 546.0 | 539.1 | |
| 0.00 | 1.66 | 0.00 | 0.94 | 23.47 | 47.54 | 24.51 | 309.54 | 0.4954 | 689.0 | 550.1 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 26.77 | 45.12 | 22.08 | 317.53 | 0.4992 | 719.0 | 551.2 | |
| 0.00 | 1.75 | 0.00 | 1.00 | 27.04 | 44.99 | 21.96 | 318.08 | 0.5005 | 694.0 | 593.2 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 24.76 | 44.37 | 21.34 | 315.25 | 0.4713 | 674.0 | 560.1 | |
| 0.00 | 2.44 | 0.00 | 1.39 | 26.87 | 44.31 | 21.27 | 318.65 | 0.4919 | 544.0 | 425.6 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 28.44 | 42.81 | 19.78 | 322.82 | 0.4944 | 778.0 | 632.5 | |
| 0.00 | 2.01 | 0.00 | 1.14 | 30.03 | 39.90 | 16.86 | 328.89 | 0.4882 | 670.0 | 530.3 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 28.56 | 39.47 | 16.44 | 327.68 | 0.4667 | 800.0 | 632.8 | |
| 0.00 | 3.93 | 0.00 | 2.19 | 28.12 | 39.19 | 16.16 | 327.52 | 0.4589 | 755.0 | 556.5 | |
| 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. | |