SDO HMI 2011-11-09 01:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.09 | 562.36 | 54.79 | 327.84 | -13.68 | 121.88 | 26.77 | 236.44 | 0.5270 | 639.0 | 310.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.65 | -6.33 | 124.68 | 29.57 | 251.51 | 0.5192 | 654.0 | 504.2 | |
| 1.38 | 315.00 | 0.83 | 187.86 | -15.07 | 124.01 | 28.90 | 236.21 | 0.5637 | 485.2 | 369.0 | |
| 48.72 | -2.00 | 29.05 | -2.00 | -15.12 | 123.56 | 28.45 | 235.73 | 0.5587 | 1216.1 | 999999 | |
| 1.90 | 2.85 | 1.11 | 1.67 | -13.69 | 122.53 | 27.42 | 237.05 | 0.5353 | 901.9 | 520.8 | |
| 0.00 | 1.64 | 0.00 | 0.96 | -14.80 | 122.26 | 27.15 | 235.02 | 0.5406 | 788.0 | 650.1 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -13.51 | 121.85 | 26.75 | 236.70 | 0.5256 | 702.0 | 547.7 | |
| 0.00 | 1.81 | 0.00 | 1.06 | -15.64 | 121.03 | 25.92 | 232.49 | 0.5329 | 820.0 | 639.9 | |
| 29.66 | 167.20 | 16.83 | 94.95 | -11.22 | 120.42 | 25.31 | 239.25 | 0.4900 | 1193.4 | 348.6 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -7.42 | 119.76 | 24.65 | 245.88 | 0.4551 | 826.0 | 674.2 | |
| 2.33 | 10.18 | 1.31 | 5.71 | -10.76 | 119.51 | 24.40 | 239.17 | 0.4747 | 895.8 | 749.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -10.67 | 119.44 | 24.33 | 239.27 | 0.4730 | 491.0 | 596.6 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -10.47 | 118.83 | 23.72 | 239.01 | 0.4633 | 789.0 | 598.1 | |
| 1.47 | 2.33 | 0.84 | 1.33 | -14.90 | 119.24 | 24.13 | 231.72 | 0.5053 | 830.6 | 692.5 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -16.00 | 119.10 | 23.99 | 229.84 | 0.5136 | 725.0 | 651.7 | |
| 0.00 | 2.33 | 0.00 | 1.31 | -12.55 | 118.58 | 23.47 | 234.94 | 0.4770 | 857.0 | 677.4 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -13.05 | 118.60 | 23.49 | 234.09 | 0.4814 | -501.0 | -412.6 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -9.87 | 118.22 | 23.11 | 239.51 | 0.4507 | 731.0 | 530.5 | |
| 0.00 | 0.43 | 0.00 | 0.24 | -13.11 | 118.47 | 23.36 | 233.85 | 0.4803 | -572.0 | -422.4 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -9.96 | 118.00 | 22.89 | 239.10 | 0.4483 | 934.0 | 717.6 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -13.10 | 118.07 | 22.96 | 233.40 | 0.4753 | -902.0 | -769.7 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -10.32 | 117.60 | 22.49 | 237.96 | 0.4458 | 826.0 | 590.2 | |
| 0.00 | 0.52 | 0.00 | 0.28 | -8.94 | 117.50 | 22.39 | 240.58 | 0.4338 | 688.0 | 579.8 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -13.50 | 117.85 | 22.74 | 232.45 | 0.4760 | -772.0 | -694.8 | |
| 0.00 | 9.05 | 0.00 | 5.10 | -13.99 | 117.76 | 22.66 | 231.51 | 0.4795 | -742.0 | -691.0 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -13.49 | 117.68 | 22.57 | 232.26 | 0.4740 | -678.0 | -541.8 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -6.39 | 117.16 | 22.06 | 245.68 | 0.4113 | 669.0 | 424.5 | |
| 0.00 | 2.67 | 0.00 | 1.51 | -14.43 | 117.71 | 22.60 | 230.72 | 0.4829 | -682.0 | -581.8 | |
| 1.38 | 5.00 | 0.76 | 2.77 | -10.83 | 117.21 | 22.10 | 236.53 | 0.4449 | 902.7 | 805.4 | |
| 4.23 | 5.00 | 2.37 | 2.81 | -14.01 | 117.30 | 22.19 | 230.91 | 0.4742 | -973.1 | -817.6 | |
| 0.00 | 1.55 | 0.00 | 0.87 | -14.47 | 117.02 | 21.91 | 229.79 | 0.4751 | -697.0 | -489.8 | |
| 0.00 | 4.14 | 0.00 | 2.33 | -14.85 | 117.03 | 21.92 | 229.17 | 0.4788 | -750.0 | -610.1 | |
| 3.02 | 5.60 | 1.69 | 3.14 | -14.22 | 116.89 | 21.79 | 230.05 | 0.4713 | -886.5 | -823.4 | |
| 0.00 | 2.07 | 0.00 | 1.16 | -14.90 | 116.80 | 21.69 | 228.79 | 0.4767 | -847.0 | -677.8 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -13.12 | 116.46 | 21.35 | 231.39 | 0.4557 | -838.0 | -638.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -13.13 | 112.74 | 17.63 | 226.01 | 0.4117 | -733.0 | -624.2 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -15.45 | 109.69 | 14.58 | 216.81 | 0.4066 | -910.0 | -674.0 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -15.76 | 109.39 | 14.28 | 215.79 | 0.4077 | -730.0 | -592.9 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -14.12 | 108.52 | 13.41 | 216.65 | 0.3785 | -848.0 | -586.5 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -13.35 | 104.71 | 9.60 | 209.19 | 0.3341 | -688.0 | -571.2 | |
| 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. | |