SDO HMI 2011-09-01 20:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.67 | 420.07 | 58.50 | 240.06 | 24.50 | 300.27 | 25.15 | 308.96 | 0.4986 | -19.2 | -31.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.56 | 207.40 | 15.48 | 120.82 | 23.46 | 303.55 | 28.43 | 303.94 | 0.5284 | -1085.3 | -333.4 | |
| 6.35 | -1.00 | 3.69 | -1.00 | 23.09 | 303.43 | 28.30 | 303.39 | 0.5244 | -1315.5 | 999999 | |
| 2.15 | -1.00 | 1.25 | -1.00 | 24.01 | 303.42 | 28.29 | 304.97 | 0.5304 | -745.5 | 999999 | |
| 3.22 | -1.00 | 1.87 | -1.00 | 23.73 | 303.17 | 28.04 | 304.71 | 0.5255 | -1083.6 | 999999 | |
| 1.70 | 4.02 | 0.99 | 2.35 | 24.68 | 303.39 | 28.27 | 306.11 | 0.5347 | -773.6 | -644.7 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 25.78 | 303.68 | 28.55 | 307.68 | 0.5459 | 812.0 | 624.4 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 20.56 | 302.41 | 27.29 | 299.63 | 0.4958 | -878.0 | -741.4 | |
| 7.78 | -1.00 | 4.51 | -1.00 | 23.69 | 302.86 | 27.73 | 304.88 | 0.5214 | -1164.7 | 999999 | |
| 0.00 | 1.70 | 0.00 | 1.00 | 25.52 | 303.15 | 28.03 | 307.69 | 0.5379 | 758.0 | 550.4 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 24.45 | 302.89 | 27.76 | 306.14 | 0.5271 | -680.0 | -504.7 | |
| 0.00 | 5.01 | 0.00 | 2.90 | 24.38 | 302.46 | 27.33 | 306.38 | 0.5215 | -681.0 | -658.4 | |
| 0.00 | 1.88 | 0.00 | 1.08 | 23.36 | 301.93 | 26.80 | 305.07 | 0.5078 | -939.0 | -777.2 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 24.24 | 302.09 | 26.96 | 306.46 | 0.5160 | -739.0 | -504.3 | |
| 1.70 | 8.14 | 0.98 | 4.67 | 24.37 | 301.45 | 26.32 | 307.24 | 0.5094 | -865.7 | -663.2 | |
| 1.16 | -14.00 | 0.67 | -14.00 | 24.45 | 301.21 | 26.08 | 307.59 | 0.5071 | -843.4 | 999999 | |
| 0.00 | 6.53 | 0.00 | 3.69 | 23.47 | 299.83 | 24.70 | 307.17 | 0.4830 | 843.0 | 489.9 | |
| 3.94 | 11.36 | 2.24 | 6.47 | 24.90 | 299.87 | 24.74 | 309.63 | 0.4949 | -917.5 | -579.7 | |
| 0.00 | 6.80 | 0.00 | 3.88 | 25.41 | 299.79 | 24.67 | 310.58 | 0.4983 | -783.0 | -658.3 | |
| 2.06 | 5.19 | 1.16 | 2.93 | 23.81 | 299.35 | 24.22 | 308.25 | 0.4799 | 872.3 | 694.6 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 24.04 | 299.11 | 23.98 | 308.91 | 0.4789 | 570.0 | 467.6 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 24.35 | 298.69 | 23.57 | 309.88 | 0.4766 | 575.0 | 456.4 | |
| 1.07 | 1.16 | 0.60 | 0.65 | 24.56 | 298.16 | 23.03 | 310.83 | 0.4722 | 579.5 | 689.0 | |
| 2.77 | 5.63 | 1.55 | 3.15 | 24.96 | 297.26 | 22.13 | 312.53 | 0.4654 | 813.7 | 542.3 | |
| 4.56 | 6.44 | 2.55 | 3.59 | 25.10 | 296.93 | 21.80 | 313.17 | 0.4630 | 964.8 | 447.5 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 25.40 | 296.66 | 21.53 | 314.00 | 0.4628 | 836.0 | 682.4 | |
| 2.95 | 30.50 | 1.66 | 17.15 | 26.84 | 296.61 | 21.49 | 316.46 | 0.4764 | 787.2 | 379.0 | |
| 8.41 | -26.00 | 4.72 | -26.00 | 26.66 | 296.43 | 21.30 | 316.38 | 0.4726 | 1026.8 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.80 | 26.21 | 296.31 | 21.18 | 315.80 | 0.4669 | 604.0 | 480.4 | |
| 0.00 | 3.67 | 0.00 | 2.04 | 25.81 | 295.98 | 20.85 | 315.54 | 0.4594 | 831.0 | 621.4 | |
| 1.61 | 4.65 | 0.90 | 2.61 | 26.78 | 295.94 | 20.82 | 317.17 | 0.4687 | 823.8 | 588.5 | |
| 0.00 | 3.13 | 0.00 | 1.75 | 26.66 | 295.70 | 20.58 | 317.28 | 0.4650 | 1027.0 | 849.1 | |
| 0.00 | 3.49 | 0.00 | 1.95 | 27.07 | 295.75 | 20.62 | 317.90 | 0.4697 | 119.0 | 105.8 | |
| 24.68 | 87.82 | 13.68 | 48.62 | 25.68 | 295.24 | 20.11 | 316.26 | 0.4501 | 1168.5 | 578.9 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 26.19 | 295.22 | 20.10 | 317.14 | 0.4552 | 610.0 | 497.9 | |
| 0.00 | 4.83 | 0.00 | 2.69 | 26.55 | 295.07 | 19.95 | 317.93 | 0.4573 | 726.0 | 616.2 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 25.44 | 294.16 | 19.04 | 317.29 | 0.4361 | 1043.0 | 842.5 | |
| 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. | |