SDO HMI 2011-10-10 18:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.38 | 183.83 | 18.62 | 112.09 | 23.46 | 153.84 | 32.41 | 302.54 | 0.5853 | -540.4 | -317.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.22 | 167.29 | 3.82 | 102.50 | 23.06 | 154.80 | 33.37 | 301.20 | 0.5939 | -905.4 | -406.2 | |
| 2.45 | -1.00 | 1.50 | -1.00 | 22.73 | 154.63 | 33.20 | 300.77 | 0.5900 | -704.7 | 999999 | |
| 21.18 | -1.00 | 12.98 | -1.00 | 23.33 | 154.45 | 33.02 | 301.83 | 0.5912 | -1191.7 | 999999 | |
| 0.53 | -1.00 | 0.32 | -1.00 | 23.14 | 154.00 | 32.58 | 301.80 | 0.5848 | -1398.5 | 999999 | |
| 0.00 | 1.75 | 0.00 | 1.06 | 25.90 | 151.76 | 30.34 | 307.63 | 0.5759 | -666.0 | -542.5 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 23.05 | 150.90 | 29.47 | 303.77 | 0.5468 | 431.0 | 469.4 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 26.20 | 150.24 | 28.81 | 309.30 | 0.5609 | 726.0 | 581.7 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 25.82 | 147.99 | 26.57 | 310.68 | 0.5330 | 800.0 | 628.5 | |
| 0.00 | 1.75 | 0.00 | 1.02 | 25.90 | 147.61 | 26.18 | 311.18 | 0.5293 | 669.0 | 534.1 | |
| 0.00 | 2.01 | 0.00 | 1.15 | 26.07 | 145.14 | 23.72 | 313.94 | 0.5038 | 634.0 | 454.5 | |
| 0.00 | 1.75 | 0.00 | 1.00 | 25.80 | 144.80 | 23.37 | 313.88 | 0.4975 | 897.0 | 723.0 | |
| 0.00 | 2.98 | 0.00 | 1.70 | 26.44 | 144.71 | 23.29 | 314.99 | 0.5026 | 761.0 | 660.3 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 25.88 | 144.45 | 23.02 | 314.39 | 0.4944 | 826.0 | 539.6 | |
| 0.00 | 2.10 | 0.00 | 1.20 | 26.83 | 144.62 | 23.19 | 315.71 | 0.5052 | 746.0 | 524.2 | |
| 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. | |