SDO HMI 2011-07-05 18:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.13 | 258.68 | 33.56 | 153.76 | 17.03 | 354.26 | 31.04 | 296.50 | 0.5526 | -381.7 | -225.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.60 | 16.40 | 356.27 | 33.05 | 294.20 | 0.5758 | -47.0 | -7.5 | |
| 29.42 | 193.58 | 17.69 | 116.13 | 16.90 | 355.54 | 32.32 | 295.43 | 0.5685 | -1051.6 | -353.7 | |
| 2.00 | -2.00 | 1.20 | -2.00 | 17.41 | 355.26 | 32.04 | 296.44 | 0.5674 | -682.7 | 999999 | |
| 15.71 | -2.00 | 9.35 | -2.00 | 16.83 | 354.62 | 31.40 | 295.84 | 0.5563 | -1069.4 | 999999 | |
| 0.00 | 1.82 | 0.00 | 1.07 | 16.28 | 354.15 | 30.93 | 295.18 | 0.5473 | -822.0 | -697.2 | |
| 0.00 | 3.63 | 0.00 | 2.17 | 18.22 | 354.33 | 31.11 | 298.37 | 0.5598 | 259.0 | 17.3 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 17.44 | 354.18 | 30.96 | 297.15 | 0.5536 | -718.0 | -548.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 17.70 | 354.04 | 30.82 | 297.67 | 0.5532 | -558.0 | -381.2 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 17.07 | 353.85 | 30.63 | 296.73 | 0.5474 | -613.0 | -410.9 | |
| 3.27 | 4.99 | 1.95 | 2.98 | 18.67 | 354.08 | 30.86 | 299.27 | 0.5592 | 834.2 | 639.1 | |
| 0.00 | 1.91 | 0.00 | 1.14 | 19.19 | 353.96 | 30.74 | 300.20 | 0.5607 | -790.0 | -675.0 | |
| 1.73 | 2.45 | 1.02 | 1.45 | 18.24 | 353.66 | 30.44 | 298.84 | 0.5514 | -789.2 | -653.6 | |
| 0.00 | 1.82 | 0.00 | 1.07 | 17.05 | 353.36 | 30.14 | 297.01 | 0.5409 | -797.0 | -659.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 15.75 | 352.74 | 29.52 | 295.12 | 0.5258 | -843.0 | -656.6 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 16.54 | 352.69 | 29.47 | 296.56 | 0.5292 | -737.0 | -604.0 | |
| 4.00 | 6.63 | 2.35 | 3.90 | 18.24 | 352.77 | 29.55 | 299.45 | 0.5399 | 820.4 | 636.1 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 19.55 | 352.43 | 29.21 | 301.90 | 0.5438 | -805.0 | -703.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 19.83 | 352.41 | 29.19 | 302.39 | 0.5454 | -699.0 | -542.0 | |
| 0.00 | 2.27 | 0.00 | 1.33 | 19.05 | 352.00 | 28.78 | 301.39 | 0.5352 | -754.0 | -682.0 | |
| 0.00 | 1.82 | 0.00 | 1.05 | 19.27 | 350.94 | 27.72 | 302.61 | 0.5233 | -853.0 | -683.8 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 16.04 | 350.30 | 27.08 | 297.33 | 0.4944 | 619.0 | 504.0 | |
| 0.00 | 2.18 | 0.00 | 1.23 | 15.48 | 350.00 | 26.78 | 296.50 | 0.4872 | 659.0 | 499.4 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 15.02 | 349.76 | 26.54 | 295.79 | 0.4813 | 834.0 | 635.6 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 16.24 | 349.83 | 26.61 | 298.07 | 0.4893 | 660.0 | 583.1 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 16.27 | 349.69 | 26.47 | 298.24 | 0.4876 | 820.0 | 613.9 | |
| 0.00 | 2.00 | 0.00 | 1.12 | 14.82 | 349.10 | 25.88 | 295.89 | 0.4710 | 743.0 | 603.5 | |
| 0.00 | 1.82 | 0.00 | 1.03 | 16.66 | 349.32 | 26.10 | 299.26 | 0.4851 | 693.0 | 545.0 | |
| 0.00 | 1.73 | 0.00 | 0.97 | 17.56 | 348.32 | 25.10 | 301.83 | 0.4780 | 895.0 | 738.6 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 12.00 | 347.64 | 24.42 | 291.07 | 0.4352 | 746.0 | 546.3 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 17.72 | 348.31 | 25.09 | 302.14 | 0.4789 | 719.0 | 566.6 | |
| 0.00 | 2.45 | 0.00 | 1.37 | 17.39 | 347.77 | 24.55 | 302.01 | 0.4695 | 801.0 | 624.8 | |
| 0.00 | 3.72 | 0.00 | 2.08 | 17.65 | 347.28 | 24.06 | 302.98 | 0.4650 | 938.0 | 774.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 18.29 | 346.95 | 23.73 | 304.52 | 0.4656 | 684.0 | 612.3 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.01 | 346.18 | 22.96 | 302.86 | 0.4459 | 835.0 | 699.1 | |
| 0.00 | 3.45 | 0.00 | 1.91 | 17.11 | 345.92 | 22.70 | 303.33 | 0.4432 | 920.0 | 684.5 | |
| 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. | |