SDO HMI 2011-11-22 08:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.90 | 122.85 | 21.38 | 75.56 | 17.69 | 313.27 | 33.37 | 297.81 | 0.5944 | -96.3 | -137.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.17 | 19.56 | 319.75 | 39.85 | 297.13 | 0.6807 | -482.0 | -483.0 | |
| 0.00 | 1.37 | 0.00 | 0.91 | 19.11 | 319.05 | 39.15 | 296.82 | 0.6707 | -598.0 | -549.8 | |
| 0.00 | 1.80 | 0.00 | 1.20 | 19.21 | 318.91 | 39.01 | 297.02 | 0.6696 | -848.0 | -699.2 | |
| 3.86 | 13.37 | 2.50 | 8.66 | 18.31 | 317.32 | 37.41 | 296.50 | 0.6468 | -843.0 | -356.8 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 17.21 | 316.58 | 36.68 | 295.24 | 0.6331 | -823.0 | -721.7 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 11.58 | 313.97 | 34.07 | 287.42 | 0.5773 | -782.0 | -660.1 | |
| 0.00 | 0.69 | 0.00 | 0.43 | 16.94 | 314.84 | 34.93 | 295.71 | 0.6102 | 571.0 | 451.9 | |
| 2.74 | 6.00 | 1.73 | 3.78 | 18.32 | 315.07 | 35.17 | 297.70 | 0.6198 | -726.0 | -571.9 | |
| 0.00 | 2.74 | 0.00 | 1.72 | 18.18 | 314.73 | 34.83 | 297.66 | 0.6149 | -771.0 | -629.8 | |
| 1.54 | 14.23 | 0.96 | 8.83 | 17.53 | 314.51 | 34.61 | 296.80 | 0.6090 | 345.8 | -559.8 | |
| 2.57 | 6.26 | 1.61 | 3.90 | 18.12 | 314.41 | 34.51 | 297.76 | 0.6108 | -796.6 | -768.1 | |
| 1.80 | -10.00 | 1.12 | -10.00 | 17.20 | 314.17 | 34.27 | 296.47 | 0.6032 | -891.8 | 999999 | |
| 0.00 | 2.06 | 0.00 | 1.28 | 17.75 | 314.26 | 34.35 | 297.28 | 0.6070 | -808.0 | -676.6 | |
| 0.00 | 1.46 | 0.00 | 0.90 | 18.28 | 313.88 | 33.98 | 298.32 | 0.6051 | -840.0 | -734.2 | |
| 0.00 | 1.89 | 0.00 | 1.11 | 8.38 | 312.34 | 32.43 | 282.37 | 0.5453 | -841.0 | -568.4 | |
| 0.00 | 1.46 | 0.00 | 0.89 | 16.32 | 313.44 | 33.53 | 295.50 | 0.5896 | -818.0 | -581.1 | |
| 0.00 | 2.31 | 0.00 | 1.41 | 16.11 | 313.14 | 33.23 | 295.33 | 0.5848 | -948.0 | -769.7 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 18.44 | 313.58 | 33.68 | 298.75 | 0.6022 | -746.0 | -590.2 | |
| 0.00 | 2.91 | 0.00 | 1.79 | 17.19 | 313.16 | 33.26 | 297.03 | 0.5905 | -232.0 | -201.1 | |
| 1.29 | 1.89 | 0.78 | 1.15 | 16.33 | 312.96 | 33.05 | 295.79 | 0.5835 | -733.3 | -894.9 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 16.67 | 313.02 | 33.12 | 296.29 | 0.5860 | -738.0 | -606.8 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 16.09 | 312.69 | 32.79 | 295.55 | 0.5789 | -724.0 | -589.3 | |
| 0.00 | 1.46 | 0.00 | 0.89 | 18.27 | 312.72 | 32.82 | 299.01 | 0.5907 | 686.0 | 539.6 | |
| 1.97 | 2.31 | 1.19 | 1.40 | 17.33 | 312.08 | 32.18 | 297.92 | 0.5776 | -824.5 | -621.2 | |
| 0.00 | 1.29 | 0.00 | 0.78 | 18.25 | 312.12 | 32.22 | 299.37 | 0.5832 | 468.0 | 331.3 | |
| 0.00 | 2.14 | 0.00 | 1.30 | 18.23 | 311.82 | 31.92 | 299.52 | 0.5794 | 822.0 | 587.3 | |
| 3.43 | 37.21 | 2.07 | 22.38 | 18.30 | 311.25 | 31.35 | 300.02 | 0.5727 | 596.3 | 597.9 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 18.03 | 311.09 | 31.18 | 299.69 | 0.5690 | -96.0 | -125.9 | |
| 2.23 | 3.86 | 1.32 | 2.28 | 15.76 | 310.60 | 30.70 | 296.27 | 0.5501 | 671.0 | 607.5 | |
| 10.29 | -27.00 | 6.20 | -27.00 | 18.55 | 311.01 | 31.11 | 300.59 | 0.5712 | 944.5 | 999999 | |
| 1.89 | -27.00 | 1.13 | -27.00 | 18.34 | 310.78 | 30.88 | 300.41 | 0.5671 | 834.3 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 16.01 | 310.32 | 30.42 | 296.88 | 0.5477 | 722.0 | 534.5 | |
| 1.29 | 3.17 | 0.77 | 1.90 | 18.03 | 310.62 | 30.71 | 300.03 | 0.5631 | 553.9 | 519.8 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 18.94 | 310.36 | 30.46 | 301.67 | 0.5655 | -489.0 | -377.6 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 12.45 | 307.10 | 27.19 | 292.53 | 0.4851 | 777.0 | 664.4 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 17.22 | 307.58 | 27.68 | 300.97 | 0.5196 | 688.0 | 534.5 | |
| 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. | |