SDO HMI 2011-11-14 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.33 | 316.78 | 32.15 | 202.06 | 16.13 | 63.80 | 37.35 | 292.22 | 0.6319 | -892.0 | -325.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.01 | 304.39 | 30.68 | 194.49 | 16.04 | 64.02 | 37.57 | 291.97 | 0.6342 | -1211.5 | -345.0 | |
| 0.00 | 1.29 | 0.00 | 0.84 | 18.97 | 64.67 | 38.21 | 296.07 | 0.6536 | -783.0 | -618.7 | |
| 1.98 | -1.00 | 1.25 | -1.00 | 15.72 | 63.45 | 36.99 | 291.72 | 0.6258 | -1225.8 | 999999 | |
| 0.34 | -1.00 | 0.22 | -1.00 | 16.09 | 63.26 | 36.80 | 292.37 | 0.6248 | -839.8 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.70 | 14.96 | 62.56 | 36.11 | 290.88 | 0.6117 | -829.0 | -639.8 | |
| 0.00 | 1.46 | 0.00 | 0.91 | 15.88 | 62.33 | 35.88 | 292.44 | 0.6121 | -781.0 | -606.7 | |
| 0.00 | 1.03 | 0.00 | 0.65 | 17.98 | 61.60 | 35.15 | 296.08 | 0.6119 | -660.0 | -563.2 | |
| 0.00 | 1.29 | 0.00 | 0.79 | 18.88 | 59.46 | 33.01 | 298.68 | 0.5898 | 488.0 | 416.3 | |
| 0.00 | 1.38 | 0.00 | 0.82 | 18.72 | 57.10 | 30.65 | 299.96 | 0.5594 | 715.0 | 557.1 | |
| 0.00 | 1.98 | 0.00 | 1.18 | 18.20 | 56.92 | 30.47 | 299.22 | 0.5542 | 827.0 | 688.4 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 21.33 | 56.26 | 29.81 | 304.75 | 0.5658 | 708.0 | 542.7 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 22.43 | 55.01 | 28.56 | 307.49 | 0.5590 | 819.0 | 691.5 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 21.71 | 54.67 | 28.22 | 306.66 | 0.5498 | 734.0 | 540.2 | |
| 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. | |