SDO HMI 2011-11-13 02:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.75 | 417.45 | 27.33 | 229.06 | 16.16 | 64.07 | 22.25 | 302.33 | 0.4324 | -789.7 | -392.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.48 | 14.42 | 66.18 | 24.35 | 296.68 | 0.4488 | -584.0 | -533.1 | |
| 49.75 | 395.76 | 27.33 | 217.34 | 16.04 | 64.32 | 22.50 | 301.75 | 0.4343 | -1412.9 | -430.6 | |
| 0.00 | 3.01 | 0.00 | 1.68 | 18.80 | 64.45 | 22.63 | 306.98 | 0.4578 | -283.0 | -431.6 | |
| 0.00 | 2.58 | 0.00 | 1.41 | 17.42 | 62.42 | 20.60 | 306.72 | 0.4206 | -878.0 | -685.2 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 14.36 | 61.67 | 19.85 | 301.06 | 0.3856 | -748.0 | -599.9 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 17.99 | 59.71 | 17.89 | 311.58 | 0.3922 | 713.0 | 570.7 | |
| 0.00 | 2.24 | 0.00 | 1.21 | 18.55 | 59.64 | 17.82 | 312.78 | 0.3970 | 892.0 | 727.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 18.21 | 59.31 | 17.49 | 312.64 | 0.3897 | 870.0 | 734.2 | |
| 0.00 | 2.07 | 0.00 | 1.10 | 17.87 | 57.58 | 15.76 | 314.79 | 0.3658 | 909.0 | 715.9 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 18.55 | 57.58 | 15.76 | 316.14 | 0.3732 | 874.0 | 550.0 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.09 | 56.83 | 15.01 | 314.47 | 0.3485 | 851.0 | 735.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 21.61 | 56.08 | 14.26 | 324.30 | 0.3941 | 915.0 | 704.7 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 20.75 | 54.72 | 12.90 | 325.54 | 0.3706 | 964.0 | 768.9 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 21.04 | 54.00 | 12.18 | 327.48 | 0.3679 | 746.0 | 663.2 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 19.37 | 50.26 | 8.43 | 333.73 | 0.3140 | 736.0 | 574.1 | |
| 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. | |