SDO HMI 2011-11-13 23:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.31 | 260.45 | 17.53 | 145.88 | 28.16 | 42.77 | 12.49 | 335.93 | 0.4688 | -878.0 | -445.2 | |
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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 | 0.50 | 26.06 | 52.36 | 22.08 | 319.46 | 0.5215 | -600.0 | -569.9 | |
| 0.00 | 1.38 | 0.00 | 0.80 | 29.72 | 49.11 | 18.82 | 328.19 | 0.5337 | -611.0 | -484.8 | |
| 0.00 | 2.24 | 0.00 | 1.30 | 29.16 | 48.82 | 18.54 | 327.92 | 0.5248 | -725.0 | -644.6 | |
| 0.00 | 0.52 | 0.00 | 0.30 | 32.28 | 44.94 | 14.66 | 336.42 | 0.5368 | -478.0 | -611.7 | |
| 8.77 | 244.79 | 4.92 | 137.10 | 28.32 | 43.03 | 12.75 | 335.61 | 0.4723 | -1103.3 | -470.3 | |
| 0.95 | -5.00 | 0.53 | -5.00 | 28.61 | 42.96 | 12.68 | 336.01 | 0.4759 | -581.2 | 999999 | |
| 17.03 | -5.00 | 9.53 | -5.00 | 27.96 | 42.85 | 12.56 | 335.55 | 0.4662 | -1371.8 | 999999 | |
| 3.27 | -5.00 | 1.83 | -5.00 | 28.49 | 42.50 | 12.21 | 336.66 | 0.4713 | -909.7 | 999999 | |
| 1.29 | -5.00 | 0.72 | -5.00 | 28.23 | 42.47 | 12.18 | 336.46 | 0.4675 | -1026.7 | 999999 | |
| 0.00 | 3.87 | 0.00 | 2.18 | 29.83 | 40.05 | 9.76 | 341.96 | 0.4770 | -780.0 | -697.6 | |
| 0.00 | 3.44 | 0.00 | 1.88 | 27.13 | 36.74 | 6.45 | 346.25 | 0.4225 | 583.0 | 643.0 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 25.48 | 36.38 | 6.09 | 345.92 | 0.3957 | 848.0 | 734.2 | |
| 0.00 | 2.32 | 0.00 | 1.26 | 26.90 | 36.36 | 6.07 | 346.89 | 0.4176 | 561.0 | 551.1 | |
| 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. | |