SDO HMI 2011-10-20 14:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.53 | 28.15 | 4.72 | 15.37 | -15.50 | 4.86 | 13.14 | 211.41 | 0.4194 | 144.0 | 27.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.48 | 0.00 | 0.81 | -14.62 | 6.85 | 15.13 | 216.59 | 0.4255 | 644.0 | 493.6 | |
| 0.00 | 1.31 | 0.00 | 0.73 | -17.31 | 6.77 | 15.05 | 212.85 | 0.4589 | 620.0 | 485.5 | |
| 0.00 | 1.39 | 0.00 | 0.77 | -15.79 | 6.39 | 14.67 | 214.14 | 0.4361 | 838.0 | 671.2 | |
| 5.92 | 7.23 | 3.27 | 4.00 | -16.65 | 6.33 | 14.61 | 212.90 | 0.4467 | 937.2 | 614.1 | |
| 0.00 | 1.48 | 0.00 | 0.81 | -14.73 | 6.19 | 14.47 | 215.22 | 0.4207 | 886.0 | 835.5 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -16.30 | 6.24 | 14.52 | 213.19 | 0.4413 | 543.0 | 336.8 | |
| 2.61 | 3.40 | 1.45 | 1.89 | -17.52 | 6.14 | 14.42 | 211.49 | 0.4564 | -930.6 | -814.7 | |
| 0.00 | 1.65 | 0.00 | 0.91 | -16.03 | 6.00 | 14.27 | 213.09 | 0.4358 | 733.0 | 638.7 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -15.06 | 4.12 | 12.39 | 210.74 | 0.4072 | 758.0 | 571.5 | |
| 0.00 | 1.92 | 0.00 | 1.03 | -14.86 | 1.99 | 10.27 | 206.48 | 0.3881 | -800.0 | -402.3 | |
| 0.00 | 1.48 | 0.00 | 0.79 | -13.06 | 1.91 | 10.19 | 208.59 | 0.3617 | -793.0 | -583.7 | |
| 0.00 | 2.53 | 0.00 | 1.34 | -13.08 | 1.66 | 9.94 | 207.97 | 0.3601 | -989.0 | -713.0 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -12.92 | 1.32 | 9.59 | 207.35 | 0.3551 | -753.0 | -629.7 | |
| 0.00 | 1.22 | 0.00 | 0.65 | -13.49 | 1.21 | 9.49 | 206.37 | 0.3626 | -995.0 | -838.7 | |
| 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. | |