SDO HMI 2011-10-10 01:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.65 | 210.62 | 21.82 | 118.63 | 23.48 | 154.16 | 23.39 | 310.04 | 0.4776 | -573.3 | -309.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.85 | 190.63 | 5.00 | 107.60 | 23.07 | 155.03 | 24.27 | 308.26 | 0.4835 | -1023.1 | -410.2 | |
| 0.00 | 1.23 | 0.00 | 0.71 | 26.71 | 155.40 | 24.64 | 313.90 | 0.5189 | -734.0 | -568.5 | |
| 29.80 | -1.00 | 16.82 | -1.00 | 23.31 | 154.65 | 23.88 | 309.07 | 0.4809 | -1273.5 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.88 | 22.22 | 153.56 | 22.80 | 308.27 | 0.4589 | 568.0 | 379.8 | |
| 0.00 | 1.40 | 0.00 | 0.80 | 26.61 | 153.95 | 23.19 | 315.30 | 0.5025 | -620.0 | -428.7 | |
| 0.00 | 2.02 | 0.00 | 1.12 | 25.56 | 150.31 | 19.54 | 318.10 | 0.4538 | 672.0 | 663.3 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 26.17 | 150.20 | 19.44 | 319.22 | 0.4592 | 743.0 | 623.6 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 23.48 | 148.11 | 17.35 | 317.72 | 0.4083 | 866.0 | 673.8 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 25.53 | 148.34 | 17.58 | 320.85 | 0.4335 | 790.0 | 554.2 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 26.04 | 148.31 | 17.55 | 321.70 | 0.4391 | 647.0 | 502.5 | |
| 0.00 | 1.84 | 0.00 | 1.01 | 25.83 | 148.00 | 17.24 | 321.84 | 0.4336 | 856.0 | 732.1 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 30.61 | 147.51 | 16.75 | 329.22 | 0.4866 | 630.0 | 498.7 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 26.10 | 146.48 | 15.72 | 324.67 | 0.4224 | 760.0 | 583.2 | |
| 0.00 | 4.38 | 0.00 | 2.38 | 26.14 | 144.86 | 14.10 | 327.49 | 0.4086 | 774.0 | 772.9 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 24.30 | 142.09 | 11.32 | 330.14 | 0.3610 | 621.0 | 489.9 | |
| 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. | |