SDO HMI 2011-08-09 00:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.99 | 34.13 | 1.10 | 18.88 | -16.42 | 243.27 | 13.18 | 209.66 | 0.4449 | -128.5 | -136.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.99 | 3.79 | 1.10 | 2.10 | -14.71 | 246.40 | 16.31 | 217.47 | 0.4482 | 983.4 | 830.1 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -15.23 | 246.21 | 16.12 | 216.44 | 0.4528 | 798.0 | 740.0 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -14.96 | 245.86 | 15.77 | 216.22 | 0.4462 | 841.0 | 666.3 | |
| 0.00 | 2.26 | 0.00 | 1.25 | -14.69 | 245.78 | 15.68 | 216.43 | 0.4421 | 953.0 | 749.7 | |
| 0.00 | 4.52 | 0.00 | 2.50 | -15.88 | 245.12 | 15.02 | 213.69 | 0.4512 | 952.0 | 672.4 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -17.46 | 242.32 | 12.23 | 206.78 | 0.4504 | -776.0 | -619.6 | |
| 0.00 | 3.34 | 0.00 | 1.85 | -17.22 | 242.14 | 12.05 | 206.69 | 0.4458 | -739.0 | -620.5 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -17.05 | 241.91 | 11.81 | 206.41 | 0.4418 | -924.0 | -717.4 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -17.31 | 241.86 | 11.77 | 206.05 | 0.4451 | -776.0 | -640.0 | |
| 0.00 | 2.98 | 0.00 | 1.65 | -17.41 | 241.64 | 11.54 | 205.53 | 0.4450 | -611.0 | -498.6 | |
| 0.00 | 4.24 | 0.00 | 2.34 | -17.11 | 241.55 | 11.46 | 205.67 | 0.4402 | -541.0 | -722.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -17.13 | 241.23 | 11.14 | 205.01 | 0.4384 | -792.0 | -624.3 | |
| 0.00 | 2.62 | 0.00 | 1.44 | -17.18 | 240.42 | 10.33 | 203.36 | 0.4339 | -558.0 | -628.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -17.81 | 240.39 | 10.30 | 202.71 | 0.4428 | -721.0 | -522.7 | |
| 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. | |