SDO HMI 2011-05-31 09:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.32 | 214.72 | 29.07 | 177.53 | 16.80 | 20.60 | -50.85 | 68.16 | 0.8012 | -566.8 | -158.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 1.05 | 21.48 | 21.98 | -49.47 | 62.11 | 0.8025 | -508.0 | -454.1 | |
| 0.00 | 1.81 | 0.00 | 1.48 | 20.34 | 21.99 | -49.46 | 63.47 | 0.7987 | -453.0 | -404.6 | |
| 0.00 | 1.08 | 0.00 | 0.92 | 20.03 | 20.34 | -51.11 | 64.39 | 0.8131 | -415.0 | -313.5 | |
| 0.00 | 3.25 | 0.00 | 2.65 | 17.28 | 21.33 | -50.12 | 67.38 | 0.7960 | -342.0 | -169.2 | |
| 31.26 | 180.40 | 25.24 | 145.85 | 16.51 | 21.56 | -49.89 | 68.25 | 0.7917 | -861.5 | -249.6 | |
| 0.00 | 0.81 | 0.00 | 0.69 | 18.58 | 19.79 | -51.66 | 66.29 | 0.8142 | -420.0 | -308.0 | |
| 0.00 | 1.08 | 0.00 | 1.02 | 19.11 | 15.77 | -55.68 | 66.79 | 0.8511 | 612.0 | 550.4 | |
| 0.00 | 1.45 | 0.00 | 1.36 | 18.92 | 15.70 | -55.75 | 67.03 | 0.8513 | 554.0 | 457.9 | |
| 0.00 | 1.63 | 0.00 | 1.59 | 19.45 | 14.36 | -57.09 | 66.76 | 0.8635 | 236.0 | 179.1 | |
| 0.00 | 2.17 | 0.00 | 2.04 | 17.35 | 15.26 | -56.19 | 68.94 | 0.8519 | 651.0 | 568.5 | |
| 0.00 | 2.80 | 0.00 | 2.66 | 17.80 | 14.93 | -56.52 | 68.50 | 0.8556 | 680.0 | 562.6 | |
| 1.26 | 13.19 | 1.22 | 12.68 | 18.06 | 14.50 | -56.95 | 68.30 | 0.8597 | 426.0 | 421.7 | |
| 2.80 | 3.79 | 2.61 | 3.54 | 16.04 | 15.22 | -56.23 | 70.46 | 0.8498 | -579.9 | -440.5 | |
| 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. | |