SDO HMI 2011-05-31 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.46 | 112.07 | 14.03 | 64.75 | 16.24 | 40.93 | -26.11 | 55.30 | 0.5150 | -330.4 | -126.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.47 | 19.53 | 42.91 | -24.13 | 48.11 | 0.5196 | 693.0 | 587.0 | |
| 19.41 | 74.58 | 11.05 | 42.45 | 16.10 | 42.50 | -24.54 | 54.10 | 0.4946 | -1130.4 | -380.3 | |
| 2.98 | 4.61 | 1.71 | 2.64 | 15.22 | 41.25 | -25.79 | 56.86 | 0.5033 | -856.1 | -679.7 | |
| 0.00 | 5.78 | 0.00 | 3.34 | 15.82 | 40.68 | -26.36 | 56.38 | 0.5151 | -883.0 | -709.4 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 15.92 | 40.38 | -26.66 | 56.49 | 0.5195 | -634.0 | -449.6 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 16.30 | 40.25 | -26.78 | 55.97 | 0.5239 | -503.0 | -416.3 | |
| 0.00 | 1.81 | 0.00 | 1.06 | 15.17 | 38.42 | -28.62 | 59.44 | 0.5389 | 232.0 | 340.1 | |
| 0.00 | 6.86 | 0.00 | 4.10 | 17.24 | 37.80 | -29.24 | 56.61 | 0.5609 | 860.0 | 777.5 | |
| 0.81 | 4.79 | 0.49 | 2.91 | 16.78 | 35.78 | -31.26 | 58.91 | 0.5823 | 996.9 | 785.8 | |
| 0.00 | 2.26 | 0.00 | 1.38 | 17.16 | 35.71 | -31.33 | 58.38 | 0.5856 | 656.0 | 599.4 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 15.95 | 35.74 | -31.29 | 60.23 | 0.5776 | 821.0 | 567.0 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 16.72 | 35.42 | -31.62 | 59.27 | 0.5863 | 782.0 | 636.6 | |
| 0.00 | 1.72 | 0.00 | 1.05 | 16.94 | 35.26 | -31.77 | 59.04 | 0.5896 | 749.0 | 569.9 | |
| 1.26 | 1.44 | 0.78 | 0.89 | 16.98 | 35.07 | -31.97 | 59.13 | 0.5921 | 589.5 | 550.0 | |
| 0.00 | 2.08 | 0.00 | 1.28 | 17.17 | 35.00 | -32.04 | 58.89 | 0.5942 | 637.0 | 506.2 | |
| 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. | |