SDO HMI 2011-06-07 07:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.96 | 117.77 | 19.58 | 79.62 | 17.21 | 19.71 | 39.80 | 295.84 | 0.6810 | -397.3 | -195.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.08 | 0.00 | 2.30 | 20.97 | 24.66 | 44.75 | 298.52 | 0.7505 | -606.0 | -528.5 | |
| 5.61 | 82.83 | 3.87 | 56.83 | 16.88 | 21.35 | 41.44 | 294.57 | 0.6987 | -731.9 | -358.2 | |
| 2.17 | -2.00 | 1.50 | -2.00 | 17.01 | 21.13 | 41.22 | 294.84 | 0.6967 | -671.5 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.58 | 20.22 | 21.84 | 41.93 | 298.82 | 0.7179 | -578.0 | -473.1 | |
| 15.30 | -2.00 | 10.44 | -2.00 | 16.72 | 20.67 | 40.76 | 294.65 | 0.6903 | -925.9 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.51 | 20.74 | 21.40 | 41.49 | 299.70 | 0.7156 | -570.0 | -473.9 | |
| 1.63 | 7.06 | 1.06 | 4.59 | 17.10 | 17.23 | 37.33 | 296.84 | 0.6518 | -862.1 | -708.9 | |
| 0.00 | 0.63 | 0.00 | 0.41 | 18.47 | 15.29 | 35.38 | 299.92 | 0.6359 | 468.0 | 368.1 | |
| 4.25 | 14.57 | 2.71 | 9.28 | 18.03 | 15.15 | 35.24 | 299.36 | 0.6318 | 705.4 | 593.0 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 16.72 | 14.78 | 34.87 | 297.65 | 0.6204 | 651.0 | 571.6 | |
| 0.00 | 3.17 | 0.00 | 2.01 | 17.42 | 14.89 | 34.98 | 298.62 | 0.6255 | 613.0 | 560.3 | |
| 0.00 | 2.72 | 0.00 | 1.74 | 18.99 | 14.94 | 35.03 | 300.88 | 0.6347 | 755.0 | 646.8 | |
| 0.00 | 1.09 | 0.00 | 0.69 | 18.73 | 14.65 | 34.74 | 300.70 | 0.6298 | 817.0 | 703.3 | |
| 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. | |