SDO HMI 2011-07-02 20:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.81 | 38.96 | 5.94 | 21.44 | 15.96 | 24.37 | 22.55 | 301.75 | 0.4363 | -179.2 | -312.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.66 | 13.28 | 26.85 | 25.04 | 293.96 | 0.4526 | 881.0 | 783.3 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 12.74 | 26.04 | 24.22 | 293.43 | 0.4379 | -686.0 | -479.0 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 15.46 | 25.55 | 23.73 | 299.52 | 0.4477 | -721.0 | -580.8 | |
| 0.00 | 0.82 | 0.00 | 0.47 | 21.66 | 26.27 | 24.46 | 310.10 | 0.5050 | -681.0 | -493.2 | |
| 0.00 | 4.27 | 0.00 | 2.35 | 15.15 | 25.10 | 23.28 | 299.33 | 0.4395 | -898.0 | -826.4 | |
| 0.00 | 7.63 | 0.00 | 4.19 | 14.69 | 25.05 | 23.23 | 298.41 | 0.4356 | -917.0 | -719.5 | |
| 6.72 | 8.08 | 3.70 | 4.45 | 15.41 | 24.86 | 23.04 | 300.09 | 0.4379 | -982.4 | -863.8 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 21.64 | 25.59 | 23.77 | 310.80 | 0.4970 | -558.0 | -480.1 | |
| 3.18 | 5.18 | 1.75 | 2.86 | 17.27 | 24.26 | 22.44 | 304.44 | 0.4439 | 805.3 | 680.0 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 16.33 | 24.11 | 22.29 | 302.74 | 0.4345 | 562.0 | 459.1 | |
| 0.00 | 2.27 | 0.00 | 1.24 | 16.20 | 22.79 | 20.98 | 303.94 | 0.4161 | -937.0 | -749.0 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 17.52 | 20.84 | 19.02 | 309.17 | 0.4026 | 727.0 | 573.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 18.03 | 20.76 | 18.94 | 310.29 | 0.4064 | 873.0 | 738.6 | |
| 0.91 | 2.27 | 0.49 | 1.22 | 16.81 | 20.32 | 18.51 | 308.41 | 0.3894 | 917.0 | 782.2 | |
| 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. | |