SDO HMI 2011-06-12 14:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.61 | 33.97 | 4.88 | 19.21 | -15.75 | 246.12 | -23.76 | 126.38 | 0.4813 | 25.0 | 194.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 3.08 | 0.25 | 1.69 | -15.43 | 250.28 | -19.60 | 130.58 | 0.4274 | 892.0 | 829.3 | |
| 4.08 | 4.71 | 2.23 | 2.58 | -15.28 | 250.07 | -19.82 | 129.98 | 0.4286 | 969.9 | 714.9 | |
| 0.00 | 6.79 | 0.00 | 3.72 | -15.06 | 249.85 | -20.03 | 129.28 | 0.4291 | 982.0 | 848.6 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -15.22 | 249.43 | -20.45 | 129.02 | 0.4357 | 692.0 | 496.2 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -14.80 | 245.11 | -24.78 | 123.26 | 0.4865 | 777.0 | 556.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -15.27 | 244.77 | -25.11 | 123.76 | 0.4945 | 624.0 | 399.2 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -18.89 | 243.77 | -26.11 | 128.72 | 0.5358 | 593.0 | 514.1 | |
| 0.00 | 2.17 | 0.00 | 1.25 | -15.60 | 243.32 | -26.56 | 122.94 | 0.5152 | -848.0 | -681.2 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -15.66 | 242.92 | -26.96 | 122.69 | 0.5208 | -817.0 | -663.8 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -15.98 | 242.80 | -27.08 | 123.11 | 0.5245 | -764.0 | -551.6 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -15.70 | 242.38 | -27.50 | 122.27 | 0.5278 | -876.0 | -731.9 | |
| 4.08 | 5.07 | 2.40 | 2.99 | -16.72 | 241.72 | -28.16 | 123.37 | 0.5433 | -850.6 | -649.1 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -16.15 | 241.78 | -28.11 | 122.48 | 0.5385 | -474.0 | -479.5 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -16.37 | 241.60 | -28.29 | 122.69 | 0.5424 | -703.0 | -466.9 | |
| 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. | |