SDO HMI 2011-06-28 18:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.27 | 23.06 | 5.57 | 28.91 | 16.70 | 349.43 | -66.44 | 72.88 | 0.9187 | -60.9 | -9.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 1.03 | 17.17 | 355.30 | -60.58 | 71.78 | 0.8780 | -308.0 | -267.5 | |
| 0.00 | 2.27 | 0.00 | 2.44 | 16.22 | 353.74 | -62.13 | 73.03 | 0.8893 | -601.0 | -505.6 | |
| 0.73 | 1.82 | 0.78 | 1.95 | 15.93 | 353.63 | -62.24 | 73.37 | 0.8900 | -388.9 | -437.4 | |
| 0.00 | 1.54 | 0.00 | 1.68 | 15.79 | 353.36 | -62.51 | 73.55 | 0.8919 | -322.0 | -246.7 | |
| 0.00 | 1.00 | 0.00 | 1.09 | 15.44 | 353.27 | -62.60 | 73.95 | 0.8923 | -308.0 | -201.4 | |
| 0.00 | 1.00 | 0.00 | 1.12 | 15.91 | 352.37 | -63.50 | 73.51 | 0.8993 | -459.0 | -412.7 | |
| 0.00 | 1.45 | 0.00 | 1.70 | 16.53 | 351.19 | -64.68 | 72.94 | 0.9082 | -500.0 | -422.9 | |
| 1.36 | 1.63 | 1.62 | 1.95 | 16.71 | 350.78 | -65.09 | 72.79 | 0.9112 | -285.5 | -314.0 | |
| 0.00 | 1.00 | 0.00 | 1.27 | 17.79 | 349.15 | -66.72 | 71.75 | 0.9226 | -305.0 | -228.6 | |
| 0.00 | 0.73 | 0.00 | 0.90 | 14.58 | 349.63 | -66.25 | 75.20 | 0.9179 | 637.0 | 572.0 | |
| 0.00 | 1.09 | 0.00 | 1.41 | 15.00 | 348.55 | -67.32 | 74.81 | 0.9251 | 269.0 | 210.9 | |
| 2.18 | 6.26 | 3.17 | 9.09 | 17.56 | 345.91 | -69.96 | 72.24 | 0.9419 | 408.8 | 388.5 | |
| 0.00 | 1.00 | 0.00 | 1.43 | 16.94 | 346.34 | -69.53 | 72.87 | 0.9392 | 355.0 | 411.5 | |
| 0.00 | 1.27 | 0.00 | 1.85 | 17.30 | 345.85 | -70.02 | 72.52 | 0.9422 | 3.0 | 166.6 | |
| 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. | |