| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.12 | 213.99 | 23.75 | 112.61 | 17.17 | 19.97 | 9.20 | 333.10 | 0.3399 | -346.9 | -336.2 | |
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back to the solar disc SDO HMI 2011-06-04 23:59:10 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.24 | 175.89 | 12.25 | 92.67 | 16.82 | 21.15 | 10.38 | 329.55 | 0.3417 | -1253.1 | -502.4 | |
| 5.52 | -1.00 | 2.91 | -1.00 | 17.17 | 21.07 | 10.30 | 330.27 | 0.3460 | -970.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 18.70 | 20.81 | 10.03 | 333.06 | 0.3657 | -779.0 | -599.6 | |
| 5.15 | -1.00 | 2.72 | -1.00 | 17.07 | 20.62 | 9.84 | 331.23 | 0.3410 | -997.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.61 | 16.81 | 6.04 | 341.90 | 0.3240 | -536.0 | -443.3 | |
| 2.89 | 3.71 | 1.52 | 1.94 | 17.99 | 16.60 | 5.82 | 342.86 | 0.3289 | -879.7 | -717.6 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 19.83 | 15.01 | 4.23 | 348.56 | 0.3517 | 778.0 | 617.8 | |
| 0.00 | 3.26 | 0.00 | 1.69 | 16.72 | 14.61 | 3.84 | 347.60 | 0.3000 | 741.0 | 763.1 | |
| 5.61 | 12.48 | 2.94 | 6.54 | 18.60 | 14.56 | 3.78 | 349.04 | 0.3305 | 1035.2 | 698.5 | |
| 2.71 | 3.62 | 1.41 | 1.88 | 17.29 | 14.40 | 3.63 | 348.66 | 0.3086 | 994.6 | 840.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.70 | 14.38 | 3.60 | 349.00 | 0.3153 | 810.0 | 594.5 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 22.34 | 14.49 | 3.71 | 351.14 | 0.3904 | 570.0 | 489.6 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 18.25 | 14.26 | 3.49 | 349.68 | 0.3238 | 1073.0 | 863.3 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 18.96 | 14.18 | 3.41 | 350.31 | 0.3351 | 797.0 | 615.9 | |
| 0.00 | 3.53 | 0.00 | 1.84 | 18.15 | 14.07 | 3.29 | 350.19 | 0.3217 | 743.0 | 768.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 18.63 | 13.92 | 3.14 | 350.88 | 0.3291 | 774.0 | 642.8 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 23.47 | 13.72 | 2.95 | 353.31 | 0.4066 | 755.0 | 529.8 | |
| 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. | |