| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.22 | 455.48 | 49.53 | 249.92 | -17.78 | 352.23 | -19.16 | 133.51 | 0.4329 | 1077.4 | 438.2 | |
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back to the solar disc SDO HMI 2011-12-12 17:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.55 | -17.43 | 354.92 | -16.48 | 137.06 | 0.3989 | 779.0 | 606.8 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -16.32 | 354.79 | -16.60 | 134.79 | 0.3881 | -711.0 | -504.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -11.59 | 354.64 | -16.75 | 124.19 | 0.3429 | 709.0 | 569.3 | |
| 16.85 | 442.36 | 9.29 | 242.69 | -18.72 | 352.43 | -18.96 | 135.44 | 0.4404 | 1166.1 | 455.4 | |
| 60.60 | -4.00 | 33.19 | -4.00 | -17.48 | 352.34 | -19.05 | 133.15 | 0.4285 | 1400.7 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -18.35 | 351.88 | -19.51 | 134.01 | 0.4426 | 629.0 | 507.9 | |
| 2.98 | -4.00 | 1.65 | -4.00 | -18.85 | 351.66 | -19.73 | 134.54 | 0.4502 | 763.1 | 999999 | |
| 7.06 | -4.00 | 3.90 | -4.00 | -18.01 | 351.66 | -19.73 | 133.11 | 0.4417 | 784.6 | 999999 | |
| 1.11 | -4.00 | 0.61 | -4.00 | -17.42 | 351.63 | -19.76 | 132.03 | 0.4362 | 790.5 | 999999 | |
| 1.62 | -4.00 | 0.89 | -4.00 | -17.24 | 351.65 | -19.74 | 131.72 | 0.4341 | 768.3 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -17.85 | 350.95 | -20.44 | 131.88 | 0.4483 | 572.0 | 394.8 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -19.28 | 350.67 | -20.72 | 133.93 | 0.4656 | 755.0 | 592.7 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -21.32 | 350.21 | -21.18 | 136.54 | 0.4913 | 694.0 | 527.5 | |
| 0.00 | 2.64 | 0.00 | 1.45 | -15.30 | 350.58 | -20.81 | 126.68 | 0.4291 | -885.0 | -706.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -17.32 | 349.96 | -21.44 | 129.66 | 0.4551 | -892.0 | -734.9 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -19.61 | 345.75 | -25.64 | 128.77 | 0.5250 | -323.0 | -354.0 | |
| 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. | |