| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.76 | 189.22 | 23.68 | 124.83 | 14.40 | 251.99 | 39.63 | 290.51 | 0.6618 | -603.9 | -283.5 | |
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back to the solar disc SDO HMI 2011-11-27 11:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.28 | 176.21 | 22.05 | 116.81 | 14.28 | 252.42 | 40.06 | 290.14 | 0.6667 | -1069.4 | -331.4 | |
| 2.48 | -1.00 | 1.63 | -1.00 | 14.50 | 251.79 | 39.43 | 290.70 | 0.6597 | -870.9 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 17.16 | 251.66 | 39.30 | 294.62 | 0.6680 | -587.0 | -443.9 | |
| 0.00 | 1.20 | 0.00 | 0.80 | 17.32 | 251.66 | 39.30 | 294.84 | 0.6686 | -462.0 | -375.6 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 17.44 | 251.57 | 39.21 | 295.06 | 0.6681 | -628.0 | -423.5 | |
| 0.00 | 0.68 | 0.00 | 0.45 | 17.02 | 251.26 | 38.90 | 294.58 | 0.6627 | -752.0 | -657.0 | |
| 0.00 | 0.60 | 0.00 | 0.38 | 17.05 | 249.07 | 36.71 | 295.67 | 0.6364 | 570.0 | 517.6 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 17.10 | 245.30 | 32.94 | 297.85 | 0.5901 | 596.0 | 486.8 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 13.57 | 244.32 | 31.96 | 292.65 | 0.5597 | 702.0 | 525.2 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 9.91 | 242.62 | 30.26 | 286.99 | 0.5211 | 646.0 | 541.5 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 10.09 | 242.47 | 30.10 | 287.40 | 0.5196 | 845.0 | 705.5 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 17.83 | 243.51 | 31.14 | 300.20 | 0.5718 | 831.0 | 748.5 | |
| 0.00 | 1.63 | 0.00 | 0.97 | 17.68 | 243.11 | 30.75 | 300.23 | 0.5661 | 810.0 | 700.1 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 17.62 | 242.63 | 30.27 | 300.49 | 0.5597 | 882.0 | 706.8 | |
| 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. | |