| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.72 | 88.14 | 18.83 | 58.02 | 19.10 | 170.67 | -37.84 | 61.90 | 0.6594 | -103.1 | 188.1 | |
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back to the solar disc SDO HMI 2011-11-27 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.88 | 0.00 | 1.21 | 18.76 | 172.05 | -36.46 | 61.65 | 0.6416 | -764.0 | -723.5 | |
| 1.54 | 45.14 | 1.00 | 29.40 | 18.98 | 171.64 | -36.86 | 61.57 | 0.6475 | -509.9 | 91.5 | |
| 8.12 | -2.00 | 5.25 | -2.00 | 18.51 | 171.72 | -36.78 | 62.20 | 0.6443 | -842.7 | 999999 | |
| 1.71 | 4.62 | 1.12 | 3.02 | 19.63 | 171.24 | -37.27 | 60.86 | 0.6554 | -583.4 | -669.1 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 20.34 | 171.04 | -37.47 | 59.96 | 0.6613 | -613.0 | -477.1 | |
| 8.89 | -2.00 | 5.80 | -2.00 | 19.13 | 171.21 | -37.30 | 61.58 | 0.6533 | -543.8 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.80 | 20.52 | 170.42 | -38.09 | 60.04 | 0.6692 | 693.0 | 508.2 | |
| 0.00 | 1.28 | 0.00 | 0.85 | 20.33 | 170.36 | -38.15 | 60.34 | 0.6690 | 519.0 | 467.7 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 19.02 | 170.29 | -38.22 | 62.21 | 0.6635 | 727.0 | 611.0 | |
| 1.45 | 22.06 | 0.97 | 14.72 | 19.11 | 169.86 | -38.65 | 62.30 | 0.6688 | 836.1 | 434.6 | |
| 6.41 | -10.00 | 4.29 | -10.00 | 19.48 | 169.60 | -38.91 | 61.92 | 0.6735 | 749.7 | 999999 | |
| 0.60 | 8.46 | 0.40 | 5.68 | 18.69 | 168.93 | -39.58 | 63.34 | 0.6777 | 667.0 | 518.1 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 20.49 | 167.98 | -40.53 | 61.32 | 0.6963 | 556.0 | 427.8 | |
| 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. | |