| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.19 | 251.96 | 23.52 | 131.08 | 17.69 | 223.45 | 7.26 | 336.75 | 0.3069 | -625.3 | -379.5 | |
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back to the solar disc SDO HMI 2011-11-27 04:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.44 | 11.14 | 225.16 | 8.97 | 317.88 | 0.2292 | 694.0 | 537.4 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 18.88 | 225.05 | 8.87 | 334.11 | 0.3354 | 726.0 | 483.8 | |
| 16.69 | 220.89 | 8.68 | 114.95 | 17.43 | 224.07 | 7.88 | 334.64 | 0.3069 | -1226.6 | -430.1 | |
| 0.00 | 0.43 | 0.00 | 0.22 | 14.46 | 223.46 | 7.27 | 331.53 | 0.2583 | 744.0 | 604.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.10 | 223.56 | 7.37 | 339.39 | 0.3440 | 960.0 | 698.6 | |
| 26.53 | -3.00 | 13.81 | -3.00 | 17.83 | 223.43 | 7.24 | 337.01 | 0.3086 | -1299.6 | 999999 | |
| 0.34 | 10.44 | 0.18 | 5.43 | 18.39 | 221.94 | 5.76 | 341.94 | 0.3086 | -751.8 | -708.0 | |
| 0.00 | 2.31 | 0.00 | 1.21 | 19.85 | 221.90 | 5.72 | 343.51 | 0.3314 | -817.0 | -691.4 | |
| 0.00 | 2.40 | 0.00 | 1.23 | 15.87 | 221.74 | 5.56 | 339.55 | 0.2678 | 647.0 | 576.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.14 | 221.69 | 5.51 | 338.68 | 0.2560 | 906.0 | 803.4 | |
| 0.00 | 1.88 | 0.00 | 0.97 | 15.41 | 221.61 | 5.42 | 339.37 | 0.2598 | 853.0 | 751.3 | |
| 0.00 | 2.82 | 0.00 | 1.48 | 19.85 | 221.55 | 5.37 | 344.46 | 0.3299 | -948.0 | -713.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.57 | 221.39 | 5.21 | 340.32 | 0.2610 | 962.0 | 749.9 | |
| 1.63 | 1.63 | 0.85 | 0.85 | 19.48 | 221.35 | 5.17 | 344.69 | 0.3230 | -911.4 | 0.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.33 | 220.66 | 4.47 | 345.72 | 0.3017 | 761.0 | 547.1 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.22 | 220.17 | 3.98 | 346.32 | 0.2817 | 673.0 | 481.8 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 18.02 | 220.12 | 3.94 | 347.14 | 0.2946 | 635.0 | 597.7 | |
| 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. | |