| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.78 | 45.23 | 5.03 | 23.23 | 17.23 | 314.49 | -1.67 | 5.66 | 0.2669 | -509.2 | -561.9 | |
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back to the solar disc SDO HMI 2011-11-19 14:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 0.88 | 17.88 | 318.10 | 1.94 | 353.15 | 0.2709 | -768.0 | -669.8 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 18.19 | 317.32 | 1.16 | 355.96 | 0.2748 | -720.0 | -575.5 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.00 | 317.26 | 1.10 | 356.14 | 0.2716 | -843.0 | -704.4 | |
| 6.69 | 19.64 | 3.44 | 10.10 | 17.91 | 316.85 | 0.69 | 357.55 | 0.2697 | -1092.6 | -743.7 | |
| 0.00 | 2.66 | 0.00 | 1.34 | 13.26 | 316.65 | 0.49 | 357.46 | 0.1902 | -814.0 | -749.6 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 11.51 | 315.90 | -0.26 | 1.63 | 0.1600 | -800.0 | -695.8 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 17.54 | 315.55 | -0.61 | 2.23 | 0.2634 | -886.0 | -721.0 | |
| 3.09 | 3.69 | 1.59 | 1.90 | 18.19 | 315.05 | -1.11 | 3.87 | 0.2748 | 959.0 | 758.7 | |
| 0.00 | 1.80 | 0.00 | 0.92 | 16.47 | 311.81 | -4.35 | 16.60 | 0.2557 | -949.0 | -716.4 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 16.28 | 311.51 | -4.65 | 17.92 | 0.2543 | -1162.0 | -932.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.20 | 311.36 | -4.80 | 17.32 | 0.2698 | -771.0 | -563.9 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 17.05 | 311.33 | -4.83 | 17.60 | 0.2674 | -938.0 | -729.5 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 18.20 | 308.57 | -7.59 | 24.65 | 0.3022 | -890.0 | -681.7 | |
| 0.00 | 1.37 | 0.00 | 0.70 | 14.62 | 306.92 | -9.24 | 36.12 | 0.2648 | 872.0 | 579.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.99 | 306.29 | -9.87 | 29.48 | 0.3310 | -749.0 | -588.0 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 15.97 | 305.20 | -10.96 | 37.74 | 0.3000 | 774.0 | 601.0 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 18.31 | 302.95 | -13.21 | 38.16 | 0.3526 | 679.0 | 444.3 | |
| 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. | |