| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.12 | 270.83 | 38.61 | 201.19 | 17.45 | 223.04 | -46.41 | 68.09 | 0.7470 | -697.0 | -200.3 | |
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back to the solar disc SDO HMI 2011-11-23 03:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.70 | 18.64 | 223.36 | -46.09 | 66.45 | 0.7469 | -572.0 | -405.3 | |
| 40.03 | 243.42 | 29.50 | 180.22 | 17.40 | 223.42 | -46.03 | 68.05 | 0.7428 | -1051.3 | -263.1 | |
| 9.34 | -2.00 | 7.03 | -2.00 | 17.94 | 222.43 | -47.03 | 67.66 | 0.7549 | -590.6 | 999999 | |
| 1.29 | 2.31 | 0.98 | 1.76 | 18.73 | 221.95 | -47.50 | 66.78 | 0.7621 | -293.9 | -284.6 | |
| 0.00 | 1.20 | 0.00 | 0.91 | 17.98 | 221.72 | -47.73 | 67.81 | 0.7625 | -361.0 | -182.6 | |
| 0.00 | 1.37 | 0.00 | 1.07 | 19.80 | 220.74 | -48.72 | 65.80 | 0.7774 | 771.0 | 532.1 | |
| 1.46 | 13.54 | 1.10 | 10.28 | 16.54 | 221.84 | -47.61 | 69.63 | 0.7575 | -244.3 | 274.4 | |
| 0.00 | 2.14 | 0.00 | 1.61 | 15.87 | 222.01 | -47.44 | 70.46 | 0.7541 | 515.0 | 518.4 | |
| 0.00 | 1.03 | 0.00 | 0.78 | 16.17 | 221.87 | -47.58 | 70.10 | 0.7564 | -325.0 | -276.1 | |
| 0.00 | 1.11 | 0.00 | 0.86 | 16.17 | 220.80 | -48.65 | 70.37 | 0.7678 | 703.0 | 607.4 | |
| 0.00 | 0.86 | 0.00 | 0.67 | 16.38 | 220.31 | -49.14 | 70.23 | 0.7734 | 671.0 | 629.6 | |
| 0.00 | 1.37 | 0.00 | 1.10 | 17.55 | 219.11 | -50.34 | 69.05 | 0.7882 | 641.0 | 581.3 | |
| 0.00 | 1.54 | 0.00 | 1.23 | 17.24 | 219.13 | -50.32 | 69.43 | 0.7874 | 493.0 | 503.2 | |
| 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. | |