| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.27 | 60.99 | 8.55 | 32.08 | 4.70 | 157.85 | -19.36 | 80.52 | 0.3364 | 51.3 | -68.7 | |
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back to the solar disc SDO HMI 2014-11-25 04:00:26 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.97 | 4.20 | 1.02 | 2.17 | 4.04 | 160.39 | -16.81 | 81.50 | 0.2931 | -1213.2 | -859.5 | |
| 3.08 | 4.63 | 1.60 | 2.40 | 4.31 | 160.26 | -16.94 | 80.67 | 0.2958 | -1074.9 | -773.0 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 4.27 | 159.70 | -17.50 | 81.04 | 0.3050 | -859.0 | -679.3 | |
| 0.00 | 9.34 | 0.00 | 4.86 | 4.27 | 159.49 | -17.72 | 81.15 | 0.3086 | -846.0 | -794.9 | |
| 0.94 | 2.91 | 0.49 | 1.52 | 4.98 | 159.16 | -18.05 | 79.06 | 0.3158 | -1021.1 | -832.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 5.36 | 158.64 | -18.56 | 78.17 | 0.3253 | -932.0 | -649.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 4.56 | 158.35 | -18.85 | 80.75 | 0.3278 | 836.0 | 626.6 | |
| 1.28 | 7.20 | 0.67 | 3.77 | 5.21 | 158.24 | -18.97 | 78.84 | 0.3314 | -972.5 | -731.3 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 4.50 | 158.07 | -19.13 | 81.06 | 0.3323 | 752.0 | 557.0 | |
| 0.51 | 1.54 | 0.27 | 0.81 | 5.30 | 157.83 | -19.38 | 78.81 | 0.3383 | -778.2 | -640.2 | |
| 3.26 | 7.11 | 1.72 | 3.77 | 5.82 | 156.77 | -20.44 | 77.86 | 0.3569 | 1059.6 | 869.2 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 4.78 | 156.48 | -20.72 | 80.88 | 0.3587 | 861.0 | 620.8 | |
| 1.80 | 3.43 | 0.95 | 1.82 | 5.14 | 156.41 | -20.80 | 79.93 | 0.3608 | 996.0 | 789.5 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 4.39 | 156.15 | -21.06 | 82.07 | 0.3634 | 1040.0 | 754.7 | |
| 0.77 | 1.97 | 0.41 | 1.05 | 4.15 | 155.99 | -21.21 | 82.77 | 0.3654 | 960.2 | 834.3 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 4.30 | 155.89 | -21.31 | 82.40 | 0.3673 | 785.0 | 708.5 | |
| 2.66 | 9.68 | 1.42 | 5.17 | 4.24 | 155.45 | -21.76 | 82.70 | 0.3743 | 958.6 | 775.9 | |
| 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. | |