SDO HMI 2014-11-08 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.27 | 24.04 | 1.73 | 12.85 | -14.48 | 20.68 | -12.40 | 146.92 | 0.3745 | 282.8 | 193.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.53 | -11.74 | 28.41 | -4.67 | 163.21 | 0.2772 | 752.0 | 550.8 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -9.73 | 26.66 | -6.42 | 154.39 | 0.2562 | 658.0 | 422.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -13.99 | 25.11 | -7.98 | 155.93 | 0.3317 | 762.0 | 630.5 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -13.66 | 23.88 | -9.20 | 152.28 | 0.3356 | 900.0 | 666.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -14.54 | 23.16 | -9.92 | 151.74 | 0.3538 | 905.0 | 690.9 | |
| 1.98 | 4.74 | 1.04 | 2.49 | -12.96 | 22.52 | -10.57 | 147.81 | 0.3369 | 1143.0 | 872.6 | |
| 0.00 | 3.45 | 0.00 | 1.82 | -13.21 | 22.29 | -10.79 | 147.66 | 0.3424 | 846.0 | 729.5 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -14.15 | 21.28 | -11.81 | 146.82 | 0.3642 | 749.0 | 587.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -13.97 | 21.22 | -11.86 | 146.42 | 0.3622 | 824.0 | 597.9 | |
| 1.29 | 2.84 | 0.69 | 1.52 | -14.36 | 19.85 | -13.23 | 144.12 | 0.3800 | -1063.2 | -869.6 | |
| 0.00 | 2.50 | 0.00 | 1.38 | -16.31 | 15.87 | -17.21 | 139.93 | 0.4431 | -738.0 | -694.4 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -18.72 | 14.41 | -18.67 | 141.15 | 0.4855 | -867.0 | -632.5 | |
| 0.00 | 1.47 | 0.00 | 0.83 | -19.11 | 14.20 | -18.89 | 141.37 | 0.4920 | -576.0 | -452.5 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -17.67 | 14.13 | -18.95 | 139.27 | 0.4762 | -787.0 | -603.7 | |
| 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. | |