SDO HMI 2014-11-10 23:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.40 | 0.00 | 10.89 | -24.18 | 7.51 | 3.00 | 186.26 | 0.4689 | 379.4 | 409.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.52 | -22.38 | 10.00 | 5.49 | 191.53 | 0.4447 | 852.0 | 671.9 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -22.31 | 9.64 | 5.13 | 190.83 | 0.4425 | 850.0 | 679.2 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -23.20 | 9.38 | 4.88 | 189.92 | 0.4555 | 752.0 | 624.1 | |
| 0.00 | 1.46 | 0.00 | 0.83 | -24.91 | 9.15 | 4.64 | 188.82 | 0.4809 | 709.0 | 578.1 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -23.73 | 8.98 | 4.47 | 188.91 | 0.4626 | 711.0 | 673.4 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -24.43 | 8.97 | 4.46 | 188.65 | 0.4733 | 845.0 | 697.1 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.84 | 8.92 | 4.41 | 188.41 | 0.4793 | 674.0 | 608.1 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -24.70 | 8.91 | 4.41 | 188.45 | 0.4772 | 729.0 | 565.6 | |
| 0.00 | 3.27 | 0.00 | 1.83 | -23.96 | 8.82 | 4.32 | 188.53 | 0.4658 | 794.0 | 773.2 | |
| 0.00 | 1.55 | 0.00 | 0.87 | -23.79 | 8.59 | 4.08 | 188.13 | 0.4627 | 814.0 | 692.9 | |
| 0.00 | 1.55 | 0.00 | 0.84 | -20.85 | 5.45 | 0.95 | 182.16 | 0.4120 | -721.0 | -521.6 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -25.29 | 4.69 | 0.19 | 180.35 | 0.4814 | -474.0 | -400.6 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.35 | 1.56 | -2.94 | 174.26 | 0.4691 | -653.0 | -519.2 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -33.80 | 354.97 | -9.53 | 167.15 | 0.6211 | -571.0 | -443.4 | |
| 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. | |