SDO HMI 2014-11-29 14:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.13 | 30.45 | 3.21 | 18.66 | 16.56 | 152.20 | 33.17 | 297.24 | 0.5919 | 4.4 | 118.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.93 | 6.16 | 2.49 | 3.90 | 17.21 | 154.73 | 35.70 | 296.75 | 0.6266 | 845.0 | 589.1 | |
| 0.00 | 2.05 | 0.00 | 1.26 | 15.48 | 153.02 | 33.99 | 295.03 | 0.5969 | 868.0 | 690.8 | |
| 0.00 | 3.68 | 0.00 | 2.25 | 15.54 | 152.59 | 33.56 | 295.38 | 0.5917 | 770.0 | 756.4 | |
| 0.00 | 1.28 | 0.00 | 0.78 | 15.45 | 152.20 | 33.18 | 295.46 | 0.5864 | 856.0 | 661.2 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 16.77 | 152.27 | 33.24 | 297.50 | 0.5940 | 682.0 | 500.8 | |
| 0.00 | 3.68 | 0.00 | 2.25 | 16.47 | 152.17 | 33.15 | 297.08 | 0.5912 | 579.0 | 507.5 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 15.89 | 151.15 | 32.12 | 296.80 | 0.5752 | -528.0 | -332.8 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 17.22 | 151.07 | 32.04 | 298.96 | 0.5815 | -876.0 | -642.3 | |
| 0.00 | 1.97 | 0.00 | 1.18 | 15.84 | 150.59 | 31.57 | 297.06 | 0.5678 | -573.0 | -385.1 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 17.07 | 150.82 | 31.80 | 298.89 | 0.5775 | -482.0 | -460.1 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 17.50 | 150.69 | 31.66 | 299.67 | 0.5784 | -390.0 | -412.4 | |
| 1.20 | 2.56 | 0.72 | 1.54 | 16.52 | 150.43 | 31.40 | 298.27 | 0.5694 | -809.4 | -681.0 | |
| 0.00 | 1.71 | 0.00 | 1.03 | 17.35 | 150.47 | 31.45 | 299.57 | 0.5748 | -758.0 | -605.6 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 17.26 | 150.31 | 31.29 | 299.54 | 0.5722 | -900.0 | -758.3 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 17.78 | 150.38 | 31.35 | 300.33 | 0.5762 | -698.0 | -490.0 | |
| 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. | |