SDO HMI 2014-11-28 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.27 | 41.68 | 3.96 | 22.55 | 17.32 | 151.58 | 17.73 | 313.79 | 0.4042 | 57.4 | -187.7 | |
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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 | 0.56 | 18.05 | 153.64 | 19.79 | 312.08 | 0.4356 | 899.0 | 832.2 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 18.24 | 153.63 | 19.78 | 312.43 | 0.4373 | 457.0 | 401.9 | |
| 3.34 | 10.09 | 1.83 | 5.53 | 17.96 | 153.23 | 19.38 | 312.48 | 0.4299 | 928.1 | 753.9 | |
| 0.68 | -3.00 | 0.38 | -3.00 | 18.08 | 153.12 | 19.27 | 312.87 | 0.4298 | 746.8 | 999999 | |
| 0.43 | 2.65 | 0.23 | 1.45 | 18.09 | 152.59 | 18.74 | 313.64 | 0.4238 | 937.6 | 746.2 | |
| 0.51 | 1.63 | 0.28 | 0.88 | 16.37 | 151.63 | 17.78 | 311.84 | 0.3949 | 637.3 | 485.8 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 16.03 | 151.53 | 17.68 | 311.32 | 0.3904 | 592.0 | 575.1 | |
| 0.00 | 2.57 | 0.00 | 1.38 | 16.68 | 150.91 | 17.06 | 313.58 | 0.3897 | -752.0 | -595.1 | |
| 1.28 | 10.09 | 0.69 | 5.41 | 16.32 | 150.75 | 16.90 | 313.12 | 0.3839 | -1060.7 | -812.1 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 17.48 | 150.86 | 17.01 | 315.19 | 0.3977 | -776.0 | -625.0 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 18.35 | 150.75 | 16.90 | 316.94 | 0.4060 | -827.0 | -551.0 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 17.46 | 150.50 | 16.65 | 315.72 | 0.3933 | -735.0 | -579.8 | |
| 0.00 | 3.08 | 0.00 | 1.67 | 18.38 | 150.53 | 16.68 | 317.37 | 0.4039 | -606.0 | -618.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 16.60 | 150.26 | 16.41 | 314.48 | 0.3812 | -765.0 | -658.8 | |
| 1.03 | 2.74 | 0.55 | 1.47 | 17.43 | 149.88 | 16.04 | 316.72 | 0.3861 | -975.7 | -770.5 | |
| 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. | |