SDO HMI 2014-07-06 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.09 | 51.44 | 14.47 | 40.89 | -12.73 | 298.25 | 49.19 | 250.72 | 0.7842 | 84.5 | 23.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.82 | 25.26 | 2.29 | 20.60 | -12.84 | 299.38 | 50.32 | 250.95 | 0.7961 | 732.9 | 600.1 | |
| 1.09 | -1.00 | 0.89 | -1.00 | -13.16 | 299.42 | 50.36 | 250.57 | 0.7973 | 698.9 | 999999 | |
| 1.00 | -1.00 | 0.81 | -1.00 | -13.02 | 299.28 | 50.22 | 250.69 | 0.7956 | 935.3 | 999999 | |
| 6.27 | -1.00 | 5.12 | -1.00 | -13.41 | 299.34 | 50.28 | 250.24 | 0.7972 | 743.3 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.53 | -13.02 | 298.45 | 49.39 | 250.44 | 0.7872 | 260.0 | 284.7 | |
| 3.73 | 8.27 | 2.90 | 6.43 | -11.89 | 297.45 | 48.39 | 251.51 | 0.7737 | -622.6 | -504.1 | |
| 1.09 | 5.09 | 0.85 | 3.98 | -12.84 | 297.50 | 48.44 | 250.34 | 0.7769 | -580.5 | -500.6 | |
| 0.00 | 0.64 | 0.00 | 0.49 | -11.63 | 297.20 | 48.14 | 251.76 | 0.7704 | -458.0 | -420.3 | |
| 0.82 | -7.00 | 0.64 | -7.00 | -12.93 | 297.33 | 48.27 | 250.17 | 0.7755 | -676.3 | 999999 | |
| 0.00 | 0.55 | 0.00 | 0.42 | -12.10 | 297.08 | 48.02 | 251.13 | 0.7704 | -508.0 | -489.5 | |
| 0.00 | 0.73 | 0.00 | 0.57 | -13.62 | 297.09 | 48.03 | 249.23 | 0.7750 | -522.0 | -406.5 | |
| 1.27 | 5.45 | 0.97 | 4.17 | -11.85 | 296.51 | 47.45 | 251.25 | 0.7636 | -636.1 | -528.2 | |
| 0.00 | 3.54 | 0.00 | 2.70 | -12.18 | 296.17 | 47.11 | 250.72 | 0.7610 | -641.0 | -500.1 | |
| 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. | |