SDO HMI 2014-07-04 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.34 | 0.00 | 10.39 | 5.39 | 261.04 | -10.07 | 81.77 | 0.2108 | 742.5 | 615.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.54 | 4.02 | 276.71 | 5.60 | 278.10 | 0.0988 | -946.0 | -737.2 | |
| 0.00 | 4.54 | 0.00 | 2.26 | 8.90 | 269.76 | -1.35 | 13.26 | 0.1017 | 837.0 | 698.3 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -1.87 | 269.13 | -1.98 | 158.77 | 0.0960 | 973.0 | 727.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 2.79 | 267.79 | -3.32 | 97.62 | 0.0587 | 916.0 | 731.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 12.18 | 266.63 | -4.48 | 26.14 | 0.1740 | 916.0 | 763.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 1.53 | 260.32 | -10.79 | 98.76 | 0.1902 | 960.0 | 761.4 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 1.32 | 260.17 | -10.94 | 99.74 | 0.1934 | 958.0 | 719.0 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 1.62 | 260.13 | -10.98 | 98.15 | 0.1931 | 798.0 | 610.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 7.59 | 259.77 | -11.34 | 68.46 | 0.2106 | 945.0 | 607.5 | |
| 0.00 | 2.36 | 0.00 | 1.25 | 5.67 | 250.99 | -20.12 | 82.38 | 0.3469 | 824.0 | 709.3 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 5.87 | 250.39 | -20.72 | 81.99 | 0.3569 | 737.0 | 595.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 4.54 | 249.45 | -21.66 | 85.85 | 0.3705 | 1003.0 | 816.7 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 4.48 | 249.16 | -21.95 | 86.07 | 0.3752 | 731.0 | 643.9 | |
| 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. | |