SDO HMI 2014-09-04 19:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.26 | 355.79 | 141.99 | 895.12 | -13.86 | 94.39 | -76.33 | 105.79 | 0.9797 | 62.2 | -83.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.27 | 341.76 | 0.45 | 868.28 | -11.32 | 99.98 | -70.74 | 104.27 | 0.9564 | 573.7 | -83.8 | |
| 0.00 | 1.88 | 0.00 | 2.78 | -6.90 | 101.52 | -69.20 | 99.99 | 0.9438 | 159.0 | 98.2 | |
| 18.49 | -1.00 | 33.01 | -1.00 | -11.91 | 99.03 | -71.69 | 104.68 | 0.9615 | 497.3 | 999999 | |
| 1.43 | 4.29 | 2.63 | 7.88 | -11.64 | 98.40 | -72.32 | 104.28 | 0.9642 | 212.4 | 61.3 | |
| 0.00 | 3.75 | 0.00 | 6.89 | -11.22 | 98.26 | -72.46 | 103.83 | 0.9644 | -219.0 | -168.2 | |
| 1.34 | -1.00 | 2.63 | -1.00 | -12.19 | 97.48 | -73.24 | 104.67 | 0.9686 | 90.8 | 999999 | |
| 0.00 | 1.16 | 0.00 | 2.72 | -14.13 | 95.36 | -75.36 | 106.23 | 0.9781 | 234.0 | 223.7 | |
| 7.05 | -1.00 | 19.06 | -1.00 | -15.37 | 93.88 | -76.85 | 107.20 | 0.9837 | 160.7 | 999999 | |
| 0.00 | 0.80 | 0.00 | 1.91 | -13.97 | 95.14 | -75.58 | 106.02 | 0.9788 | -74.0 | -66.1 | |
| 0.00 | 1.88 | 0.00 | 4.10 | -12.73 | 95.91 | -74.81 | 104.92 | 0.9752 | -577.0 | -511.2 | |
| 0.00 | 0.27 | 0.00 | 0.56 | -11.82 | 96.41 | -74.31 | 104.09 | 0.9726 | 165.0 | 192.7 | |
| 20.45 | -1.00 | 65.67 | -1.00 | -15.10 | 91.94 | -78.78 | 106.59 | 0.9888 | -154.9 | 999999 | |
| 7.23 | -1.00 | 18.54 | -1.00 | -12.30 | 93.85 | -76.87 | 104.11 | 0.9820 | -73.5 | 999999 | |
| 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. | |