SDO HMI 2014-10-08 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.50 | 0.00 | 12.51 | 10.83 | 97.82 | 10.94 | 253.97 | 0.2405 | -258.7 | -184.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.50 | 9.50 | 103.81 | 16.93 | 281.84 | 0.2948 | -877.0 | -631.5 | |
| 0.00 | 2.63 | 0.00 | 1.36 | 8.94 | 103.62 | 16.74 | 280.02 | 0.2903 | -889.0 | -754.0 | |
| 0.00 | 3.42 | 0.00 | 1.77 | 8.67 | 103.36 | 16.48 | 279.23 | 0.2854 | -1093.0 | -728.9 | |
| 0.00 | 4.74 | 0.00 | 2.44 | 9.33 | 102.54 | 15.66 | 281.99 | 0.2735 | 954.0 | 772.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 10.09 | 100.15 | 13.27 | 286.89 | 0.2373 | -972.0 | -816.8 | |
| 0.00 | 2.11 | 0.00 | 1.07 | 10.39 | 98.70 | 11.82 | 290.01 | 0.2154 | -611.0 | -758.7 | |
| 0.00 | 2.02 | 0.00 | 1.02 | 10.06 | 98.66 | 11.78 | 288.59 | 0.2130 | -1036.0 | -811.5 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 10.55 | 98.24 | 11.36 | 291.42 | 0.2090 | -826.0 | -627.4 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 9.49 | 97.37 | 10.49 | 287.67 | 0.1893 | -890.0 | -747.4 | |
| 0.00 | 1.05 | 0.00 | 0.52 | 8.34 | 92.38 | 5.50 | 290.71 | 0.1018 | -861.0 | -605.0 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 14.88 | 87.15 | 0.27 | 358.25 | 0.1496 | 918.0 | 646.4 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 15.09 | 84.20 | -2.68 | 16.47 | 0.1598 | 915.0 | 788.8 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 14.75 | 84.18 | -2.71 | 17.27 | 0.1545 | 909.0 | 796.0 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 22.59 | 78.64 | -8.24 | 25.18 | 0.3122 | 737.0 | 612.5 | |
| 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. | |