SDO HMI 2014-07-02 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 |
| 1.82 | 22.71 | 0.98 | 13.04 | 6.47 | 272.74 | -29.26 | 82.01 | 0.4882 | -33.0 | -162.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.83 | 8.06 | 279.22 | -22.79 | 76.49 | 0.3960 | -550.0 | -496.8 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 4.46 | 279.28 | -22.72 | 85.64 | 0.3879 | -842.0 | -740.8 | |
| 1.82 | 5.00 | 0.98 | 2.69 | 4.67 | 279.21 | -22.80 | 85.10 | 0.3892 | -1022.4 | -870.4 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 4.51 | 278.88 | -23.12 | 85.55 | 0.3944 | -590.0 | -544.5 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 6.34 | 278.67 | -23.33 | 80.99 | 0.4002 | -803.0 | -637.2 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 7.92 | 278.35 | -23.65 | 77.23 | 0.4091 | 699.0 | 544.2 | |
| 0.00 | 3.27 | 0.00 | 1.81 | 5.42 | 275.78 | -26.23 | 83.83 | 0.4443 | -765.0 | -623.1 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 8.89 | 268.79 | -33.21 | 78.41 | 0.5545 | 50.0 | 52.4 | |
| 0.00 | 2.27 | 0.00 | 1.35 | 8.86 | 268.54 | -33.47 | 78.54 | 0.5581 | 641.0 | 529.9 | |
| 0.00 | 1.64 | 0.00 | 0.99 | 9.99 | 267.48 | -34.53 | 76.82 | 0.5754 | 763.0 | 516.8 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 10.83 | 266.57 | -35.43 | 75.65 | 0.5899 | 577.0 | 549.8 | |
| 0.00 | 0.73 | 0.00 | 0.46 | 9.09 | 264.01 | -37.99 | 79.11 | 0.6212 | 497.0 | 496.1 | |
| 0.00 | 1.18 | 0.00 | 0.81 | 1.79 | 258.55 | -43.45 | 90.58 | 0.6898 | 286.0 | 283.5 | |
| 0.00 | 0.64 | 0.00 | 0.51 | 5.54 | 249.67 | -52.33 | 85.32 | 0.7927 | 578.0 | 499.4 | |
| 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. | |